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The Digital Terrain Model (DTM) and the evaluation of known and the search for new craters in the Chiemgau meteorite impact strewn field


Abstract and Figures

For several known and a few newly proposed meteorite craters in the Chiemgau meteorite impact strewn field the LiDAR data of the Digital Terrain Model DTM have been processed to reveal various maps and cross sections based on a high-resolution mesh down to 1 m and contour interval down to 0.2 m. The data processing highlights particular crater features that remain hidden in fieldwork and on conventional topographic maps and even may debunk mistaken structures.
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The Digital Terrain Model (DTM) and the evaluation of known and the
search for new craters in the Chiemgau meteorite impact strewn field.
Kord Ernstson (2017)
Abstract. - For several known and a few newly proposed meteorite craters in the Chiemgau
meteorite impact strewn field the LiDAR data of the Digital Terrain Model DTM have been
processed to reveal various maps and cross sections based on a high-resolution mesh down to
1 m and contour interval down to 0.2 m. The data processing highlights particular crater
features that remain hidden in fieldwork and on conventional topographic maps and even may
debunk mistaken structures.
Faculty of Philosophy I, University of Würzburg, Germany,
1 Introduction
2 The Chiemgau meteorite impact event
3 Data processing
3.1 Terrain imagery
3.2 Horizontal gradient
3.3 Data filtering
3.4 Cross sections
4 Examples
4.1 Small craters in the DTM
4.2 Peripheral depressions around small craters
4.3 Medium-sized craters in the DTM
4.4 Mistaken structures
5 A possible large-sized crater in the DTM
6 Discussion and conclusions
7 References
1 Introduction
Since some time the possibilities of the Digital Terrain Model (DTM), also termed Digital
Elevation Model (DEM) or Digital Surface Model (DSM) - in Germany: Digitales
Geländemodell (DGM) - have become an important tool for many purposes in the
geosciences of geography, geology and geophysics. Based on LiDAR data, topographic maps
in a regular grid down to spacing of 1 m and with highest altitude resolution down to 20 cm
(in Germany DGM 1) may be produced. Thereby the DTM represents the bare ground surface
without any objects like plants and buildings and may even be processed in thick forest (Fig.
Fig. 1. DTM shaded relief of a landslide in thick forest.
Frequently the DTM data can be gained from land surveying offices as digital (x, y, z)
files for standard coordinate systems (e.g., UTM). The data may then be processed by various
contouring and 3D surface mapping software producing maps as different as normal contour
maps, 3D surface maps, vector maps, wireframe maps or shaded relief maps. Processing may
elaborate the data files by various filter processes, computation of field gradients and
producing any desired elevation profile.
Here I shall illustrate the enormous possibilities of the DTM to explore the Chiemgau
(Germany) meteorite impact strewn field for new craters adding to the hitherto established
roughly 80 objects in the diameter range between a few meters and 600 m (rim to rim). The
DTM data processing is also applied to several craters already known for some time past. The
location map for the here-discussed sites is shown in the Appendix.
2 The Holocene Chiemgau meteorite impact event
The Chiemgau strewn field (Fig. 2/3) has originally been discovered some 15 years ago by a
group of local history researchers and amateur archeologists and has meanwhile been
established by all evidence of meteorite impact (Rappenglück, M.A. et al. 2013, 2014,
Rappenglück and Ernstson 2008, Ernstson and Rappenglück 2008, Ernstson et al. 2010,
2011a,b, 2012, 2013, 2014, Ernstson 2010, 2011, 2016, Isaenko et al. 2012, Shumilova et al.
2012, Hiltl et al. 2011, Bauer et al. 2013, Rappenglück, B. 2013, Rappenglück, B. et al. 2009,
2010, 2012, 2013, Liritzis et al. 2010) as is commonly and since fairly long time claimed
within the international impact research, and only sporadic opposition is still maintained
(Reimold & Koeberl 2014, Reimold et al. 2014, Doppler et al. 2011, Schmieder et al. 2011).
Fig. 2./ Fig.3. The Chiemgau impact strewn field in Bavaria (map to the right).
