GIUSEPPE LEONARDI and PAOLO MIETTO (Eds)
THE ITALIAN DINOSAURS
Note that many chapters of this book are here in my page of ResearchGate with full text, abstract and images. Search for chapters of year 2000.
A VERY EXPANDED ABSTRACT IN ENGLISH (THE ORIGINAL TEXT IS IN ITALIAN WITH THIS EXPANDED ABSTRACT AT THE END OF THE BOOK)
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THE JURASSIC TRACKS OF THE LAVINI DI MARCO SITE (ROVERETO, TRENTO PROVINCE) IN THE CONTEST OF THE DINOSAURS OF ITALY
SUMMARIES
FABIO M. DALLA VECCHIA, EDITOR
PART I - Introduction and general data
1 - G. LEONARDI and P. MIETTO - Introduction
2 - G. A. VENZO - Geographic-geologic framing and account of geologic studies and researches on the Lavini di Marco.
3 - A. GORFER - The Lavini di Marco: landscape, history, erudition
4 - S. ABRAM, P. LORENZI and F. PROSSER - Naturalistic and environmental aspects of the Lavini di Marco
5 - D. MASETTI - The geology of the Lavini di Marco
6 - C. BROGLIO LORIGA - Paleontological aspects of the Calcari Grigi formation
7 - G. LEONARDI - Account on the dinosaurs
PART II - The dinosaur tracks in their paleoenvironment
8 - G. LEONARDI and P. MIETTO - The Liassic dinosaur tracks of the Lavini di Marco
9 - M. AVANZINI, S. FRISIA and M. RINALDO - The Lavini di Marco during Early Jurassic: reconstruction of an ancient bioenvironment
PART III - Tetrapod paleontology of Italy and neighbour countries
10 - G. LEONARDI - The dinosaurs of Italy and neighbour countries
11 - M. A. CONTI, G. LEONARDI, P. MIETTO and U. NICOSIA - Footprints of non-dinosaurian tetrapods in the Paleozoic and Mesozoic of Italy
12 - F. M. DALLA VECCHIA - Bone remains of Paleozoic and Mesozoic tetrapods of Italy
PART IV - Other contributions
13 - G. OROMBELLI and U. SAURO - Geomorphological aspects of the landslides of Mt. Zugna
14 - M. AVANZINI and D. ZAMPIERI - The Lavini di Marco: geological-structural aspects
15 - O. GROAZ and L. VERONESE - Historical and instrumental seismicity in the Lagarina Valley
16 - P. ARZARELLO, F. FINOTTI, G. GALEAZZO, M. LANZINGER, M. MEZZANOTTE and L. VERONESE - The Park of the Rovereto dinosaur tracks: preservation, exploitation and “musealization”
ENGLISH TRANSLATION OF SOME ITALIAN TERMS REPORTED IN THE TEXT
Colatoio (pl. colatoi) = natural drainer or gully
Dante Alighieri = Italian poet (1265-1321)
Laste di Lizzana = toponym; “lasta” (pl. laste) is a local word indicating wide, flat, rocky bed surfaces on the flank of a mountain or flat slabs of rock; Lizzana is a village; therefore the literal translation is “wide, flat rocky bed surfaces on the flank of the mountain near Lizzana”.
Laste alte = toponym; topographically high, upper “laste”.
Lavini di Marco = toponym; “lavini” is a local word for “landslide accumulation”, Marco is a small village, therefore its literal translation is “landslide accumulation of Marco”.
Marocche = local name for a mix landslide-moraine
ENGLISH TRANSLATION OF LITHOSTRATIGRAPHIC TERMS
Biancone = Biancone (Big White) Formation
Calcare Massiccio = Massive Limestone Formation
Calcare del Vajont = Vajont Limestone Formation; Vajont is a locality in the Western Carnic Pre-alps near the border between Friuli-Venezia Giulia and Veneto Regions.
Calcare Selcifero = Cherty Limestone Formation
Calcari Grigi (also Calcari Grigi di Noriglio) = Grey Limestone Formation, more correctly Grey Limestone of Noriglio Formation; Noriglio is a small town village near Rovereto.
Corna = Corna (corna= horns) Formation
Dolomia Principale = Main Dolostone Formation, Hauptdolomit of German-speaking Authors.
Membro di Rotzo = Rotzo Member of Grey Limestone Formation, called also Medium Member; Rotzo is a small village of the Sette Comuni (or Asiago) Plateau
Membro Inferiore = Lower Member of Grey Limestone Formation
Membro Medio = Medium Member of Grey Limestone Formation, also called Rotzo Member
Membro Superiore = Upper Member of Grey Limestone Formation
Oolite di Massone = Oolite of Massone Formation; Massone is a village.
Oolite di San Vigilio = Oolite of San Vigilio Formation; San Vigilio is a village.
Rosso Ammonitico Inferiore = Lower Rosso Ammonitico Formation
Rosso Ammonitico Superiore = Upper Rosso Ammonitico Formation
Scaglia Rossa = Red Scaglia Formation
Scaglia Variegata = Variegated Scaglia Formation
Scisti ad Aptici = Shale with Aptychi Formation
Scisti a Fucoidi = Shale with Chondrites Formation
PART I - INTRODUCTION AND GENERAL DATA
1
Giuseppe LEONARDI and Paolo MIETTO
INTRODUCTION
One morning at the end of 1980, Luciano Chemini, an amateur naturalist from Rovereto (in the Province of Trento, Northern Italy), was walking around the steep slopes of Mt Zugna, at Vallon close to the Lavini di Marco. The Lavini di Marco is a chaotic accumulation of debris and boulders at the base of the mountain and are due to a large landslide. The area where Chemini was walking, known is known as the Laste di Lizzana and is a part of the scare caused to the mountain by the landslide. Somewhere, bands of the steep rocky floor (called colatoi=drainers) are cleaned of debris by running water. The low-angled light of the early morning sun emphasized some strange, rounded depressions crossing the colatoio. They were regularly spaced and surrounded by a rim. “These are the footprints of a prehistoric animal”, Chemini thought. This is how the tracks later known as ROLM 9 and the dinosaur tracksite of the Lavini di Marco were discovered.
Chemini reported the discovery to Michele Lanzinger, then curator of the Museo Tridentino di Scienze Naturali of Trento. Many months passed. When an exhibition of Chinese dinosaurs took place at Trento, Michele Lanzinger called upon one of the editors of this volume (Giuseppe Leonardi) to make an inspection of the tracksite. On July 23th 1991 it became clear that the Lavini were full of dinosaur footprints. A preliminary description of the tracks found at the colatoio, now known as colatoio Chemini in honour of the finder, were published in 1992.
The Museo Tridentino di Scienze Naturali of Trento and the Museo Civico of Rovereto immediately acted to protect and study the site. A task force, led by the editors of this volume, was set up to carry out a multidisciplinary and exhaustive study of the site. Systematic fieldwork began in June 1992 and led to the discovery of hundreds of tracks and footprints spread over a very wide area along the flanks of Mt. Zugna. It is a spectacular site, easy to reach and situated in a beautiful natural landscape.
This volume is dedicated to the different aspects of the site, with particular emphasis, of course, on the paleontological and geological (sedimentology but also geomorphology, structural geology and seismicity). Several chapters are dedicated to evidence of other paleoichnological sites in Italy and neighbouring regions, and Italian Paleozoic and Mesozoic tetrapod osteological materials.
It is clear that much more work must be done before we can fully understand the meaning of the Lavini di Marco site.
2
Giulio Antonio VENZO
GEOGRAPHIC-GEOLOGIC FRAMING AND ACCOUNT OF GEOLOGIC STUDIES AND RESEARCHES REGARDING THE LAVINI DI MARCO
Val Lagarina or Vallagarina is the part of the Adige river Valley between Murazzi (12 km south of Trento) and Rivoli Veronese. On its left side from Lizzana (near Rovereto) stretching 6 km southward, there is an accumulation of contiguous, large landslides known as the Lavini. Many researchers use this term not only for the accumulation but also for the whole flank of the mountain where the main landslide originated.
The dinosaur footprints are situated on the wide bed surfaces (laste) exposed by the falling of the overlaying strata. The lithostratigraphic unit is the Liassic Calcari Grigi di Noriglio.
Many scholars wrote about the Lavini and their origins. Most famous is the citation by Dante Alighieri in the canto XII of the Inferno in his Divina Commedia (1314?).
Qual è quella ruina, che nel fianco
di qua da Trento l’'Adice percosse,
o per tremoto o per sostegno manco,
che da cima del monte, onde si mosse,
al piano è sí la roccia discoscesa,
ch'alcuna via darebbe a chi sù fosse:
cotal di quel burrato era la scesa;
……
The poet describes the landslide accumulation and its possible origins, without using the names of localities except for those of the Adige valley and Trento (see the next chapter for the discussion about the actual location of the landslide mentioned by Dante).
Geological studies began in the XIX century and focused on attempts to date and identify the origin of the event that caused the accumulation. Interpretations were different and sometimes bizarre.
The accumulation was considered to be the result of multiple, different events by Canestrini (1922), Sacco (1940), Fuganti (1969), and Perna (1974). According to some authors, it would have destroyed the village of Lagaris (Neumayr, 1889) or Lagare (Montandon, 1933).
The date of the accumulation event/s was believed to be: a) a “long time ago” (Pasini, 1836; Noriller, 1871), b) end of Ice ages (de Mortillet, 1861; Paglia, 1875; De Cobelli, 1877; Suda, 1886; Canestrini, 1922; Fabiani & Trevisan, 1939; Sacco, 1940), c) beginning of the Postglacial (Taramelli, 1881), d) historical times (Gümbel, 1872; Vacek, 1911), e) more events occurring in different ages, the main one during the interglacial Riss-Wurm period, the lesser during the Postglacial (Fuganti, 1969), f) historical times due to the superficial karst corrosion (Heim, 1932), g) uncertain between 833 and 883 A.D. (Schwinner, 1912), h) in 883 A.D. following the Annals of Fulda (von Mojsisovics, 1863; Giovannelli, 1869; Penck, 1886; Neumayr, 1889; Montandon, 1933), i) possibly in 883 A.D. or on 21 July 365 or 369 A.D. (Eisbacher & Clague, 1984), l) more events during different ages, the last in 883 A.D (Perna, 1974).
The origin of the accumulation was identified as the result of two main kinds of events:
1) a landslide a) without particular causes (von Mojsisovics, 1863; Penck, 1886; Neumayr, 1889; Heim, 1932; Montandon, 1933), b) without particular causes but criticizing all other causes reported in literature (Schwinner, 1912), c) caused by the steep franapoggio dip of the stone beds and the presence of marly, plastic levels (Benecke, 1866; Gümbel, 1872; Taramelli, 1881), d) caused by the steep franapoggio dip of the stone beds and an earthquake (Eisbacher & Clague, 1984), e) caused by heavy rains and melting snow in rocks ready to fall as the result of previous earthquakes (Giovannelli, 1869), f) breakage and throwing into the air of the rocks, caused by the rising from the inner of the Earth of an unspecified elastic substance (Noriller, 1871), g) caused in great part by the retreating of the glacier (Canestrini, 1922), h) mixed geomorphological causes (also glacial exaration and fluvial erosion), but no earthquake (Fuganti, 1969), i) caused mainly by the steep franapoggio dip of the stone beds, presence of marly, plastic levels, lesser pressure after the retreat of the glacier, hard rains and earthquakes (Perna, 1974).
2) a mixed landslide-moraine or moraine: a) as a “secondary moraine” (de Mortillet, 1861; Fabiani & Trevisan, 1939; Abele, 1974), b) caused by an earthquake or the undermining of the base of the mountain (as hypothesized by Dante) but reworked by glaciers (Paglia, 1875), c) caused by the steep franapoggio dip of the stone beds, presence of marly, plastic levels and pressure of the glacier, and reworked by the latter (de Cobelli, 1877), d) caused by the steep franapoggio dip of the stone beds, presence of marly, plastic levels, retreat of the glacier, and partial reworking by the latter (Sacco, 1940), e) moraine in general (Suda, 1886)..
The last study of the Lavini was carried out by Orombelli & Sauro (1988), which identifies seven landslides under the name “Lavini di Marco”. In the text they consider only the main landslide as “Lavini di Marco”, the accumulation of which is considered to be formed by two contiguous landslides (Lavini and Gran Ruina). They identify at least two events, the main one which took place in 883 A.D., and another much older landslide that occurred more than 4000 years ago, (see chapter 13).
3
Aldo GORFER
THE LAVINI DI MARCO: LANDSCAPE, HISTORY, ERUDITION
Few natural phenomena in the Alps have been the subject such controversial geologic, historic, philological and literary interpretations as the Lavini di Marco. The descriptions of the Lavini are mostly confined to the interpretation of the causes of the event or to the debate on the probable mention of it in Dante’s Divina Comedia. The Lavini are mentioned by Innocenzo a Prato at the end of the XVI century and considered to be the result of a strong earthquake that took place in 369 A.D. All the sources of the XVII century cited earthquakes as causes of the origin of the Lavini [for more recent mentions, see the preceding chapter]. The site of accumulation of the landslide was an obligatory stop along the “grande route” connecting the Mediterranean with Continental Europe. This position led to its description by many travellers, who include the Englishman Albanis Beaumont who visited the Lavini in 1786, and the Frenchman Mercey.
The name Lavini or Slavini comes from the late Latin word labina which means “landslide”. The toponym (Labino de Marco) already existed in 1270. The oldest iconographic representation of the Lavini is a map drawn in 1438. The area is reported in most other maps that include the areas surrounding Rovereto: the early ones (1785, 1757, 1774, 1800-1801, 1810), were made under the Austro-Hungarian government (1820, 1862-63, 1894 and 1916), those made by the Italian Kingdom (1927 and 1940) and the Italian Republic (1959, 1965 and 1983).
The debate about the interpretation of the meaning of Dante’s citation of a large landslide accumulation (“ruina”) along the Adige river valley, began as early as 1324 and became fierce during the XVIII-XIX centuries. The main topics of the debate were whether the mentioned landslide that of the Lavini or not, what was the cause of it and whether Dante visited the area and when. Nowadays, the identification of Dante’s “ruina” with the Lavini is accepted by the Divina Commedia annotators with prudent reservation. It is generally accepted that Dante visited this part of Italy between 1302 and 1304, and almost definitely before 1308.
4
Sergio ABRAM, Pietro LORENZI and Filippo PROSSER
NATURALISTIC AND ENVIRONMENTAL ASPECTS OF THE LAVINI DI MARCO
The botanical aspects considered here, concerns two main areas: Mt Cengialto and the small lakes of Marco. The rare endemic Iris cengialti was found in the first area. The woods in the area belong to the alleanza Orno-Ostryon and are characterized by manna-ash, carpino nero e roverella.
Several rare species were recently found in the second area. Teucrium scordium, Potamogeton pectinatus, Carex gracilis, Polygonum minus, Bidens frondosa, Catabrosa aquatica, Ranunculus rionii, Veronica anagalloides, Alisma lanceolatum, Alisma gramineum, Sparganium minimum, Polygonum minus, Carex gracilis, Teucrium scordonia, Rorippa amphibia, Gratiola officinalis, Potentilla reptans, Agrostis stolonifera, Myriophyllum verticillatum, Phragmites australis, Typha latifolia and Salix alba can be found here.
At Lavini several extint species are documented: Hornungia petraea, Teucrium botrys, Lychnis viscaria, Minuartia capillacea. Le specie presenti attulmente sono tipiche dell’ambiente carsico Hieracium praealtum, H. tephropogon, H. dollineri, H. illyricum, H. pospichalii, H. pseudopsammogenes, Inula ensifolia, Rhamnus saxatilis, Epimedium alpinum, Hieracium porrifolium, H. illyricum, H. dollineri, Chamaecytisus purpureus, Euphorbia angulata, Salix glabra, Euphrasia tricuspidata. The rare Daphne alpina, a characteristic of the landslide block environment, is particularly abundant here. The alleanza Orno-Ostryon is the final result of the colonization of vegetation in this environment but it is arrived at over a long period of time and only gradually on the unstable landslide ground. The most important plant environments are:
- Potentilletalia caulescentis: vegetation on cliffs, characterized mainly by Potentilla caulescens, Asplenium trichomanes and A. ruta-muraria
- Stipetum calamagrostis: vegetation of the mobile debris.
- Euphrasio tricuspidatae-Selserietum albicantis: new association characterized mainly by Euphrasia tricuspidata and living on small lembi erbosi on rocky ground.
- Cotino-Amelanchieretum ovalis: brush vegetation, mainly made up of Amelanchier ovalis, Cotinus coggygria, Viburnum lantana but also with trees (Pinus sylvestris, Ostrya carpinifolia and Fraxinus ornus). In humid places Frangula alnus and Salix appendiculata are present.
- Vegetazione di margine (Geranietea sanguinei).
- Vegetazione delle aree boscate su marocca and on the "laste": this is the vegetation type that is most difficult to define.
- Woods with Pinus nigra: this species is not autoctonous.
- Woods of the alleanza Tilio-Acerion: present at the talus of old landslides and in narrow, small valleys in the marocche and on cliffs. Consisting of Tilia cordata, Ulmus glabra and Philadelphus coronarius.
- Woods with Carpinus betulus and sometimes Tilia cordata.
- Woods with Quercus cerris and Quercus petraea characteristic of siliceous soils formed of morenic deposits.
Species with altimontana-subalpina distribution (Rhododendron hirsutum, Pinus mugo, Rhamnus pumilus, Senecio rupestris, Polystichum lonchitis, Dentaria enneaphyllos, Dryopteris villarii, Saxifraga caesia, Paederota bonarota, Valeriana saxatilis, Salix retusa, S. reticulata, Mnium orthorhynchum, Myurella julacea, Drepanocladus uncinatus, Huperzia selago, Rhododendron ferrugineum, Vaccinium vitis-idaea, V. myrtillus) are found at a surprisingly low altitude. This phenomenon is known as “dealpinization” and is due to particularly cold local climatic conditions.
A census of the ornithological fauna and the mammalian fauna was done during the years 1988-89. The area of the Lavini is frequented by a lower number of species with respect to nearby areas. The birds of the area are the eagle (Aquila chrysaetos), the short-toed eagle (Circaetus gallicus), the black kite (Milvus migrans), the honey buzzard (Pernis apivorus), the buzzard (Buteo buteo), the sparrowhawk (Accipiter nisus), the hobby (Falco subbuteo), the kestrel (Falco tinnunculus), the eagle owl (Bubo bubo), the long-eared owl (Asio otus), the rock partridge (Alectoris graeca), the hazel grouse (Bonasa bonasia), the black grouse (Tetrao = Lyrurus tetrix), the blue rock thrush (Monticola solitarius), the rock thrush (Monticola saxatilis), the black birol (Turdus merula), the weathear (Oenanthe oenanthe), the great grey shrike (Lanius excubitor), the Bonelli’s warbler (Phylloscopus bonelli), the melodious warbler (Hippolais polyglotta), the spotted flycatcher (Muscicapa striata), the rock bunting (Emberiza cia), the ortolan bunting (Emberiza hortulana), the wall creeper (Tichodroma muraria), the blackcap (Sylvia atricapilla), the whitethroat (Sylvia communis), the gold crest (Regulus regulus), the long-tailed tit (Aegithalos caudatus), the blue tit (Parus caeruleus), the great tit (Parus major), the crested tit (Parus cristatus), the coal tit (Parus ater), the marsh tit (Parus palustris), the linnett (Carduelis cannabina), the carrion crow (Corvus corone), the raven (Corvus corax), the hoopoe (Upupa epops), the cuckoo (Cuculus canorus), and the nightjar (Caprimulgus europaeus).
The mammals recorded are micromammals (Sorex sp., Microtus sp. and Apodemus sp.) hedgehogs, martens, hares, foxes, badgers, some bats (Barbastella barbastellus, Nyctalus noctula, Pipistrellus kuhli), weasels, and roe deer.
Snakes are represented by vipers (Vipera aspis), Coluber viridiflavus, Elaphe longissima, Coronella austriaca, C. girondica, Natrix tassellata, N. natrix. Common are the lizards Podarcis muralis and Lacerta viridis, and also Anguis fragilis is present.
Amphibians are limited to the wet areas. They are salamanders (Salamandra salamandra), toads (Bufo bufo and B. viridis), and frogs (Rana dalmatina, R. esculenta, Bombina variegata, and Hyla arborea). Triturus alpestris is present in the small lakes of Marco.
5
Daniele MASETTI
THE GEOLOGY OF THE LAVINI DI MARCO
THE MESOZOIC SUCCESSION IN THE ADIGE RIVER VALLEY AND VENETIAN PRE-ALPS: ITS ARRANGEMENT IN THE SCENARIO OF THE TETHYS EVOLUTION
The stratigraphic succession of the Adige River valley is a pile of carbonate rocks more than 1500 m thick, deposited in marine environments between the end of the Triassic and the Late Cretaceous. The main part is constituted by the Dolomia Principale (Late Triassic), Calcari Grigi (Early to Mid Liassic) and Oolite di San Vigilio (Late Liassic-Early Dogger). These lithostratigraphic units, which represent the lower part of the Mesozoic succession, originated from shallow water deposits of a carbonate platform. The upper part, only 200 m thick, is made up of prevailing pelagic carbonates (Rosso Ammonitico, Mid-Late Jurassic; Biancone, mainly Early Cretaceous; Scaglia Rossa, Late Cretaceous).
During the Late Triassic, the present Adige valley, the Dolomites and the Venetian Pre-alps were part of the wide carbonate platform that developed along the western (?) coasts of the Paleotethys margin of the African continent. At the end of the Triassic the disruption of the Pangea began and the carbonate platform where the Dolomia Principale was depositing began to be dismembered into blocks N-S oriented and with differential subsidence. Some blocks became basins during Early Liassic (Belluno Basin) and later (?)the Lombardian Basin also began to form. Other blocks (Eastern Lombardy, Veneto and Friuli) remained carbonate platforms during the Liassic but the wetter climate led to the formation of limestone instead of dolostone. Above the Dolomia Principale deposited the Membro Inferiore of the Calcari Grigi on the Trento and Friuli Platforms; the Corna in Eastern Lombardy. Lower Liassic carbonate platforms exist elsewhere in Italy: the Calcare Massiccio of the Appennine, from Tuscany to Marche down as far as southern Italy.
Between the Early and the Middle Liassic (~195 m.y.a.) wide parts of the carbonate platforms drowned because of crustal straining due to the opening of the Ligurian Ocean to the west. The Lombardian carbonate platform of the Corna was covered by the basin deposits of the Medolo Formation. On the Trento Platform the oolitic Membro Medio of the Calcari Grigi was deposited above the Membro Inferiore. In the Northern Apennines the Calcare Massiccio was covered by the Calcari Selciferi basin or by Rosso Ammonitico facies. In the Southern Apennines the carbonate platform deposition went on undisturbed.
During the passage between Early and Middle Jurassic (180 m.y.a.) the Trento Platform drowned and became an oceanic plateau where the pelagic Rosso Ammonitico Inferiore was deposited. A high production of oolitic sands along the western margins of the Friuli Platform led to the infilling of the nearby Belluno Basin by turbidity currents (Calcare del Vajont).
During the passage between Middle and Late Jurassic (160 m.y.a.) there was an increase of silica sedimentation with the formation of the Radiolariti (derived from radiolarian ooze) in the Lombardy Basin. The Scisti ad Aptici was deposited on the western Trento Plateau, while in the Eastern Trento Plateau and in the infilled Belluno Basin the Fonzaso Formation formed. The Upper Jurassic is represented in the Venetian Alps by the Rosso Ammonitico Superiore. The widespread deposition of pelagic limestone began at the end of the Late Jurassic (Maiolica in Lombardy and Apennines, and Biancone in Veneto) due to the boom of the carbonate plankton. This kind of deposition characterized the Early Cretaceous.
Around the beginning of the Late Cretaceous the deposition of pelagic carbonate ooze was replaced by alternations of limestone, greenish marls and black levels rich in organic matter (Scaglia Variegata in Veneto and Scisti a Fucoidi in the Apennines). Above these alternations began the sedimentation of the emipelagic Scaglia Rossa. Rudist “reefs” developed on the Friuli Platform.
The beginning of the Alpine orogeny led to the uplifting of the region in the Early Tertiary and the plateau became a carbonate platform again. Tertiary carbonate platforms were surrounded by basins where the deposition of Flysch, a product of the erosion of the arising Alpine chain, began.
THE TRENTO PLATFORM AND ITS LIASSIC FORMATIONS
The Liassic shallow water limestones of the Trento Platform can be divided into two sequences. The first is made up of Calcari Grigi and Oolite di Massone (Early-Middle Lias) placed between the Dolomia Principale and a discordance at the top, corresponding to a temporal hiatus wider and wider going from west to east. The second sequence (San Vigilio Group) is Late Liassic-Early Dogger and is placed between the hiatus and the Rosso Ammonitico Inferiore, but can only be found in the western sector of the platform.
THE CALCARI GRIGI FORMATION
The Calcari Grigi were informally divided by Bosellini & Broglio-Loriga (1972) into Membro Inferiore (more than 100 metres thick) where the footprints were found, Membro Medio (or oolitic) and Membro di Rotzo or Membro Superiore [for their datation see chapter 6]. The Membro di Rotzo is the most studied and the better known.
THE MEMBRO INFERIORE OF THE CALCARI GRIGI OF THE ADIGE VALLEY
The lowermost part of this member is made of alternances of limestones in metric beds and levels of green clay, without evidence of tidal deposits. In contrast, structures typical of the tidal environment (stromatolites etc.) characterize the upper part of the member where the dinosaur footprints are found, several tens of metres below the passage to the Membro Medio.
Therefore, peritidal cycles due to the concurrent action of subsidence and carbonate deposition, constitute the upper part of the Membro Inferiore [this part is described in detail in chapter 9].
The subtidal facies, representing the lower 2/3 of the cycle, is mainly made up of homogeneous micritic, peloidal-fossiliferous limestones, completely reworked by bioturbation. Sometimes accumulations of large bivalves are present. There are both storm layers and colonies with individuals in life position. The intertidal facies are undistinguishable from the subtidal.
The supratidal facies are characterized by peculiar sedimentary structures such as storm-bacterial lamination (stromatolites), mud cracks, teepees, birdseyes, flat pebble breccias etc..
The causes of the peritidal cyclicity are autocyclical (sedimentologic) or allocyclical (glacioeustatic) without the possibility of knowing at present which one was prevalent.
Fig. XX shows a hypothetical paleogeography of Italy during an imprecise moment of the Early Lias.
THE BASAL SUBTIDAL UNIT OF THE MEMBRO INFERIORE
As mentioned above, this unit is characterized by the prevailing subtidal micrites and absence of peritidal facies. This basal part is the most typical and widespread of the Membro Inferiore; it has a thickness in excess of 100 m at the eastern sector of the platform, where it represents the whole member. It is gradually replaced by the peritidal unit to the west, where the latter reaches a maximum thickness of 50 m in the Adige Valley. The basal unit is made up of cycles about one metre thick with subtidal micrites poor in fossil content at the base and centimetric levels of green clay at the top. The origin of the clay levels is controversial: caused by subaerial exposure and limestone dissolution or by “starvation” of the lagoon with restricted circulation and the end of carbonate production. The cause of the cycles is glacioeustatic, as shown by their gerarchic organization into two orders of magnitude.
THE OOLITIC MEMBRO MEDIO
The Membro Medio originated from oolitic sands organized into submarine dunes by tidal currents. It is a wedge-shaped lithosoma thicker to the west, (more than 200 m in the Sarca River valley, Trento) and thinner to the east (150 m in the Group of Mt Baldo, 30-40 mt in the Sette Comuni Plateau where it ends east of Gallio). This member is similar to the Oolite di Massone. Biostratigraphic data suggests that this unit becomes younger from west to east. It represents a drowning of the region caused by the collapse of the western sector of the platform.
THE MEMBRO DI ROTZO
This member is rich in plants remains and bivalve banks (“Lithiotis banks”). Its western margin of deposition was situated in correspondence to the Mt Baldo Group, the eastern coincided with the Mt Grappa Massif. Its geometry is similar to that of the Membro Medio and their eastern terminations coincide. It is characterized by high clay content and a particular cyclicity. Each cycle is composed of alternations of marl-limestone at the base and Lithiotis mounds or fossiliferous calcarenites at the top. Lithiotis banks, tabular or lenticular (mounds) biogenic bodies up to 2-3 m thick, are frequent mainly in the upper part of the member. Each cycle is shallowing-upward according to the life needs of the bivalves. These cycles are interpreted as being formed in a low-angle ramp setting, with the deepest part to the west, where it was bordered by the littoral sand body of the Oolite di Massone (ramp-lagoon depositionary model).
6
Carmen BROGLIO LORIGA
PALEONTOLOGICAL ASPECTS OF THE CALCARI GRIGI
This chapter deals with the fossils found in the Calcari Grigi and excludes reptile footprints. The paleontology of this formation is essentially that of its Membro Superiore, or Membro di Rotzo, because of its fossil richness. In contrast the Membro Medio and Membro Inferiore are relatively poor in of fossils.
THE MEMBRO DI ROTZO AND THE LITHIOTIS FACIES
The fossils of this member are both marine invertebrates and terrestrial plants. They were first studied in 1764 but were subject to more detailed analysis during the 19th century. The Lithiotis facies, which takes its name from the bivalve Lithiotis problematica Gümbel, is typical of the member and is characterized by mounds or banks of this and other large, oyster-like bivalves. Other organisms are brachiopods, gastropods and foraminifers; less common are individual and colonial corals, porifera, echinoderms, ostracods and ammonoids. Vertebrates are represented by fish teeth (Pycnodus). Most of these organisms belong to the domine of shallow waters. Fossil vegetalia are shallow waters red and green calcareous algae and terrestrial Equisetatae, Filicatae, Coniferophytinae, Cicadophytinae and several parataxa of palinomorphs.
LARGE BIVALVES
The large bivalves are the peculiar component of the Lithiotis facies. They are represented by the following genera: Lithiotis Gümbel, Cochlearites Reis, Lithioperna Accorsi Benini, Mytiloperna von Yhering, Gervilleioperna Krumbeck, Pseudopachymytilus Krumbeck
Other less common but characteristic bivalves of the Liassic biofacies are: Opisoma Stoliczka, Protodiceras (Gümbel), Pachyrisma (Pachyrisma) Morris & Lycett, Pachyrisma (Durga) Böhm, Pachyrisma (Pachymegalodon) Gümbel.