The impact evidence from mineralogical-petrologic, geochemical, geologic and
geophysical investigations has been featured by heavy rock deformations, melt rocks, strong
shock metamorphism, geophysical GPR, gravity and geomagnetic evidence, abundant
occurrence of metallic, glass and carboneous spherules, accrecionary lapilli, strange matter in
the form of iron silicides such as gupeiite, xifengite, hapkeite, and various carbides, e.g.,
moissanite and khamrabaevite, microtektites, and an impact-induced Lake Chiemsee tsunami.
In the beginning of the investigations the large number of about 80 mostly rimmed craters in
an elliptically shaped strewn field of about 60 km x 30 km size (Fig. 2) attracted the attention
of the discoverers who had thoroughly documented the craters even in the very beginning.
Meanwhile, for some of these craters another than an impact origin has been considered
probable (e.g., Ernstson and Neumair 2011), but at the same time many new objects were
discovered that show all evidence of belonging to the impact crater strewn field. In part, hints
for their existence came from the interested population, but a systematic search using the
Digital Terrain Model DTM provided a significant new impulse.
As for the target geology and rocks I mention the age of the impact event to have
happened in the Bronze Age/Celtic era when the impact-affected ground consisted of moraine
material and gravel plains. Beyond that I refer to the established literature (e.g., Ernstson et al.
3 Data processing
3.1 Terrain imagery
The herein discussed terrain imagery for the Chiemgau impact strewn field is in all cases
based on the German DTM (DGM1) with a 1 m mesh and an elevation resolution of 0.2 m
optionally in the UTM or the Gauß-Krüger coordinate system. Simple data processing enables
the reduction of the 1 m and the 0.2 m standards by interpolation.
The most familiar transfer of the DTM data produces topographic maps based on
arbitrary contour intervals. In Fig. 4 such a topographic map with a 10 cm contour interval is
shown for the 15 m-diameter Einsiedeleiche crater in the Chiemgau impact strewn field.
Taking into account that the conventional 1 : 25,000 topographic maps in general consider a 5
m (rarely 2.5 m or 1.25 m) elevation contour interval, the map in Fig. 4 covering only 3 m
height difference would trace no more than a single contour line, if at all, and nobody would
recognize the existence of that crater.
Fig. 4. Einsiedeleiche crater. DTM topographic map; contour interval 0.1 m. Here and in all
other cases to follow the crater diameter is assigned to the rim crest diameter (here: 15 m).
Elaborating a 3D surface from the digital data provides a more picturesque version of
terrain imagery, in particular for the visualization of rimmed craters, as is shown in Fig. 5 for
again the Einsiedeleiche crater. In suitable data processing programs arbitrary colors and
grading can be selected, and an elevation mesh may be superimposed or omitted.
Fig. 5. DTM 3D surface of the Einsiedeleiche crater.
Maps of shaded relief that can digitally be lightened from various directions and under
various angles of entry such highlighting arbitrary topographic features give a similar 3D
visualization of the terrain surface. The shaded relief map in Fig 6 shows the Einsiedeleiche
crater in its somewhat larger environments as a distinct anomaly but not as impressive as in
the 3D surface map in Fig. 5. The special importance of shaded relief maps is due to their
nature to enable a quick look at selected features also on larger terrains. Fig. 7 is an
instructive example from the Chiemgau impact strewn field. The area is insofar exceptional as
the remarkable cluster of craters initiated a geophysical campaign, and in a first step earth
magnetic field measurements revealed extensive magnetic anomalies of exceedingly high
amplitudes and rocks sampled from the ground that showed unusually high magnetizations
(Neumair and Ernstson 2011).
Fig. 6. DTM shaded relief map of the Einsiedeleiche crater.
Fig. 7. A DTM shaded relief map of a forest area suggests a cluster of rimmed craters with
diameters between a few meters and about 20 m probably belonging to the Chiemgau impact
strewn field. For three selected craters diametrical cross sections have been plotted, which is
in more detail discussed in paragraph 3.4.