They are characterized by a large, thick shell with a small body cavity. The shell of Lithiotis, Cochlearites and Lithioperna often reaches a height of 25-30 cm and a thickness of 1-1.5 cm. Lithiotis and Cochlearites have a spoon-shaped shell; that of Lithioperna is cup-like. However, there is a wide variability of shell shape, convexity, thickness and ornamentation.
SMALL BIVALVES
The small bivalves are rather diversified; the most common are Gervilleioperna ombonii Negri, Pseudopachymytilus mirabilis (Lepsius) and the megalodontacea Protodiceras pumilus (Gümbel), Pachyrisma (Pachymegalodon) chamaeformis (Schlotheim), Pachyrisma (Durga) crassa (Böhm) and P. (Durga) nicolisi (Böhm). Gervilleioperna ombonii lived in the upper-subtidal mud, Pseudopachymytilus mirabilis in the intertidal mud, forming dense populations (mounds, see below) like the living mussels.
THE “LITHIOTIS MOUNDS”
In life these were associations of gregarious bivalves mixed with mud and in relief above the muddy bottom. Lens-like mounds with upward concavity, 25-50 cm thick correspond to communities of the smaller bivalves Pseudopachymytilus mirabilis, Gervilleioperna ombonii and Neomegalodon pumilus. The characteristic thick mounds, tabular or most frequently lens-like with upward concavity (up to 2-3 mt thick), with chaotic distribution of large bivalve shells are mono-specific associations of Lithiotis problematica, Cochlearites loppianus and Lithioperna scutata, with a prevalence of the second. The small bivalves began the colonization of the muddy bottom forming a firm base for the successive development of the colony of large bivalves.
GREGARIOUS GASTROPODS: THE GROUP “TEREBRA-NORIGLIENSIS”
Gastropods are present at different levels of Calcari Grigi but identified taxa are very few (Patella conoidea Lepsius, Patella (Scurria?) tirolensis Tausch, Emarginula orthogonia Tausch, cf. Neritopsis ?oldae Stoppani, Natica ssp., Chemnitzia terebra Benecke, Nerinea (Aptixiella) norigliensis Tausch) and rare in respect to bivalves. The turriculate gastropods Chemnitzia terebra and Nerinea (Aptixiella) norigliensis (possibly synonyms) are abundant, gregarious and identify a biofacies in the lower part of the Membro di Rotzo. They are found in the most marginal part of the platform where the waters were well oxygenated and rich in nutrients.
BRACHIOPODS
These stenoaline animals are well represented. Tausch (1890) found the genera Terebratula, Waldhemia and Spiriferina, now revised or in need of revision. At present the terebratulids are considered the most characteristic brachiopods of the unit with the species Hesperithyris renierii (Catullo), Lychnothyris rotzoana (Schauroth), Lobothyris punctata (Sowerby) and are referred to the Pliensbachian.
FORAMINIFERS AND CALCAREOUS ALGAE
The Foraminifera are diversified, the most characteristic taxa being the following: Orbitopsella gr. primaeva Hottinger, Orbitopsella gr praecursor (Gümbel), Orbitopsella cf. dubari Hottinger, Lituosepta recoarensis Cati, Planisepta compressa (Hottinger), Amijiella amij (Henson), Haurania deserta Henson, and Vidalina martana Farinacci. Like bivalves, they form oligotypic or even monotypic associations.
Orbitopsella and Planisepta (= Labyrinthina) compressa are important biostratigraphic markers. Glomospira was the only foraminifers to live in the restricted, oxygen-depleted lagoon.
Calcareous algae are represented mainly by Palaeodasycladus mediterraneus (Pia) (green algae, Dasycladales), Solenopora sp. (red algae), Thaumatoporella parvovesiculifera (Raineri) (incertae sedis). Palaeodasycladus mediterraneus is a biostratigraphic marker of the Liassic and has a wide geographical distribution.
TERRESTRIAL flora
Terrestrial flora is of particular interest in a book devoted to land animals as the dinosaurs were. The flora of the Calcari Grigi was described mainly by de Zigno (1856-1885) and more recently by Wesley (1956, 1958, 1966). According to Wesley floristic association was dominated by Bennettitales, followed by conifers, Caytoniales, Filicales (Dipteridaceae, Dickinsoniaceae, Mathoniaceae and perhaps Gleicheniaceae) and Equisetales. Study of palinomorphs (Van Erve, 1977) showed that the ferns are as nearly common as the gymnosperms in the sample, Caytoniales are relatively rare and Licopodophyta are also present.
According to Wesley, the habitat was a coastal, mangrove-like, salty swamp with the conifers living on nearby uplands and a few ferns living far from the brackish waters. The predominance of xerophitic plants would suggest a relatively arid climate. The more abundant fern evidence in the palinomorph sample would suggest a somewhat more humid climate.
The affinities to the generic level show that the megaflora of the Calcari Grigi is different from those of coeval European associations (Württemberg, southern Poland, Eastern and southern France) because of the presence of Gleichenites, Dichopteris, Cycadopteris, Sphenozamites, Dactylethrophyllum, Yuccites and Phyllotheca. Some resemblance exists with megaflora from the Lower Jurassic of Lorraine and Middle Jurassic of Sardinia. The equisetales Phylloteca brogniartiana suggests a Gondwanian affinity of the macroflora, which however is not supported by the palynomorphs.
COMMUNITIES AND LIFE ENVIRONMENTS
The following communities/ environments are identifiable in the Membro di Rotzo:
1) terrestrial - represented by the plants; mangrove community along the coast, community with ferns and conifers in hypothetical inner uplands.
2) swamp - remains of herbaceous plants
3) restricted lagoon - eurialine foraminifers and ostracods
4) intertidal-upper subtidal - Pseudopachymytilus and Gervilleioperna mounds
5) subtidal - a) low energy, Lithiotis, Cochlearites, and Lithioperna mounds; b) mid-energy with prairie-like bottom, Orbitopsella community; c) outer limit of the lagoon with (1) moderate wave motion (Labyrinthina compressa community) or (2) below the level of wave action (“terebra-norigliensis” gastropod community and, perhaps, a community with megalodontaceans).
PALEONTOLOGY OF THE MEMBRO INFERIORE AND MEMBRO MEDIO
The fossils in these members are much rarer and have not been the subject of a great deal of study. Brachiopods at the base of the Membro Inferiore are represented by “Terebratula” dubiosa Haas and Pisirhynchia uhligi Haas. Small foraminifers (Textulariidae, Ataxophragmiidae and the rare lituolid Mancyna cf. termieri) are found at various levels. The most important microfossil from a chronostratigraphical point of view is the alga Palaeodasycladus mediterraneus (Pia) which is considered to be a Liassic marker. There are also solenoporacean algae, ostracods, small gastropods and echinoderm remains.
The microbiofacies of the Membro Medio is similar, with the addition of nodosariform foraminifers and the alga Solenopora cf. liasica Le Maitre. Among the macrofauna, chetetid spongia and several valves of pectiniformes bivalvs are also found.
THE AMMONOIDS OF THE CALCARI GRIGI
Ammonoids, the basic biostatigraphic markers for the Mesozoic, are rather rare in the Calcari Grigi. They were only found in the western part of the Trento Platform; in every case they were collected in the debris near outcrops of the Calcari Grigi. The following taxa were found: Harpoceras cornacaldense Tausch, Fuciniceras (Protogrammoceras) sp., Fuciniceras suejense tinctum Wiedenmayer, Juraphyllites libertus (Gemmellaro), Charmasseiceras sp.. Harpoceras cornacaldense was attributed to the subgenus Fuciniceras (Protogrammoceras) (Sarti, 1981). Also an ammonoid association found into an isolated boulder found near Sospirolo, Mis Valley (Belluno) was attributed to the Calcari Grigi (but there is no general agreement on this attribution). The following taxa were identified: Partschiceras tenuistriatum (Meneghini), Partschiceras cf. retroplicatum (Geyer), Juraphyllites libertus (Gemmellaro), Harpophylloceras eximium (Hauer), Liparoceras (Becheiceras) bechei (Sowerby), Androgynoceras striatum (Reincke), Protogrammoceras celebratum (Fucini), Protogrammoceras dilectum (Fucini).
THE AGE OF THE LITHIOTIS FACIES AND OF THE CALCARI GRIGI
The attempt at dating the Calcari Grigi began during the second half of the last century with the description of the plants of the Membro di Rotzo by de Zigno. He dated them as Middle Jurassic on the basis of a comparison with other fossil florae and faunae found in Europe.
The ammonoids Protogrammoceras cornacaldense, Protogrammoceras sp., Juraphyllites libertus and Fuciniceras suejense tinctum indicate the Early and Late Pliensbachian. Data from the palynomorphs suggest that the Membro di Rotzo and the upper part of the Membro Medio are Late Pliensbachian-Early Toarcian.
At present dating is mainly based on the calcareous algae and, above all, foraminifers with the identification of three biozones. The reference point is the Orbitopsella Zone; fixed its cronostratigraphic collocation, dating of the levels above and below it is done according to their stratigraphical position with respect to that Zone. The Orbitopsella Zone is recognized in the Lower Jurassic series of carbonate platforms all over the world; in Northern Africa its dating (based on ammonoids) is Carixian. The Planisepta compressa Zone, corresponding to the uppermost part of the Membro di Rotzo, above the Orbitopsella Zone, is referable to the Late Pliensbachian. The horizon with plant remains is consequently Domerian, and placed between the Orbitopsella Zone and the Lituosepta Zone. Below the Calcari Grigi there is the Late Triassic Dolomia Principale, and their boundary is considered isochronous. Consequently, the Membro Inferiore and Membro Medio are Hettangian and Sinemurian in toto if the Orbitopsella Zone is Carixian, or are Hettangian-Sinemurian p.p. if the Zone extends into the Sinemurian. Actually the dating of Membro Inferiore and Membro Medio are not based on good biostratigraphic markers excluding the Early Sinemurian ammonoid Charmasseiceras. There seems to be continuity of sedimentation, without wide hiatuses, between the Dolomia Principale and the Membro Inferiore and between the latter and the Membro Medio. Palaeodasycladus mediterraneus, a biomarker of the Liassic, is present in the Membro Inferiore, together with some foraminifers, which are found in the Membro di Rotzo but not in the Triassic. This suggests a Hettangian-Early Sinemurian dating of the Membro Inferiore and Membro Medio.
7
Giuseppe LEONARDI
ACCOUNT ON THE DINOSAURS
This general account does not concern the site in the strict sense and is not reported here.
PART I I - THE DINOSAUR TRACKS IN THEIR PALEOENVIRONMENT
Giuseppe LEONARDI and Paolo MIETTO
THE LIASSIC DINOSAUR TRACKS OF THE LAVINI DI MARCO
INTRODUCTION
Three dinosaur tracks (ROLM 1, 9 and 11) were discovered for the first time at the Lavini di Marco in 1988 by Luciano Chemini. Many other footprints and tracks were found during July 1991 by a systematic field exploration of the site carried out by the research team from Museo Tridentino di Scienze Naturali and Museo Civico of Rovereto, which were led by the authors, from 1991 on. The site is one of the richest of Europe, with about 70 tracks and at least 90 isolated footprints, left by a total of about 140 individuals; total individuals are more than 200 if one considers indeterminate and unstudied specimens.
Most of the footprints are found along the “colatoi”, at the “hinge” and on the “laste alte”. The “colatoi” are regions of the mountain flank were debris and soil have been cleared away by water flow after heavy rains. The “hinge” is a zone of “knee-like” flexure of the rocky layers, high on the mountain flank; the “laste alte” is a wide, smooth and sloping flat area made by the surface of a rocky layer or few rocky layers (i.e. the topographic and stratigraphic surface coincide) high on the mount flank. In order to identify the different “colatoi” we named them “colatoio Chemini”, “colatoio of the sauropod”, “colatoio of the theropods” and “colatoio of the ornithopods” (see Fig. XX in the Italian text).
The footprints and tracks testify to the presence of many dinosaurs. The most abundant are theropods (about 80) probably Ceratosauria, then there are about 15 early sauropods, some advanced ornithopods, about 20 bipedal dinosaurs (possibly small-size primitive ornithopods), about 10 footprints or tracks of indeterminable plant-eaters (probably sauropods) and finally, some unidentified dinosaurian footprints.
The description and study of this material was carried out following methods and terminology of Leonardi (ed.) and co-authors (1987a).
Most of the fossil footprints are not true footprints but are underprints. When we tried to clean the footprints of the rocky infilling, we were not sure about which of the many surfaces was the true printed surface. In many cases the visible part of the footprint is made by non-coeval surfaces. In ROLM 2 and 9, for example, the bottom of each footprint is the true printed surface because it presents a flat pebble breccia, due to the crushing of the mud-cracked original sedimentary surface by the dinosaur foot. However, their lateral wall has a different age, because it is cut across a number of levels. The surface of the displacement rim and the surrounding field surface do not correspond to the soft and waterlogged surface on which the dinosaurs stepped, which was eroded, but a deeper and more consistent level. So each extant footprint is composed by three kinds of non-coeval surfaces.
DESCRIPTION
THEROPODS
The dinosaurs represented by tridactyl footprints, with slender and clawed digits of predators, are the most common in the site. The footprints are shallow, sometimes difficult to identify, and the tracks are incomplete or represented by few footprints. This means that the authors were light and relatively quick. Up to now about eighty individuals have been identified; however there is one surface that was over trampled by tridactyl dinosaurs that is waiting for to be studied on the “laste alte”. Therefore, the number will increase.
Identification of the footprints is difficult because of their shallowness. The morphology of the prints differs greatly in the same track, showing that it is also influenced by gait, foot stance and substrate condition. Some of the tridactyl footprints could belong to primitive ornitischians, some of which had theropod-like feet, functionally tridactyl and clawed. We consider here as theropod all the footprints that clearly do not to belong to ornithischians.
Theropod footprints can be grouped into the following categories:
1) tetradactyl (Italian text-figs. 8.4, 8.5, 8.7),
2) with wide interdigital II-IV angle (Italian text-figs. 8.3/9-15),
3) small-sized, with short and stout digits, (Italian text-figs. 8.3/20-23),
4) with long , wedge-like “heels”, (Italian text-figs. 8.4/3, 4, 11,12),
5) with broad and/or spatulated digit III, (Italian text-figs. 8.3/16-18),
6) with long, slender and sinuous digit III, (Italian text-figs. 8.3/1-8),
7) others, subdivided into:
a) “crescent”-shaped footprints, (ROLM60, ROLM154/3),
b) footprints with anomalous nails (Italian text-fig. 8.4/10),
c) grouped digits, (Italian text-fig. 8.4/6),
d) repeated prints, (Italian text-fig. 8.4/7),
e) scratches (Italian text-fig. 8.4/8),
SAUROPODS
The first sauropod track was found on June 1992 (ROLM75). Up to now ROLM 1, 2, 4, 11, 14, 21, 26, 28, 33, 61, 67, 75, 126, 173, 200 and possibly several more (Italian text-figs. 8.16-26, 8.28), can be attributed to sauropod trackmakers. Because of the poor state of preservation no new ichnotaxonomic name was given to this material. The two best preserved tracks are herein described.
ROLM 75 (Italian text-figs. 8.16, 8.24-8.26): quadrupedal, narrow gauge track, 7 m long, slightly curved, with 10 pes-manus sets. The pes-manus axis is directed outwards (32°) with respect to the trackway midline. The ratio stride/pedal footprint length is rather low (about 3), testifying the slow walking gait of the trackmaker. The pace angulation of pedes is very low (mean=95°) as is that of the manus (about 60°) because the manual print is in front and lateral to the pedal. The latter is usually pyriform and deeper anteriorly; digit prints are sometimes present, with a variable number (1 to 4) of small, short, pointed and clawed marks. However, the pes was probably pentadactyl. The hypex are very “open” and blunt. We think that sometimes the collapsing mud totally obliterated the marks of the claws. The manual prints are kidney-shaped, crescent-like or, in one case, nearly horseshoe-like, with a marked indentation in the posterior margin. This shape is partly due to the deformation caused by the overprinting of the pes. The digital prints of the manus, rarely left or preserved, are short and pointed, with hypex wide and blunt (footprints 4 or 6); it is difficult to state the actual number of digits. The track is irregular, because of the gait of the trackmaker and the variable substrate condition. There are many middle to large-size theropod footprints and associated tracks.
ROLM 28 (Italian text-figs. 8.16, 8.18, 8.19): is a short track, with 5 incomplete pes-manus sets and some underprints. There are several differences to ROLM 75: larger size (the average pes length is 52 cm against 45 cm), higher pace angulation and, consequently, narrower track, the pes-manus axis is outwardly directed to a lesser degree.
ROLM61 is similar to ROLM75 and 28. However, ROLM1, 2, 11, 26 and perhaps 126 are morphologically different: the anterior margin of the pes presents three or four digit prints with the shape of rounded lobes, manual prints are shallow or absent, perhaps totally overprinted by the pes. These trackways are narrow gauged, manual prints are often, but not always, laterally placed and do not diverge from the midline.
POSSIBLE ORNITHOPODS
There are very deep (up to 15 cm) and evident tridactyl or tetradactyl footprints. The two best examples of these specimens are described here.
ROLM 64 (Italian text-figs. 8.31-8.32, 8.40-8.41): a straight, bipedal or perhaps semibipedal track, 14 m long with 24 footprints. The animal was slowly walking with alternating short (left-right) and long (right-left) paces. We cannot exclude that the trackmaker was limping. There are huge expulsion rims with interference between adjacent rims and the mud sometimes collapsed into the footprint. The footprints generally have an oval or pyriform shape, and are tetradactyl (but the mark of digit I is rarely preserved) with digit II-IV large and hoof-like and digit I (footprint 23) medially placed as a spur, short and rounded, impressed only when the foot sank deeply into the mud.
ROLM 63 (Italian text-figs. 8.30, 8.39): bipedal track, composed of three non-consecutive footprints (a right, a left, then the right is missing and a left one follows). Also in this case digit I seems to be present. The footprints are deep (up to 8 cm). The first footprint shows three, hoof-like, toes separated from the “plantar” pad; digit III is particularly short. In the second footprint the mark of the digit II is narrow and spatulated because the mud collapsed into it.
The animal was walking slowly, with alternating short (left-right) and long (right-left) paces. Also in this case, we cannot exclude that the trackmaker was limping. There are huge expulsion rims with interference between adjacent rims and the mud sometimes collapsed into the footprint. The third preserved footprint shows the mark of digit I.
OTHER TRACKS
Other footprints and tracks, poorly preserved, belong to the same form: track ROLM9 (Italian text-figs. 8.28, 8.37), 181 (Italian text-fig. 8.29) and 30 (Italian text-fig. 8.38).
Other tracks can be identified as ornithopodian:
- ROLM 192 (Italian text-figs. 8.34, 8.35) differs from the others because of the stronger foot, with footprints deeper laterally, the “heel” is much longer and triangular, wedge-shaped because of a digit IV mark which is developed posteriorly behind the phalangeal-metatarsal articulation.
- ROLM50, a lighter form, with slender digits but ending with a hoof.
- Some tridactyl footprints with digits, a little broader than those of the theropods and without claws, could belong to less specialized and less advanced ornithopods like, for example, the “fabrosaurids” (Italian text-figs. 8.4/13-16). In any case, they will be considered as unidentified bipedals in the statistics.
FOOTPRINTS AND TRACKMAKER IDENTIFICATION
THEROPODS
Ichnologic determination of the tracks
It is very difficult and often impossible to give formal names to the ichnological material being studied because of the poor and incomplete preservation and the high morphological variability of the footprints on the same track. Besides, the hind feet of the tridactyl dinosaurs are basically the same in most ornithopods and theropods, mainly those of small to medium-size taxa. Therefore the following classification is only indicative.
Morphofamily Anchisauripodidae Lull, 1904
Grallator Hitchock, 1858: about 15 footprints could belong to this ichnotaxon (ROLM32, 37, 39, 74, 89, 93, 97, 120, 128, 140, 141, 151, 152, and 206).
Morphofamily Eubrontidae Lull, 1904
Eubrontes Hitchock, 1845: about 10 footprints could belong to this ichnotaxon (ROLM31, 36, 38-41, 44,71, 130 and 193).
Footprints comparable to Columbosauripus Sternberg, 1932: ROLM60, 76 and 96 can be morphologically compared to this Cretaceous ichnogenus.
Footprints resembling other ichnogenera
a) Some large footprints such as ROLM 13 and 41 resemble the anterior part of Bueckemburgichnus maximus Kuhn 1958.
b) ROLM70 presents features of Saltopoides igalensis Lapparent and Montenat, 1967.
c) ROLM5 shares with some genera attributed to theropods the presence of a spur-like, facing backward digit; otherwise it resembles the Grallator.
d) ROLM 49, 87, 89, 120, 132-133, 158 could belong to Coelurosaurichnus but this ichnogenus was demonstrated to be invalid (= Grallator).
In conclusion the identified ichnotaxa are Grallator, Eubrontes and that with short and broad digits. This association is similar to others found in the Lower Liassic; however, theropod footprints are of little use for biostratigraphical purposes. Noteworthy is the absence of the morphofamily Gigandipodidae Lull, 1904.
Classification of the trackmaker
The trackmaker must be found in the suborder Ceratosauria (Italian text-figs. 8.13-8.15, 8.44, 8.47, 8.54, 8.56) rather than of the suborder Carnosauria or Coelurosauria as reported in the past, mainly in paleoichnological papers. Ceratosauria was the only theropod group definitely alive during Early Jurassic times.
SAUROPODS
Ichnologic determination of the tracks
The tracks are attributed to primitive sauropods but more advanced from the ichnological point of view. They are the oldest sauropod tracks found up to now in the world. The diagnostic features are: quadrupedality with marked heteropody, characteristic shape of the manual (crescent-like etc.) and pedal prints, strong positive (outwards) divarication, short and pointed digits on the hind feet and, when present, also in the fore feet, with hypexes open, blunt and rounded; relatively low pace angulation.
Because of these typical sauropodian features, we do not attribute the tracks to prosauropods.
Since they are narrow-gauged, we do not compare them with the wide-gauged ones, like Brontopodus Farlow, Pittman & Hawthorne, 1989. They resemble Parabrontopodus Lockley, Farlow & Meyer, 1994 of the Upper Jurassic of USA and the holotype of Breviparopus Dutuit & Ouazzou, 1980, Upper Jurassic of Morocco. With the latter they share the marked positive (outwards) divarication of the pes-manus set, the manual prints placed rather laterally and their overall shape, the forward directed foot nails, the short pedal prints and their overall shape. The differences are: the manual print of Breviparopus never presents large nail marks and hypexes, the distance manus-pes is shorter, the footprints are larger (more than twice the size).
The differences reported above between ROLM75 and ROLM28 are not sufficient to classify them into two separate ichnospecies; anyway, we do not create a new ichnotaxon because of the poor preservation.
Identification of the trackmaker
The lateral position of the manual prints suggests a sauropod as the trackmaker with a rather broad shoulder girdle and particularly well developed fore-limbs. This, as well as the age, suggest the attribution to the poorly known family Vulcanodontidae Cooper, 1984. However, we cannot exclude a member of the Cetiosauridae Seeley, 1874 or, in every case, a member of the Eosauropoda Bonaparte, 1986a as being the trackmaker.
POSSIBLE ORNITHOPODS
Ichnologic determination of the tracks
The main aspect to stress is that up to now large, iguanodontid-like footprints have never been found in the Lower Jurassic. The footprints under examination are different from the coeval Moyenisauropus Ellemberger and Anomoepus E. Hitchcock, 1848, belonging to primitive ornithopods, perhaps “fabrosaurids”. They never present the mark of the true heel, digits II-IV are much shorter, mainly digit III, and hoof-like. Besides, they are much larger and the tracks are in most cases bipedal. They show a striking similarity to the Late Jurassic and Early Cretaceous footprints attributed to iguanodontids. Similarities exist also with hadrosaurids. However, all the footprints of large ornithopods lack the mark of digit I.
Discussion about the trackmakers
The trackmakers could be identified as large, graviportal ornithopods, very ancient but not very primitive from an ichnological point of view. They could be related to iguanodontids (Italian text-figs. 8.43, 8.47). The presence of digit I is a primitive character since it is not present in the iguanodontids and hadrosaurids, with the exception of Camptosaurus Marsh. If the footprints under examination are actually ornithopodian, we are not brave enough to attribute them to the family Iguanodontidae sensu stricto but we think that they could be at the base of this family or belonging to an unknown family strictly related to it. The presence of iguanodontids in the Lower Jurassic would record this group about 40 (taking into account Callovosaurus Galton) or also 50 millions before the comparison of the first bones in the fossil record.
However, we cannot ignore, mainly for the track ROLM64, another hypothesis: that the trackmaker could be a sauropod. Therefore, we avoid giving a formal name to the large “ornithopod” tracks and we will name them provisionally as “advanced ornithopods”.
DESCRIPTION AND DISCUSSION ABOUT ICHNOASSOCIATIONS
There are five levels with footprints in a section five metres thick (levels 101, 104, 105, 106, 115 and 120). The main levels (104, 105, 106, 115) are concentrated in less than two metres. The richest levels are 105 and 106.
ROLM 3-7, 49-51, 53-54, 59-76, 85-104, 107, 110, 112-116, 118, 120-124, 130-133, 140-146, 150-154, 156, 158, 174-175, 206-207 are found on the level 105, for a total of 84 individuals (57 theropods, 4 sauropods, 2 indeterminate plant-eaters, 17 indeterminate bipeds, 4 possible advanced ornithopods and a dozen unidentified footprints).
ROLM1-2, 9, 11-12, 14-15, 18, 20-23, 25-41, 43-44, 47-48, 125-128, 135-136, 159, 171, 173, 181, 192-193, 197-200 are found on level 106, for a total of 49 individuals (21 theropods, 11 sauropods, 5 indeterminate plant-eaters, 6 indeterminate bipedals, 6 possible advanced ornithopods and 8 indeterminable footprints). The associations in the two levels are different: carnivorous are dominant in the level 105 (67% against 33% - but only 12% are certain - plant-eaters) whereas the reverse happens in level 106 (57% plant-eaters, 43% carnivorous). These differences probably depend on different distribution of the microenvironments at each of these two levels.
THE ICHNOFAUNA OF THE LAVINI DI MARCO COMPARED TO OTHERS COEVAL
As the stratigraphic position of the ichnofauna is indicated as Lower Jurassic, a comparison has been made with Lower Jurassic ichnofaunas all over the world, with emphasis on the differences.
Veillon (Vandée, France; Rhetian-Early Hettangian) - Prosauropods are absent in both ichnofaunas but neither are sauropods found here. Ornithopods are absent and crocodylomorph footprints (Batrachopus E. Hitchock and Dahutherium Montenat) are present. Only theropods seem to be similar in both sites.
Saint-Laurent-deTrèves (Causses, Lozère, France; Late Hettangian) - Only theropods are represented and correspond to those found at the Lavini di Marco.
“Oppidum de Grézac” (Lodève, Herault, France; Late Hettangian) - The same considerations for Saint-Laurent-deTrèves are valid.
Holy Cross Mountains (Poland; Early and Late Hettangian) - Theropod (11%) and ornithopod (89%) footprints are found in the Late Hettangian, only theropods in the Early Hettangian. The presence of ornithopod footprints, identified as Moyenisauropus and Anomoepus E. Hitchock, are the most strikingly similar to the association described here. However, large ornithopods with hoof-ending digits are not present, as are also sauropods.
Pécs region (Hungary, Early Sinemurian) - Here only theropods (Grallator and Kayentipus Welles) are represented, therefore comparisons are impossible.
Hogänas (Sweden; Rhaetian and Early Hettangian) - Here also only theropod footprints are found.
Neyzae, Kerman and Zerab (Iran; Sinemurian/Pliesbachian) - Few footprints and short tracks attributed to Grallator and mainly to large ornithopods are reported, but unfortunately comparisons are not possible because of the poor numbers. The Iranian and our associations would be similar due of the presence of theropods and large ornithopods and different mainly because of the absence of sauropods in Iran.
Jinning (Yunnan, China; Liassic) - Also here only theropod footprints are present.
“Jeholosauripus” ichnofaunas of Liaoning and Hebei (China, Rhaetian-Liassic) - Also here only the theropod “Jeholosauripus” Yabe, Inai & Shikama (= Grallator s-satoi (Yabe, Inai & Shikama) was found.
“Changpeipus” Young ichnofaunas of Liaoning and Jilin (China, Middle Jurassic or less probably Liassic) - Also here only theropod footprints are found.
Lesotho (Southern Africa, Hettangian-Sinemurian) - There is more variability in the theropod ichnotaxonomy of this ichnofauna; prosauropods seem to be absent in the Liassic levels and the presence of sauropod tracks is doubtful. The small ornithopod Moyenisauropus (=Anomoepus) present here, is absent in the Lavini di Marco. Tritiylodontid therapsids and early mammals are abundant in Lesotho but absent at the Lavini.
Spring Grange (Zimbawe, Late Triassic or Liassic) - Also here only theropod footprints are found.
Newark Supergroup (eastern coast of North America, Liassic) - The similarity of the theropod footprints of the two ichnofaunas is noteworthy. However, here sauropods and large ornithopods are absent, whereas small ornithopods (Anomoepus) and crocodylomorphs are present.
Glenn Canyon Group (South western U.S.A., Liassic) - The differences with the ichnofauna of the Lavini di Marco are the absence of sauropods and large ornithopods, and the presence of the prosauropods, Anomoepus, and crocodylomorphs (Batrachopus).
Botucatu Formation (Southern Brazil and neighbouring countries; Liassic?) - It represents a desert eolian environment. The differences with the Lavini di Marco are found in the presence of possible small ornithopods, tritylodontid therapsids, early mammals and mammaloids; the latter two are abundant. Sauropods, prosauropods and crocodylomorphs are absent.
Queensland (Australia; Late Liassic) - Here Anomoepus prints are present, these are not found at the Lavini di Marco, together with footprints of large theropods.
Therefore, the ichnofauna of the Lavini di Marco is quite different from the others that are more or less coheval, except in the case of theropods. The most striking characteristics of this comparison are 1) the absence of prosauropods (the most common plant-eaters during Liassic times), crocodyilomorphs, therapsids, protomammals, mammals and, in general, of small quadrupedal animals, 2) the presence of early sauropods and, if the identification is correct, of early but advanced ornithopods. Consequently, the ichnoassociation found at the Lavini di Marco does not fit in with the Liassic “Anomoepus-Grallator (Eubrontes) Zone” of Haubold (1986). The presence of sauropods and early large ornithopods would suggest a younger age but the absence of mammals, mammaloids and crocodylomorphs does not support this dating. If the Hettangian/Sinemurian dating is correct, we must admit that the dinosaur fauna in the carbonate platform environment of this region was different and more evolved than in other regions of the world.
BEHAVIOUR OF THE ROVERETO DINOSAURS
The study of the ichnologic evidence is the main tool to gain knowledge of the behaviour of extinct animals.
SPEEDS AND GAITS - The tracks that allow the estimation of speeds at the Lavini di Marco are relatively few, only 35. The estimated (theoretical or predicted) walking speed for Rovereto forms (cfr Thulborn, 1990, p. 293ss) is about 3-4 km/hr for small bipeds (foot length<25 cm), 4-5 km/hr for larger bipeds (26 cm <foot length< 35 cm), 5-6 km/hr for graviportal plant-eaters with pedal prints ranging 36 to 52 cm, 5-6 km/hr for sauropods.
The real speeds, calculated from the tracks of Rovereto, are in most cases lower than these estimated walking speeds and are all less than 6 kph, with the single exception being ROLM59, a small ceratosaurid with a hind foot 13.5 cm long (10-12 kph). Calculated speeds for the relatively small ceratosaurids range from 7.5 to 11 kph; those for sauropods only 1.2-2.5 kph, the presumed ornithopods standing in the middle, with 1.4-2.2 kph. The speed of indeterminate bipeds, probably small to mid-size ornithopods, range 3.2-7.2 kph. High speeds, often used to support the theory of “warm-blooded” dinosaurs, were not found at the Lavini di Marco.
The manner of gait, estimated on the basis of the stride length/height at hip ratio (cfr Thulborn, 1990, p. 263-266), was almost always walking gait (SL/h = 0.45-1.75) but in ROLM59, which was fast trotting or almost running (SL/h = 2.7).
DIRECTIONS (Italian text-fig. 8.50) - Dinosaurs often followed preferential paths because of topographical constraints as lake or sea coasts. There are 116 tracks and single footprints useful for measuring trackmaker walking direction. The NNE quadrant presents 44% of all directions, the ESE one 17.2%, SSW 28.3%, WNW 10.3%. Therefore there is a preferential corridor along an axis NNE-SSW. The two main beds with footprints (105 and 106) present a different direction from this corridor, with a counter clockwise rotation of about 30°. In level 105 the axis was NNE-SSW, in the other level it was N-S. This trend is the same for each single taxonomical group (58 theropods, 14 sauropods, 18 indeterminate bipeds). The dinosaurs of the Lavini di Marco were not moving in packs or herds but their direction was landscape-controlled. A change of the coastline direction is hypothesized to explain the change of direction between level 105 and 106. This is in agreement with the indications provided by geochemical data (see next chapter).
STANCE - In no case is the mark of the tail is preserved, as is usual for dinosaur tracks. All the trackways are rather narrow, attesting a full erect stance. The presumed iguanodontids were nearly all bipedal and in few cases, semi-bipedal, which is different from the most accepted view of the prevailing quadrupedality of these dinosaurs.
SOCIAL BEHAVIOUR - Social behaviour of theropods and sauropods is testified in some ichnosites. In contrast, the 140 individuals investigated at the Lavini di Marco, do not show any social behaviour.
MIGRATIONS - What is the meaning of the preferential N or S directions of the Rovereto tracks? Until coeval facies on the Trento Platform that are different from tidal flats are discovered, the existence of connections between this platform and others placed south and north of it is demonstrated, or the evidence of wide emerged areas found, the hypothesis of individual migration cannot be considered. We think is most logical to admit that the dinosaurs of the Lavini di Marco lived in that place, moving when a route to other lands was disposable. Another explanation of the dinosaur presence on the tidal flat could be related to their reproductive behaviour.
THE DINOSAUR COMMUNITY
The paleoichnological record is generally biased toward the preservation of footprints of large animals. Small outcrops cannot preserve the footprints of all taxa living in the surrounding region. The site of Lavini di Marco is wide and the represented environment is quite uniform.
Plant-eaters and Predators
Predators are prevalent (57%) over the plant-eaters (43%), with these percentages respectively 33% and 67% at level 105 and 57% - 43% at level 106. This differs from the theoretical ecological model of a prevalence of plant-eaters and a small number of predators. The abundance of predator footprints against the plant-eater footprints could be caused by a different level of activity of their respective trackmakers and/or by the grouping of certain taxa in particular environments: theropods could have been more abundant around pools of fresh water. The prevalence of theropods is a characteristic of many tracksites.
Weights and sizes (Italian text-figs 8.48-8.49)
Ceratosaurids which produced footprints 12-15 cm long, could reach a total body length of two to three metres and a weight of 12 to 25 kg. The larger ceratosaurids of Rovereto, with footprints 25-35 cm long, probably had the general body appearance and size of Dilophosaurus Welles, 6 to 7 m long with a weight of 280-500 kgs; the largest (footprints length: 38 cm) could reach the size of Ceratosaurus Marsh (6 to 7 m long and weighting 600 to 1200 kgs). The smallest ceratosaurid with footprints 8 cm long (ROLM212-215) was 1.5 m long with a weight of about 4 kg; it is not possible to state if it was a juvenile or a small-sized adult. The largest ceratosaurid footprint (38 cm long) comes from a level at the top of the Membro Inferiore. Some tridactyl footprints 10 to 15 cm long (ROLM211), here reported as “indeterminate bipeds” but perhaps belonging to basal ornithischians or ancestors of Thyreophora like Scutellosaurus Colbert, indicate small, bipedal plant-eaters, 1.5 to perhaps 2 m long, weighting a few kilograms. It is possible that similar footprints but longer (up to 20 cm) could belong to ancestors of the hypsilophodontids. If the large (20 to 47 cm long) tridactyl footprints with rounded hooves (ROLM9, 30, 63 and 64) actually belong to advanced ornithopods, they could have been imprinted by a dinosaur with the size of Camptosaurus Marsh, 7 m long and weighting up to 700 kg, or Tenontosaurus Ostrom, 7 m long and weighting up to 800-900 kg. Hind footprints 30 to 50 cm long testifies to the presence of relatively small sauropods, 7 to 10 m long and weighting 1 to 3 tons.
Diets and metabolism (Italian text-fig. 8.53-55)
The diet of the Rovereto trackmakers is herein minutely discussed.
The large plant-eaters (> 1 ton) were almost certainly cold-blooded, like the living large mammals partly are. The average daily forage requirement (fresh forage) can be estimated as 3 kg for a cold-blooded sauropod weighting one ton, 6 kg for a two-ton sauropod and 9 kg for a three-ton one. The yearly need would be respectively 1095, 2190 and 3285 kg. The average daily forage requirement would have been respectively 21, 42 and 64 kg in the case of a warm-blooded sauropod, a requirement seven times higher. The yearly need would have been 7.665, 15.330 and 23.360 kg.
We cannot estimate the vegetal biomass per unit of surface needed for the dinosaurs at the Lavini di Marco. The needs were probably rather high, requiring relatively abundant vegetation, with a high yearly productivity. Cases of high biomass concentration per surface unit are known among living reptiles. For example, the biomass of the giant turtles of the Aldabra atoll reaches 46tons/square km. This animal biomass would daily consume about 720 kg of fresh vegetation per square kilometre. The atoll is nearly entirely covered by bush and presents mangrove along the lagoon coast. In the case of the Lavini di Marco a biomass of 46 tons per square kilometre would roughly correspond to about 30 sauropods per square kilometre. The surface is about a quarter of square kilometre at the outcrop and the sauropod tracks are about 15 (possibly not coeval).
Juveniles and adults (Italian text-fig. 8.43-44)
Most of the footprint lengths established fall into a narrow range. There is a large number of values between 16 and 25 cm for theropods (73%; 14% of the footprints is higher, 13% lower) (Italian text-fig. 8.44) and between 36 and 48 cm for the sauropods (75%; 17% of the footprints is higher, 8% lower) (Italian text-fig. 8.43). Theropod and sauropod footprint lengths have a gaussian distribution, the sauropod ones are skewed toward larger sizes.
Plant-eater and predator interaction
The tracks at the Lavini di Marco are, as a rule, linear straight and do not show mutual behaviours. The trackmakers were just passing through. Some tracks of large plant-eaters are associated to those of carnivorous dinosaurs, sometimes moving more or less in the same direction or crossing one another but without clear evidence of interaction. The only possible example of some interaction is that of ROLM209 (Italian text-fig. 8.26) and ROLM174 (both theropods), impressed on the expulsion rim of sauropod footprints (track ROLM75) when the sediment was still plastic: it is difficult to think that the predators were not aware of the sauropod.
THE MEGAICHNOSITE OF THE CALCARI GRIGI DI NORIGLIO
The Calcari Grigi di Noriglio Formation outcropping area is defined as a megatracksite (sensu Lockley, 1994, modified) composed by the single tracksites of the Lavini di Marco, Chizzola (Leonardi, this volume), Alti Lessini (Mietto e Roghi, 1994; Roghi, 1994; Avanzini, pers. comm.), Becco di Filadonna (Avanzini, 1998), Mt Pasubio (Avanzini, 1998). It outcrops in an area about 2000 km2 wide in the Adige Valley, Southern Trentino, Sette Comuni (Asiago) Plateau and Mts Lessini. Before Alpine orogeny this surface was obviously wider. The case of the “Calcari Grigi di Noriglio megatracksite” is that of a megatracksite where the fossil footprints are most informative because they are the only dinosaur evidence (Case 1, according to the Lockley’s classification of the vertebrate paleontologic sites; Lockley, 1994, pp. 93-94).
PALAEOENVIRONMENTAL AND PALAEOGEOGRAPHIC IMPLICATIONS
Fossil footprints can provide important support for other scientific disciplines, mainly for paleoecology (paleoenvironmental data) and paleogeography. The recent discoveries of abundant dinosaur footprints in the Triassic, Jurassic and Cretaceous carbonate platforms of Northern Italy and Istria changed the palaeoenvironmental and palaeogeographic hypotheses about this area, formerly based on geologic data only.
(((The depositional environment of the Lavini di Marco site was a tidal flat. The dinosaurs therefore could not live there during high tide, when currents destroyed footprints and other structures and wore away the conglobating sediments. During the slow withdrawal of the sea, wide surfaces covered by plastic materials emerged, which were suitable for faunal colonization, and was able to cast the feet of the animals. The abundance of footprints at different levels therefore indicates periodical regressions.))
The Trento Platform was without doubt a carbonate platform but large dinosaur associations could not live at the water line. Where would those large animals go during high tide? The huge plant-eaters would not be able to find a sufficient supply of food to survive on small islands. One of the following possible solutions must be considered:
a) the existence of a continental area very close to the Lavini di Marco, or at least a wide island, of which the Trento Platform was a fringe area;
b) the presence of abundant terrestrial vegetation in the topographically higher parts of the platform. There is little evidence of this, but even in strongly continental lithostratigraphic units, like for example the Cretaceous Oldman Formation of Canada, plants and pollens are rare;
c) the presence of a quantity of algae on the platform channels and basins to feed plant-eater dinosaurs (also in this case, no evidence).
The geographic affinity of the dinosaur fauna seems to be Gondwanian, and African in particular, especially due of the presence of early sauropods, whose oldest remains were found in Southern Africa and India.
LIASSIC TETRAPODS NOT FOUND AT THE LAVINI DI MARCO
Amphibians were rare during Early Jurassic; the only group which could be present in the Lavini di Marco is that of primitive frogs but this is unlikely because of the salty environment. The Lower Jurassic is also comparatively poor in reptiles. However, at the Lavini di Marco we found the footprints of the last primitive diapsids, of sphenodontids and of kuehnosaurids but substrate conditions were not the best for the preservation of the footprints of such small animals. The absence of footprints of small primitive crocodiles, mainly protosuchids, is astonishing but it could be due to the particular environment. Among dinosaurs, scelidosaurs and, above all, prosauropods are absent. Actually we cannot completely exclude that some poorly preserved footprints identified as sauropodian could be prosauropodian. Besides, we cannot exclude that ROLM192, identified as ornithopodian, is actually prosauropodian. The relatively small footprints of the tritylodont and tritelodont synapsids could be present but they have not been found up to now. The total absence of evidence of primitive mammals is surprising; perhaps they were too small and/or preferred dryer and higher environments.
Anyway, dinosaurs seem to occupy all the ecological niches at the Lavini di Marco as in many other regions of the world, leaving no room to other tetrapods.
9
Marco AVANZINI, Silvia FRISIA and Matteo RINALDO
THE LAVINI DI MARCO DURING THE EARLY LIASSIC; RECONSTRUCTION OF AN ANCIENT BIOENVIRONMENT
The tidal flat where the Calcari Grigi deposited at the Triassic-Jurassic transition was located in the tropical belt, characterized by high temperatures without wide thermal ranges. Early dolomitization is indicative of a relatively arid climate and this suggests very arid conditions during the previous deposition of the Late Triassic Dolomia Principale.
The central part of the Membro Inferiore is characterized by the presence of inter-supratidal environments with fossilized cianobacterial mats (stromatolites); this interval is only 20 m thick at Mt Zugna and some of these stromatolitic levels were printed by dinosaurs. Sedimentologic, ichnologic and geochemical characteristics of the tracksite can be studied laterally and vertically.
Six rocky layers with footprints have been found up to now. They are located in a section about 5 m thick and correspond to the stratigraphic levels 101, 104, 105, 106, 115 and 120 (Italian text-fig. XX). Each single level can be traced over an area of a hundred of metres.
CALCAREOUS AND DOLOMITIC LEVELS
The levels 104A, 105 and 106 partim are calcareous and made by stromatolites and mud with bioclasts (ostracodes, small bivalves, calcareous algae, etc.). Abundant iron oxides concentrated into veins, laminae or globular bodies, fragments of red carbonated mud, small holes filled by silt and spatic calcite and particular chemical transformations are indicative of subaerial exposure of these levels.
Level 104A: level 104 is a subtidal layer with a mean thickness of 70 cm but very variable because of its rough upper surface which is distinguished as 104A. The depressions present in this upper part of the layer were filled by laminate mud covered by a crust of dolomite, calcite, clay and iron oxide. The topographic characteristics of level 104 are reminiscent of the lateral microkarstification of today’s tropical islands.
Level 105: it is an alternance of stromatolitic bands, peloidal grey muds and reddish muds, its thickness ranges from 15 mm to 100 mm. Its upper part presents mud-cracking, showing polygons with a diameter of 10-30 up to 50 mm. The reddish horizons probably formed in the topographically higher parts. Where the mud-cracks are larger, along the “colatoio of the ornithopods” this level is comparable to a paleosoil. Footprints of small theropods are common where level 105 is thinner. Footprints of large animals deformed the stromatolitic levels, have fragments of reddish paleosoils sticking into them.
The dolomitized levels show structures of dissolution and dedolomitization which testifies the influence of fresh waters. Dolomitization stops abruptly at contact with the overhanging layer, extending bottomwards along fractures caused by drying and dinoturbation. Probably dolomitization here was caused by dolomite sovrassature fluids due to rapid evaporation of marine water inundating the tidal flat. Dolomitized levels with footprints are 101, 106 partim and 115.
Level 106: it is the richest in dinosaur footprints, it is 100 to 150 mm thick and presents a high lateral variability of the facies. Stromatolites and flat pebbles breccias are common. Footprints are deep north of the “colatoio Chemini” and cut this level and part of level 105; in some cases at the base of the colatoio they reach level 104.
GEOCHEMICAL DATA
The high value of Na in some levels suggests the presence of ipersaline fluids during the diagenesis, low values of Sr at the top of level 104 could be related to fresh water influx.
Analysis of the isotopes points out a diagenesis of marine kind for both the calcareous and dolomitic levels. There is little geochemical evidence of the presence of soils with vegetation. Anyway sedimentologic structures and isotopic data indicate that fresh water played a role in the diagenesis of the layers with footprints.
RECONSTRUCTION IN TIME AND SPACE OF THE PALEOENVIRONMENT OF THE LAVINI DI MARCO
“Time” 104: emersion and karstification of the tidal flat occurred. However, diagenesis was mainly influenced by marine water. The red crust at the top, dissolution phenomena and values of the ratios of oxygen isotopes found in the calcite cements, indicate that the dinosaurs walked on a surface where the presence of fresh water was not sufficient to influence the diagenesis. After a period of some thousands of years, during which the level emerged, sedimentation began again with stromatolitic laminae marking the rising of the sea level.
“Time” 105: this level shows a vertical alternance of several emersions and drownings with strong environmental changes in a few centimetres of geological record. The events were:
a) formation of thin paleosoils, in association with early cementation,
b) microkarstification caused by fresh water,
c) mud deposition, perhaps by storms,
d) imbibition of this mud and deformation caused by dinosaur printing,
e) oxidation and drying of the dinoturbated surface,
f) cementation of the surface.
The influence of both marine and fresh waters are testified respectively by the presence of the marine alga Thaumatoporella and the values of the isotopic ratios, and by the absence of typical marine organisms (foraminifers, brachiopods, etc.) and microtextures. Diagenetic and sedimentologic features seem to indicate a prevalence of emersion and a coastline possibly far away. Comparison with present carbonate platforms in tropical humid climate shows that the lenses of fresh waters were ephemeral, climate was semiarid and vegetation scarce when level 105 formed.
“Time” 106: level 106 was less exposed to subaerial alteration [weathering]. In the northern outcropping area it represents sedimentation in a wide brackish pond. The southern area was less wet, characterized by a series of emerged bars with shallow pools intercalated, and was probably topographically slightly higher. The presence of black pebbles, usually considered the consequence of plant burning, would suggest the presence of vegetation.
The dinosaur footprints were printed in two different paleoenvironments in a palaeogeographic contest of a tidal flat placed at the margins of a continent. The calcareous levels are characterized by the alternation of subaerial exposures and the development of ephemeral lenses of fresh or brackish waters. The dolomitic levels correspond to marine transgressions and a higher influence of salty waters.
Plant remains (thin lignite beds, root fragments) are scarce but present in the Membro Inferiore. Besides sedimentologic evidence of pedogenesis are often found on the surfaces bearing the dinosaur footprints. This means that plants were present in the semiarid environment of the Lavini di Marco.
THE MECHANISMS OF PRESERVATION OF THE FOOTPRINTS
The main factor influencing the preservation of the footprints is the nature of the printed sediments. The preservation on the top surface of level 106 was probably caused by two main events: hardening of the substrate due to long subaerial exposition and subsequent covering by mud due to the transgression which deposited the level 107. The substrate deformed by the footprints in the “colatoio Chemini” was a “sandwich” of plastic, semilithified sediments, elastic cianobacterial laminae and semiliquid muds from levels 105 and 106. The mechanical features of the cianobacterial mat avoided the mud to fill the print after foot withdrawal. Marine water soon soaked the deformed sediment; this favoured its early cementation and the preservation of the footprints.
THE CONTRIBUTION OF SEDIMENTOLOGY TO THE STUDY OF THE DINOSAUR FOOTPRINTS AT THE LAVINI DI MARCO
Thanks to the sedimentologic study it was possible to identify some reference levels outcropping over wide areas of the Lavini di Marco and to recognize the sequence of the levels with footprints. Sedimentologic features permitted the reconstruction the sequence in which the dinosaurs traversed some parts of the site and the sedimentologic analysis shows that it is very difficult to state on which surface the animals actually walked, since underprints are formed into many other surfaces. Sometimes it is possible to recognize the space and temporal association of two prints, as is the case of the sauropod track ROLM75 which preserves the print of a theropod on the expulsion rim of a footprint. The tracks disappear when they reach dry areas like those where mud-cracks are found. A footprint left in very fluid mud has more chance of being preserved, and more so, as an underprint in the underlying more cohesive layer, because of the collapse of the fluid mud and the infilling of the depression. In the case of quadrupedal tracks at some outcropping places of level 106 (e.g. ROLM1 and ROLM2), the manual prints were much shallower than pedal prints and left a shallow or no underprint at all. The erosion of the original printed surface led to the preservation of apparently semi-bipedal tracks which in turn caused the wrong preliminary identification of the trackmaker. Cianobacterial mats are more suitable for the good preservation of true prints because of their mechanical properties. The slippery nature of the surface was probably responsible of the slow gait of the trackmakers, the different lengths of consecutive paces and the dragging marks.
PART III - TETRAPOD PALEONTOLOGY OF ITALY AND NEIGHBOURING COUNTRIES
10
Giuseppe LEONARDI
THE DINOSAURS OF ITALY AND NEIGHBOURING COUNTRIES
INTRODUCTION
Ten years ago Italy was considered a country almost without dinosaur evidence. This view of things changed after the publication of a paper by Mietto (1988) regarding Triassic dinosaurian tracks in the Dolomites and, above all, after the discovery of the Lavini di Marco site. Even if Italy is not very rich in dinosaur evidence, about a dozen of tracksites and two sites with bones have been found.
ITALIAN DINOSAURS
THE DINOSAURS OF THE LAVINI DI MARCO
They are considered here in chapter 8. They were numerous, diversified and sometimes large-sized. In order of decreasing frequency, there were ceratosaurian theropods, sauropods (Vulcanodontidae or primitive Cetiosauridae), advanced ornithopods and primitive ornithopods. Those of Lavini di Marco are the most abundant ichnologic sample in Italy.
CARNIAN (UPPER TRIASSIC) DINOSAURS
Mts Pisani (Agnano, Pisa; codex: AGPM = Agnano-Monti Pisani)
The most ancient dinosaur of Italy is represented by a single, small (6-7 cm long) tridactyl footprint described as Coelurosaurichnus toscanus by Friederich von Huene (1941). The specimen comes from the Quarziti Viola Zonate at the top of the Quarziti di Monte Serra, clastic sediments of deltaic plain of Late Carnian age. Leonardi & Lockley (1995) showed that this footprint is attributable to Grallator.
Lerici (La Spezia)
Here a rather rich footprint association is preserved (see chapter 11). Dinosaurs are represented by some footprints and short tracks attributable to Grallator and/or Anomoepus or Pseudotetrasauropus. The footprints are in the upper part of the Formazione di Montemarcello (Middle Carnian or Norian).
UPPERMOST CARNIAN AND NORIAN (UPPER TRIASSIC) DINOSAURS
Mt Pelmetto (Dolomiti, Belluno; codex: ZAMP = Zoldo Alto-Monte Pelmetto)
The dinosaur footprints in this site are preserved mainly on the surface of a large boulder fallen from the overhanging rocky wall. The original position was at the base of the Dolomia Principale, near the passage to the Formazione di Raibl (Upper Carnian). Three tracks were attributed to small theropods (footprint length = 6-7 cm), another track to a small-size (footprint length = 10-12 cm) primitive ornithischian; a track left by a larger (footprint diameter = about 15 cm) and semibipedal trackmaker was identified as possibly prosauropodian (Mietto, 1988). Many single tridactyl footprints were found on other blocks (P. Mietto, pers. comm).
Tre Cime di Lavaredo (Dolomiti, Belluno; codex: AUTC = Auronzo-Tre Cime)
Here there is a boulder from the Dolomia Principale with a short track (two tridactyl footprints 30 cm long) attributed to Eubrontes (Mietto, 1992).
Puez (Altopiano del Puez, Selva Val Gardena, Bolzano; codex SEPU=Selva Val Gardena-Puez)
In this site there is a probable mid-size tridactyl footprint on a bed surface of the Dolomia Principale (Leonardi & Avanzini, 1994).
Cellina Valley (Pordenone)
Two large tridactyl footprints have been found near Casera Cjasevent. At least another seven boulders with dinosaur footprints are present in the surrounding region (Dalla Vecchia & Mietto, 1998). They all come from the Dolomia Principale.
Other localities
Paolo Mietto has discovered many Carnian and Norian sites in the Eastern Dolomites, mainly with poorly preserved footprints.
JURASSIC DINOSAURS
Chizzola (Ala, Trento; codex ALCH=Ala-Chizzola)
About 3 km before of the site of the Lavini di Marco and belonging to the Calcari Grigi, a large (length = 33 cm) footprint classified here as Eubrontes, and other two tridactyl footprints were found in 1994. They were destroyed by public works in recent times.
Northern Mts Lessini (= Alti Lessini) (Verona, codex VRBL=Verona-Bella Lasta)
Mietto & Roghi (1994) and Roghi (1994) reported the presence of two levels with tridactyl footprints in the “Bella Lasta” area of Mts Lessini. The best preserved footprint, 30 cm long, was attributed to a large ornithopod. This site is more recent than that of the Lavini di Marco, and belongs to the mid-upper part of the Calcari Grigi (Pliensbachian).
Becco di Filadonna (Trento)
Some tens of dinosaur footprints (large tridactyl footprints and a sauropod pair) have been found in this locality near Trento (Avanzini, 1998). The site is slightly younger (base of the Membro Medio of the Calcari Grigi, late Sinemurian) than that of the Lavini di Marco.
Other localities
Marco Avanzini has discovered new dinosaur footprints in the Calcari Grigi of Mt Pasubio and Mts Lessini.
CRETACEOUS DINOSAURS
Porto Corsini (Ravenna)
(Lower Cretaceous - Upper Hauterivian/Lower Barremian)
A large (36 cm long) theropod footprint and a sauropod manual print were found in a limestone boulder at the pier of Porto Corsini (Dalla Vecchia & Venturini, 1995; Dalla Vecchia, 1998). The boulder was quarried at the base of the Cansiglio Plateau (Carnic Pre-alps, Pordenone) in the Calcare di Cellina Formation.
Mt Bernadia (Nimis, Udine)
(Lower Cretaceous - Aptian)
Possible cross-sections of dinosaur footprints are exposed in this site (Venturini, 1995; Dalla Vecchia & Venturini, 1995).
Pietraroia (Benevento)
(Lower Cretaceous - Aptian, Albian)
A nearly complete (the tail is mostly lacking as are the distal hind limbs), articulated skeleton of a very small dinosaur was found at this site and was described and identified by Leonardi & Teruzzi (1994) as a juvenile theropod belonging to the Maniraptora clade. The most striking feature is the preservation of some soft parts such as muscle fibres, the intestine and possibly the liver. For this specimen the taxon Scipionyx samniticus was later instituted, and it was described in detail by C. Dal Sasso and M. Signore in Nature, March 1998.
Villaggio del Pescatore (Duino, Trieste)
(Upper Cretaceous - Senonian)
This site preserves bone remains belonging to Hadrosauria, distributed at different levels (Dalla Vecchia, pers. comm.).
NEIGHBOURING COUNTRIES
SWITZERLAND
More than 800 footprints are preserved in the Ladinian-Carnian at Vieux Emosson, Vallese Canton. Brachychirotherium Beurlen, Isochirotherium and dinosauroid footprints are present. The very badly preserved dinosauroid footprints are perhaps tridactyl, tetradactyl and pentadactyl, testifying to the high diversity of the ichnofauna.
Thirteen tracks are exposed in the Grigioni National Park of Engandina along the western flank of the Piz dal Diavel (Furrer, 1984). The footprints, mainly large tridactyl and dinosauroid, are preserved in the Norian Diavel Formation. A long track with large tetradactyl footprints was attributed to prosauropods.
ISTRIA (CROATIA) AND SLOVENIA
Sauropod bones have recently been discovered in the Upper Hauterivian-Lower Barremian limestones of Southern Istria (Dalla Vecchia, 1994b). Dinosaur footprints are common in the Cretaceous of Istria. Large theropod footprints of Late Barremian age are exposed along the shore of the Main Brioni Island, Southern Istria. Albian tridactyl footprints most of which belong to mid-sized theropods have been found in two sites of the Main Brioni Island and other three sites along the coast of the peninsula (Dalla Vecchia & Tarlao, 1995; Dalla Vecchia et al., 1993). In the Fenoliga Islet (Southern Istria) a long track attributed to a sauropod (Leghissa & Leonardi, 1990) is preserved, together with theropod tracks, on an Upper Cenomanian limestone bed (Gogala, 1975; Gogala & Pavlovec, 1978; Pavlovec & Gogala, 1992).
A track left by a large reptile, probably a dinosaur, preserved in Norian-Rhetian dolostones, is reported from the environs of Idrija, Slovenia (Dalla Vecchia, 1997).
PALEOGEOGRAPHICAL AND PALEOENVIRONMENTAL CONSIDERATIONS
The discoveries of abundant dinosaur evidence in the examined region put up for discussion the previous paleogeographical and paleoenvironmental reconstructions, which pointed to a generalized presence of shallow marine environments. In fact, the dinosaur faunas needed sufficiently wide emerged areas, covered by vegetation and with fresh water, for their survival.
11
M. A. CONTI, Giuseppe LEONARDI, Paolo MIETTO and Umberto NICOSIA
FOOTPRINTS OF NON-DINOSAURIAN TETRAPODS IN THE PALEOZOIC AND MESOZOIC OF ITALY
Researches carried on during the last 30 years have shown that tetrapod footprints are relatively common in the Upper Paleozoic and Triassic rocks of Sardinia and Northern Italy. In this contribution they are grouped following a chronological order.
CARBONIFEROUS ICHNOFAUNAS
Footprints attributed to small microsaur amphibians (Salichnium heringi (Geinitz)) were found in the Upper Carboniferous of Sardinia. Two footprints attributed to Limnopus sp. and Hylopus cf. H. hardingi Dawson come from the Upper Carboniferous of Carnia (NE Italy).
LOWER PERMIAN ICHNOFAUNAS
The Lower Permian ichnological record comes from the Collio Formation of Eastern Lombardy (Val Trompia and Orobian basin) and Western Trentino (Tregiovo). This ichnofauna is revised here and is composed of: Antichnium salamandroides, Camunipes cassinisi, Dromopus lacertoides, D. didactylus, Amphisauropus latus, Ichniotherium cottae, Anhomoichnium orobicum, and an unidentified amphibian and lacertoid ichnotaxon. They belong to two small amphibian taxa, a relatively large plant-eating reptile and six small reptilian taxa. Temnospondylian amphibians, Captorhinida, Araeoscelida, Lepidosauromorpha, Pelicosauria and perhaps Diadectidae are represented.
UPPER PERMIAN ICHNOFAUNAS
A peculiar and very important ichnofauna is that of the Val Gardena Sandstone of NE Italy, dated to 255-265 m.y.a (Changxingian-Djulfian). Footprints have been found mainly in the provinces of Bolzano/Bozen and Trento but specimens also come from the environs of Recoaro (Vicenza) and Carnia (Udine). A revised list of the ichnotaxa and their supposed makers is given in Italian text-fig. 11.12. All footprints belong to reptiles: large plant-eaters such as pareiasaurs (Pachypes dolomiticus), mid-sized plant-eaters like pelicosaurian caseids, large predators like the gorgonopsians and possibly also primitive “thecodonts” (the oldest chirotheroid footprints) and small predators like the primitive cynodonts (Dicynodontipus). Small lacertoid reptiles of uncertain diet are represented by Hyloidichnus tirolensis, Paradoxichnium, Rhynchosauroides (very common), Janusichnium and footprints attributed to Procolophonomorpha.
TRIASSIC ICHNOFAUNAS
LOWER TRIASSIC - Footprints were found in the Werfen Formation of Dolomites, Recoaro area (Vicenza) and Carnia (Udine). Most of them are identifiable as Rhynchosauroides.
LOWER ANISIAN - Rhynchosauroides and Parasynaptichnium gracilis were found in the Gracilis Formation of Recoaro area (Vicenza). Rhynchosauroides is also present in the Conglomerato di Voltago of Valsugana (Trento).
UPPER ANISIAN - The Conglomerato di Richtofen of the Pusteria Valley, Upper Adige Valley, Western Dolomites (Alto Adige) and Eastern Dolomites and the equivalent Conglomerato del Tretto of Recoaro area yielded Rhynchosauroides tirolicus, Chirotheriun cf. rex, Brachychirotherium aff. B. parvum, Synaptichnium sp. and Rotodactylus sp.
UPPER TRIASSIC - Vertebrate footprints are reported from many sites in Northern Italy. Dinosaur footprints and the sites with dinosaur footprints are described in chapter 10.
A rich ichnofauna was found at Mt. Pisano (Pisa and Lucca). It is composed of footprints of a presumed urodelian amphibian and rhynchosauroid and chirotherian footprints; at present it is under revision. The specimens come from the Quarziti Viola Zonate at the top of the Quarziti di Monte Serra, clastic deltaic plain sediments of Early Carnian age.
Archosaurian tracks were found recently in the Upper Carnian marl-dolostone alternations of Dogna valley (Valcanale, Udine province) (Dalla Vecchia, 1996).
A site in the environs of Lerici (La Spezia) is under study. There are two bipedal, tridactyl or tetradactyl dinosaur ichnotaxa, tridactyl footprints with a very developed central digit and stout nails, large Brachychirotherium Beurlen, a smaller chirotheroid taxon, some large footprints with a vaguely chirotherian aspect left by a quadrupedal animal, and many mid-sized footprints of uncertain attribution. The clastic levels with footprints belong to the upper part of the Montemarcello Formation (possibly Middle Carnian or Norian).
A chirotheriod footprint was found in the Upper Carnian site of M. Pelmetto (see chapter 10). “Thecodont”, poorly preserved footprints are found in the Late Carnian Dolomia di Dürrestein of Dolomites.
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12
Fabio Marco DALLA VECCHIA
BONE REMAINS OF PALEOZOIC AND MESOZOIC TETRAPODS IN ITALY
Italy is usually considered a country poor in bone remains of Paleozoic and Mesozoic terrestrial tetrapods. However, the Italian tetrapod record (including truly terrestrial, fresh water, coastal and flying tetrapods) is noteworthy, even if bone remains are not very common. From a systematic point of view most of the main Linnean groups are represented.
Temnospondylian amphibians (Metoposaurus H.v. Meyer) are known from the Ladinian and Carnian of Alto Adige/Süd Tirol; Urodela (Celtedens megacephalum (Costa)) from the Albian of Southern Italy (Pietraroia, Benevento).
Reptilia are much more common.
Remains of non-marine Chelonia are present in the Upper Cretaceous of the Italian Karst (Carso) and Puglia region.
Drepanosaurus unguicaudatus Pinna is a Diapsida incertae sedis from the middle Norian of Lombardy. Sphenodonta were found in the Norian of Lombardy and, with some doubt, in the Albian of Southern Italy (Chometokadmon fitzingeri Costa; Pietraroia, Benevento). In the same localities and formations Squamata (Vallesaurus cenensis Wild, Norian; Costasaurus rusconi (Costa), Albian) were also found.
Protorosauria (Prolacertiformes) are well represented mainly in the Anisian/Ladinian of Lombardy and near Tessin with Tanystropheus longobardicus (Bassani) and Macrocnemus bassanii Nopcsa. Bones belonging to Tanystropheus were also found in the uppermost Ladinian and Upper Norian (T. fossai Wild) of Lombardy, and in the Carnian of Friuli (NE Italy). Langobardisaurus Renesto is present in the middle Norian (Alaun) of Friuli and Lombardy.
Megalancosaurus preonensis Calzavara et al. is a small, strange “thecodont” of uncertain taxonomic position from the middle Norian of Friuli and Lombardy.
The predator rauisuchian Ticinosuchus ferox Krebs is present in the Anisian/Ladinian of Lombardy and near Tessin, and possible dorsal scutes of rauisuchians are present in the Carnian of Alto Adige/Süd Tirol. The plant-eatinf aetosaurs are represented by remains of Aetosaurus ferratus Fraas found in the middle Norian of Lombardy. The crocodile-like phytosaurs are testified to mainly by a complete skull and lower jaw of Mystriosuchus planirostris (H.v.Meyer) from the middle Norian of Lombardy.
Rare is the evidence of non-marine crocodiles: remains of small individuals were found in the Albian of Southern Italy (Pietraroia, Benevento) and in the Senonian of Italian Karst (Duino, Trieste).
Pterosaurs are perhaps the most interesting mesozoic reptiles of Italy. The oldest pterosaurs found up to now in the World come from the Middle Norian of Friuli and Lombardy (Preondactylus buffarinii Wild, Peteinosaurus zambellii Wild, Eudimorphodon ranzii Zambelli and E. rosenfeldi Dalla Vecchia). Dinosaurs, found in the Cretaceous of Campania (Pietraroia, Benevento) and Venezia Giulia (Duino, Trieste), are described elsewhere in this book.
Therapsids could be represented by a jaw with tricuspidate teeth from the Carnian of Dolomites, which could alternatively belong to an immature prolacertiform.
Coastal reptiles, i.e. animals not very well adapted to aquatic life, are rather common mainly in the Triassic.
Nothosauria and Placodontia bones and skeletons are abundant in the Middle Triassic (mainly in Lombardy but also in Veneto and Friuli regions), and Carnian (Alto Adige/Süd Tirol and Friuli). Placodontia are also present in the Norian and Rhetian of Lombardy.
Thalattosauria is a particularly diversified group in the Anisian/Ladinian of Lombardy and near Tessin. Endennasaurus acutirostris Renesto was found in the Middle Norian of Lombardy.
Finally, remains probably belonging to a coastal varanoid was reported from the Upper Cretaceous of Puglia.
PART IV - OTHER CONTRIBUTIONS
13
Giuseppe OROMBELLI and Ugo SAURO (with the contribution of F. FERRARESE)
GEOMORPHOLOGICAL ASPECTS OF THE LANDSLIDES OF MT ZUGNA
The Mt Zugna is a N-S, approximately 10 km long ridge made up of a homoclinalic block with a 20° average slope of the strata (which is about the same immersion of the slope) and a W and NW dip.
The main landslide called “i Lavini”, is composed of a wide scar on the flank of the mountain and a broad accumulation at the base of the slope and in the Adige valley below. The whole landslide complex of Mt Zugna is not a unique body but is formed by different landslide accumulations. There are another seven lesser landslides: two landslides at Corna Calda, the landslide of Doss delle Gardene, a landslide at an altitude of 772 m SSE of the Damiano Chiesa cave, the Marco landslide, the Varini landslide and the landslide ok km 346 along State road n.12. Here is some data on the main landslide: length of the fallen part = 5200 m , width of the same =2300 m, thickness = less than 100 m, mean probably less than 20-30 m, total length = 5600 m, maximum difference in height = 1150 m (from 1320 to 170 m a.s.l.). The use of software such as the Geographical Information System (G.I.S.) permitted the estimation of the volume of the landslide accumulations down in the valley (excluding those accumulated on the flanks) of the Lavini, Pinera, Marco and Varini as being about 41.000.000 m3. They extend over a surface of 3.78 km2, with a mean thickness of 10.95 m. The area of depletion for the main (Lavini) accumulation body is about 1.80 km2, with a mean accumulation thickness of 17.5 m.
The accumulation of the main body covers the alluvioni and the terraces of the Adige river therefore the landslide is a postglacial event. The minor landslide of Varini covers soil dated by 14C to 1300 ±100 B.P. (580-895 a.d. following the calibration of Klein et al., 1982). Soil below the landslide of altitude 772 m was dated 5630±80 B.P. The blocks of the main accumulation on the valley bottom shows only embrional corrosion microstructures and degradation of the niche surface is poorly developed (similar to the Varini landslide), both pointing to the recent age of the landslide. The conclusion is that all these landslides are very recent, with an age ranging between 1000 and 2000 years ago, probably between 800 a.d and 1117 a.d.. Only the landslide of altitude 772 m and the southern Corna Calda landslide are older.
Most of the landslides of Mt Zugna can be classified as block rockslides, some of which evolved in debris flow or debris avalanches. The difference in height ranges 300 to 1200 m and the distances passed across are between several tens of metres and 6 km.
The main landslide originated due to the detaching of a set of strata in the upper part of the niche, the thrust of which caused the removal of the corresponding strata downslope. This body began to move as a block, afterwards disintegrating progressively into slabs and boulders and then into finer material. The Costa Stenda ridge divided the body into two parts, the lesser directed to the west forming the lobe of Marco, the large to NW to form the main accumulation of “i Lavini”. The main body slowed down in the funnel-shaped depression delimited by Costa Stenda ridge and Costa Violina ridge (fault of the Vallone and of Lizzana). This bottleneck caused overbanking, the overcoming of the obstacle of Costa Stenda, with the removal of the top of the relief. This removed part broke into large blocks which now constitute the spectacular chaotic accumulation of the “Ruina” of Pinera, just north of Marco. The main body went beyond the depression and expanded at the base of the mountain over the Adige valley bed, stopping nearly two kilometres from the base of the slope.
A sismical shake is considered the most probable cause of these landslides.
14
Marco AVANZINI and Dario ZAMPIERI
THE LAVINI DI MARCO: GEOLOGIC-STRUCTURAL ASPECTS
Between 165 and 130 million years ago the Adriatic (or Apulian) passive continental margin where the Trento Platform was located, saw the opening of the relatively small Ligurian Ocean, separating Laurasia and Africa. The plate movement, initially divergent, at a certain point became convergent, with an abrupt acceleration 85 m.y.a. About 60 m.y.a the convergent movement led. to the closing and disappearance of the ocean with the deformation of the relative sediments against the European continental margin. The collision between European and African Plates caused the rising of the Alpine mountain chain, mainly during the Neogene. The section of Southern Alps including the Trento Platform was characterized by strong crustal shortening, with overthrustings of scales of marine carbonates which forms the present orography of the zone.
The Southern Alps are that part of the Alpine chain placed south of the Insubric Line, running W to E from the Bergamasc Alps to the Pusteria Valley. They are formed by overthrusts directed S-SE.
During Mesozoic times the future Southern Alps were part of the margin of the Tethysian Gulf separating the Gondwana from Laurasia. During the Late Jurassic the region rifted. The rifting structures strongly influenced the successive tectonical evolution of Southern Alps. The Lavini di Marco are placed at the margin of a distensive belt produced by the Jurassic rifting, which separated the Lombardian Basin and the Trento Platform. The progressive drowning of the Platform caused by the rifting advanced from W to E.
Southern Trentino is now characterized by large folds and overthrusts oriented N-NE, known as the “structural system of the Giudicarie”. It represents the reactivation of the W dipping Jurassic distensive faults which created the margin between Lombardian Basin and the Trento Platform. Structural systems with different directions of compression (E-NE, E-W; N-NE; NW-SE) overlap in the area. The Lavini di Marco are placed in the peripheral zone of deformation of the Giudicarie system.
The Mt Zugna-Zugna Torta is a homoclinal structure, therefore a block with stratification dipping always in the same direction. The average dip of strata on the W flank where the landslide developed is the same as the average sloping of the topographical surface.
The flanks of the niche of the main landslide is delimited by two slopes (ridges) which are set in correspondence to two subvertical transcurrent faults (Vallone fault and Lizzana fault) which converge into a single structure near the Damiano Chiesa cave. There are three hinges (homoclinal folds) and are parallel to the vertical ridge of the eastern flank of the niche. They are therefore spatially and genetically associated to the Vallone Fault. They are characterized by a single bed surface with a deeply sloping (up to 60°) tract, which connects the upslope, and downslope with tracts dipping like the slope inside the niche (20-25°). They were caused by the left transpression of the fault; they are the superficial result of a somewhat asymmetrical flower-like structure where the thrust faults created by the transpression do not reach the surface.
The calcite veins found inside the niche are oriented NNW and WNW (with the data reported to the original horizontal position of the strata). These two directions represent the directions of maximum horizontal compressive stress.
The deformation structures in the Lavini di Marco rocks are of two types: those produced before the landslide event (the homocline of the mount, the faults, flexures and the system of veins) and those caused by it ( superficial folds, tensional flexures) or after it.
15
Oscar GROAZ and Luigi VERONESE
HISTORICAL AND INSTRUMENTAL SEISMICITY IN THE LAGARINA VALLEY
The Lagarina Valley does not present the high seismicity of the neighbouring Lake Garda region and the Belluno-Friuli area. According to historical records, the big medieval earthquakes (1117, 1222, 1348) caused damage in this area, as well as in many other areas of northern Italy. Other historical records concern the earthquakes of 1868, 1888 and 1895. Probably the estimated intensity was never higher than the grade 7 of the Mercalli Scale, as the descriptions suggest. The instrumental data are in agreement with this pattern. The main events were on 1968 (6 grade of the M. S.), 1983 and 1989 (6-7 grade of the M. S.).
16
Paolo ARZARELLO, Franco FINOTTI, Giorgio GALEAZZO, Michele LANZINGER, Maurizio MEZZANOTTE and Luigi VERONESE
THE PARK OF THE ROVERETO DINOSAUR TRACK: PRESERVATION, EXPLOITATION AND TRANSFORMATION INTO AN OPEN-AIR MUSEUM
A modern Museum is no longer only the place where material is stored and exhibited but is an instrument for the divulgation and communication of knowledge. This “global” Museum promotes interaction between the users (the citizens) and the territory. Our aim is the realization of an open-air museum at the dinosaur site of the Lavini di Marco.
VIBROMETRIC PROSPECTING
In May 1992 vibrometric investigations were made to estimate the damage that artificial explosions could cause to the footprints. In fact, two places where military bomb-disposal experts blast war surplus are situated in the Lavini area. The results tell us that the risk of alteration of the layers with the footprints is very limited.
FOTOGRAMMETRIC SURVEYING
A fotogrammetric survey was made in order to have a precise and objective map of the layers with the footprints. The geometric survey concerned nine tracks considered to be the most important by the Management of the Civic Museum of Rovereto: ROLM 63, 64, 75 on 1993, ROLM 1, 2, 9, 11, 12, 26 on 1994.
CASTING OF THE FOOTPRINTS
Casts were made of the most important tracks and footprints to prevent the loss of data and source evidence due to the rapid weathering of the limestone. Six tracks were cast: ROLM9, 11, 12, 63. 64, 75. Some parts of the footprints where consolidated with low-concentration Paraloid@ and the surfaces were covered with Trecon Ag@ to better detach the silicon rubber cast. Several layers of the silicon rubber Trecosil 755@ were spread by a brush. This rubber hardens in about 12 hours at a temperature of 15°celsius. A countercast was made with fibreglass and polyester. A mould was realized from the cast using polyester resin added with calcium carbonate and reinforced with mat.
THE PALEONTOLOGICAL TREK OF THE DINOSAURIAN TRACKS
The paleontological importance of the site has as a consequence aroused the interest of many persons. Therefore the problem arose of how to allow scientists, students, tourists, etc to visit the site while satisfying the necessity of protecting the surrounding landscape.
A track was prepared with tables placed at the most meaningful stops to explain the dinosaur tracks and their probable makers to the uninformed tourist. This track allows the tracks along the colatoi without to be seen without trampling on them. It begins at the colatoio Chemini where tracks can be seen in two different areas from elevated stopping places. One side of the colatoio is protected by a low fence. The colatoio was drained to avoid damage caused by flooding. The track also reaches the zone of the “hinge” up along the flank of the mountain. Then it circles around and ends at the starting point.
This route will be improved with regards scientific information by the setting up of explanatory panels.
17 The Lavini di Marco site: an overview
Marco Avanzini, Giuseppe Leonardi, Daniele Masetti and Paolo Mietto
Up until 10 years ago the only evidence of the presence of dinosaurs in Italy was represented by a single footprint of a small predator from the Carnian (Late Triassic) (Carnian terrains), at Monti Pisani.
This apparent total lack of dinosaur fossils was explained by the fact that during the Mesozoic the Italian paleography was dominated by a prevalence of areas submerged by the sea.
In recent years it has been possible to completely refute this prejudice and today we know that the presence of dinosaurs in Italy is documented from the beginning of their evolutionary history to the end. Numerous sites, have been discovered in Trentino, Veneto and Friuli, and also in various Apennine areas in Liguria, Tuscany, Campania and in Puglia’s Murge range, as well as close to Italy’s borders within other countries.
This evidence is mainly limited to tracks, but also includes bone remains and has led to a profound and critical revision of the paleogeographic reconstruction of our country during the Mesozoic especially with regards to the large animal associations represented by the tracks such as those at the Lavini di Marco.
The phenomenon is not restricted to dinosaurs: the presence of tracks of continental vertebrates are documented in many parts of Italy from the upper Palaeozoic to the end of the Mesozoic. Today we have a mass of data available that allows us to document the presence of amphibian but mainly reptile fauna, in the continental environments of the Permo- Carboniferous, in innumerable continental layers that interrupt the continuity of the succession of the strictly marine Triassic, in Triassic and then Jurassic tidal flats. This results in an extremely diversified, rich and in some respects unexpected overall picture. There is no lack of bone remains of continental vertebrates (amphibians, land and flying reptiles), from the Palaeozoic and Mesozoic terrains, even though in truth body fossils of dinosaurs are still very rare. These are faunistic associations consistently and systematically repeated over time, which suggests the existence of an environment favourable to continental tetrapod life.
The area that has to date produced the greatest amount of dinosaur evidence is that of the Lavini di Marco, which is close to the town of Rovereto in southern Trentino. The Lavini di Marco are a series of landslides that detached themselves from the slopes of Monte Zugna about 1200 years ago. The landscape is particularly harsh and desolate, and since Mediaeval times it has represented a challenge to the comprehension of this phenomenon. Today the area still poses a large number of questions and represents, after the discovery of the tracks, a key site to understanding paleogeography, the paleoenvironment and the paleobiology not only of this area and the fauna it conserves but also for the whole Trento Platform and the Southern Alps.
The data recovered to date at the Lavini during eight years of research provides us with a window into a lost world. On six stratigraphical levels, compressed into just 5 metres and in an area of little more than a quarter of a square kilometer, there are footprints and trackways of a large number of carnivorous and herbivorous dinosaurs of various forms and sizes. The number of individuals has still to be defined but it is well over 200 animals.
It all took place almost at the beginning of the Jurassic and more probably in the early Sinemurian, on a large tidal flat which in many ways is comparable to the present coastline of the Persian Gulf.
Many carnivorous theropods attributable to all the several forms of ceratosaurs, of small, medium and large sizes, from 1 to 9 meters long, accompanied - or rather, followed by - a large number of small or large herbivores. Identified amongst these with a certain amount of surprise are a score or so of sauropods, that are up to now the oldest ever found in the world, weighing from 1 to 3 tons, and probably evolved ornithopods, of large dimensions with graviportal hind legs. These latter are not known from the bone remains found in this portion of the Jurassic period, which constitutes a separate problem that has yet to be solved.
Paleontological studies of our material have not only identified the possible authors of the tracks, but have also allowed their comparison with the contemporary ichnofaunas and faunas of the whole world, and have led to a series of considerations, that are in many ways completely new. Many particularly interesting aspects have emerged: the social behavior of the individual, its posture, gait and speed, the directions followed which contribute towards the outlining of some preferential corridors and then of some details of the paleogeography of that time in an extraordinary manner.
Carnivore tracks are more numerous (57%), than those of the herbivores (43%), notwithstanding what the biomass pyramid theory would forecast. This inversion of data probably needs to be placed in relation to the higher level of activity of carnivores than herbivores.
As often occurs in fossil fauna, the presence of hatchling and juvenile individuals is quite rare, and our ichnoassociation is mainly made up of adults, which is also probably because young animals do not leave deep tracks in the sediments and those they did leave would be more easily washed away or eroded.
The carnivores are documented by tracks that vary in length from 8 to 38 centimeters. The examples with smaller body sizes would not have been longer than half a meter, with a body weight of 3 to 4 kilos. The larger carnivores were probably 8 to 9 meters in length and weighed up to 1200 kilos. Among the herbivores, the sauropods for example have left tracks from 35 to 50 cm long, which were left by animals of 7 to 10 meters in length, weighing from 1 to 3 tons.
Animals like these latter undoubtedly consumed a large amount of vegetation. If considered to be “cold blooded” their daily foraging needs would have been modest, from 3 to 9 kilos. If considered “warm blooded” their
needs would have been between 21 and 64 kilos. Whatever the needs the annual consumption of plants would have been impressive.
It was particularly interesting to make a detailed study, of the interrelations between the different groups, and expand them to the world of the hypothetical small and medium sized tetrapods (mesofauna) and marine and continental invertebrates; and finally to the plant world, which is the basis for all animal life.
This latter topic, inserted into a paleogeographic and paleoenvironmental framework, poses a series of questions that are not easily answered as it would appear that there is an absence of the fundamental presupposition that would justify the presence of dinosaurs - especially the large herbivores - in an environment like that reconstructed for Rovereto: the vegetation. It would not appear to be justified to imagine, at the current state of our knowledge, that in the area of the tidal flats of the Lavini di Marco, there was sufficient plant biomass to sustain these large animals. This remains, therefore, the theme on which all current research is concentrated, as well as that foreseen for the immediate future.
It was possible to identify in this field, from amongst the large amount of data collected, two different environmental situations within a larger paleogeographical context of a tidal flat situated at the edge of a continent. The calcareous footprint bearing levels are characterized by the alternation of subareal exposures at the moment in which small amounts of water (both fresh and saltwater) develop on the platform. Analysis of the dolomitized footprint bearing layers, would seem to indicate the approach of the coastline - even if we do not know its exact location - and therefore the hypothesizing of different diagenetic mechanisms. There is also no lack of evidence of more marked subareas at particular times and in areas that are further away from the sea. In general therefore, the environment was characterized by cyclic excursions of the sea level which forced the dinosaurs to adapt to different conditions.
From an alimentary viewpoint, sedimentological and geochemical analysis does not justify the presence of so many dinosaurs in such an inhospitable environment, which was without the ideal vegetation cover essential for the survival of large herbivores.
In summary, sedimentological and diagenetic analysis shows that the geological features of the Lavini di Marco identifies a tidal flat where there was cyclic fluctuations in the sea levels. This tidal flat was characterized by a semi-arid climate and by the presence of slow moving fresh water as indicated by geochemical data.
It is therefore inevitable for one to pose the following question:
Did these dinosaurs live there as would seem logical to assume or were they just passing through? If they were passing through where did they come from? We have debated these questions from the first to the last day of these eight years of research.
Experts in sedimentary fossil environments have passed sentence: the Calcari Grigi at the Lavini di Marco identify an environment very similar to those tidal flats presently found in certain arid tropical areas and southern seas islands. Excellent exotic holiday locations for rich tourists; but with so little vegetation cover the survival of large herbivore dinosaurs would have been problematical. It would also seem that the tidal flat had a semi-arid climate, even harsher than first thought, with a chronic shortage of freshwater.
On the other hand dinosaur experts have declared: that there is no doubt that large herbivores lived on these flats and would have needed many thousands of tons of forage each year to survive and it is difficult that they would have been content with conditions that were so harsh.
The problem is further complicated by the enormous diffusion that carbonate platform environments had during the Early Liassic. Flat plains covered a large part of what is Italy today with small differences in facies. Not one area in Italy, at least not to the knowledge of the authors, features plant fossil content that would make it a candidate, at least according to traditional concepts, as a place for the development of dinosaur fauna similar to the one found at the Lavini di Marco.
Paleoenvironmental analysis clearly evidences that the Liassic carbonate platforms known in outcrops had no or very little vegetation, apart from bacterial moss. If this latter is excluded as a source of food for herbivore dinosaurs, we can only conclude that the mythical land of the
dinosaurs needs to be looked for several hundred kilometers from the Adige Valley. Unless.
All of our knowledge of the facies of platforms are based on the study of their characteristics in the area they appear. Although they are extensive, these areas present large interruptions in correspondence with the Padana and Veneto Plains. It is therefore possible that an area that had continental characteristics, that was habitually subaereal, with scarce vegetation, even forest trees, and was situated to the south of the pre-alpine area, below the present plains (Pianura Padana). A favorable clue to this is supplied by the paleogeography of the Middle Liassic.
Many definitely continental elements that are a feature of this stratigraphic unit, such as clay, carbon deposits derived from higher plants and the non-marine kerogene (an organic substance contained in bituminous rocks that give origin to oil), are distributed in such a way as to suggest their origins as being south of Monti Lessini, below the present Pianura Padana. It is clear that simple clues in a different era to that in which we are interested does not allow us to solve the problem. However, while awaiting new discoveries they do represent a working hypothesis to be taken into consideration.
However, even though this is only an hypothesis, a completely different scenario can be suggested. As often observed here, with little vegetation available, it would seem to be very difficult to justify the presence of large herbivores on the tidal flat in question - and this is also deduced from geological-stratigraphical data and the examination of similar environments of present times.
The problem also reappears for the dinosaur tracks that are also being found in large numbers in the older upper Triassic tidal flat of the Dolomia Principale. Hypothesizing that the Rovereto dinosaurs were in reality emigrants and just passing through would resolve the question of the lack of vegetation in tidal environments or at least it would move it elsewhere.
And what if the key to the solution would lie elsewhere? What else could have caused the large herbivores to come together in such an inhospitable environment? Given also that it had been ascertained that reptiles were not migratory by nature? If it was not food what was it? Perhaps instead food was a necessity linked to reproductive habits?
Available data is therefore contradictory. How can this impasse be resolved?
The migratory hypothesis could perhaps be admitted for large herbivores, mainly the sauropods, but it does not seem probable that all the fauna migrated, that is that all of the protagonists, both large and small, carnivores and herbivores, bipeds and quadrupeds from such different groups with such different needs were just passing through the site studied. If the heavy sauropods, weighing several tons, might have been able to survive a journey of many days, by sustaining themselves with
accumulated fat, perhaps contained in special storage organs, the same cannot be easily said of the small “fabrosaurids”; or for the carnivores, which generally do not migrate en masse together with the herbivores, but rather wait to ambush them as they pass. But one cannot say; we know so little about the lives of dinosaurs, when we try to go into detail! Above all on questions of metabolism, the debate between experts is still open and lively, and sometimes even leads to verbal abuse.
An alternative hypothesis that cannot be discounted is that the vegetation, even though present in small quantities in our area, existed here and there in greater concentrations, even if modest, in areas that have not yet been localised and perhaps together it was sufficient to feed the local fauna, at least for the small and large sized animals.
It is possible that the large number of tracks in the area does not represent so much an abundance of fauna, but wanderings in search of the small amount of food available, on the part of a smaller number of dinosaurs in respect to the more than 200 individuals we spoke of earlier. The mediocre or bad quality of the prints sometimes
does not allow the definite identification of individuals.
Documentation only exists for the terrain that is visible, while large surface areas are still invisible inside the mountain or have been destroyed by erosion. The continuity of the visible strata and the uniformity of the environment and the landscape would seem to be very probable, and in fact seems to be confirmed by the analyses carried out to date, but is not sufficiently representative of the whole truth, which still remains very complex.
Each layer in this environment obviously represents only a moment on the clock of geological time, while long intervals have not left a sign. Many layers were deposited and destroyed, redeposited and again destroyed, perhaps with their vegetation. Various inter-supratidal levels present the marks of destructive tidal movements and the frequent lack of stratification of the subtidal banks speaks of the eternal mobility and mutability of marine environments, that is unfavorable for the conservation of plants, especially those of small dimensions.
These are hypotheses that do not allow the contradictions of the data to be resolved in a convincing manner. But the data does exist; on one hand the dinosaur fauna with an impressive biomass, a harsh, sterile and apparently inhospitable environment on the other; both fascinating and stimulating, but when put together , disconcerting. The enigma that results, here at the Lavini di Marco and the platform of the Dolomia Principale Formation and elsewhere, is still a challenge to geologists and paleontologists, which has the advantage of keeping open research and enlivening intellectual curiosity, while this book is being finished.
In the eight years following the discovery of the dinosaur trackways at Rovereto, the research, notwithstanding the large requirement of personnel and equipment, has in practice been limited to a first still incomplete approach, which, however, has supplied a great deal of original data about the trackways, the authors of the prints and the environment, which allowed us to make many partial conclusions that we believe are worth publishing.
In the meantime, it is essential that the site is preserved. Therefore this initiative plays in important role not only in the cultural use of this immense patrimony, but also in its conservation for future generations.