3.2. Horizontal gradient
The computation of the horizontal gradient is a useful tool with data processing of the DTM.
For every point in the elevation grid the maximum slope with regard to the neighboring points
is determined as a figure (unit m/m), and all figures constitute a new map of the horizontal
gradient, in other words a map of the terrain slope. Because structures are now shown in
higher resolution, this procedure may be considered a kind of high-pass filter. In Fig. 8 the
Einsiedeleiche crater is used again to emphasize the multiple possibilities of the DTM by
presenting the horizontal gradient map. The smaller Einsiedeleiche 2 crater is interpreted as a
probable impact companion that in the thick forest was unknown previously.
Fig. 8. Horizontal gradient of the elevation data accentuates a smaller companion crater of the
Einsiedeleiche crater.
3.3 Data filtering
2D data filtering offers various possibilities to DTM processing starting from the concept that
the terrain is composed of the superposition of various elevation wavelengths. Low-pass
filters are enhancing topographic general trends while high-pass filters are accentuating
smaller, local topographic features. Filtering does not produce new field data but may
highlight particular terrain attributes for the eye.
Frequently, small-scale bumps may largely mask general terrain trends of interest, and
a simple low-pass filter may easily clarify the matter. A procedure borrowed from
geophysical potential fields (e.g., gravity and geomagnetic fields) can also be helpful with
DTM data processing for separating local anomalies from a general trend in a field of contour
lines. In gravimetry e.g., a regional trend field may be derived from the measured data by
various procedures, and subtracting the regional field from the measured field will result in
the local or residual field mostly being the main subject of interest.
The procedure may be copied for DTM data processing if one wants to separate local
topographic features from a general trend in the terrain elevation. An example for crater
evaluation in the Chiemgau strewn field is shown in Fig. 9. Top down we see the original
topography for the Leonberg #012 crater situated in a mountain slope. A trend field for the
terrain slope is computed from the original data by applying a strong low-pass moving-
average filter. The resulting trend field in Fig. 9 then visualizes the smoothed mountain slope
before - simply put - any event produced the distinct hole in the ground. Focusing on the
residual topography after removal of the trend there is no way of overlooking that the change
in the ground can be attributed to a roughly circular bowl-shaped structure surrounded by a
likewise distinct rim wall. Here the data evaluation need not end, and a subsequent low-pass
filter may yet beautify the crater topographic anomaly. At this point of having illuminated the
DTM terrain imagery and its fundamental properties it is largely irrelevant whether the
Leonberg crater was formed in the Chiemgau impact event. If it were however, a fragmented
closely spaced triplet impactor must be taken into consideration.
Fig. 9. Low-pass filters applied to the DTM of the Leonberg #012 crater. Explanation in the
text. Contour interval is in all cases 0.1 m.
3.4 Cross sections
The high resolution of the DTM elevation data can usefully be applied to plot crater profiles
providing not only very precise crater depths and diameters but also details of the geometry of
the crater bowl, the in most cases existing distinct rim wall and the crater periphery. In Fig.
10A this is illustrated by typical cross sections for a few craters in the Chiemgau impact
strewn field.
Fig. 10A. DTM diametrical cross sections for smaller craters in the Chiemgau meteorite
impact strewn field. Except for the Einsiedeleiche 2 and Emmerting Siedlung craters the
impact nature has been proven (shock metamorphism) or suggested (strong rock deformation,
melt rocks, geophysical anomalies). For all cross sections the same scale applies.
As discussed for DTM contour maps (Fig. 8) horizontal gradients may be computed and
plotted also for crater cross sections. This may be done either for profiles selected from the
gradient contour maps or by mathematical differentiation of an already extracted elevation
curve like those shown in Fig. 10A. The latter has been performed and is shown in Fig. 10B
for one of the diametrical #001 crater cross sections. As emphasized for the gradient contour
maps the profiles for the horizontal gradient distinguish by still higher resolution for
particular crater shapes.
Fig. 10B. DTM crater profile and horizontal gradient curve. Inflection points and weaker
amplitudes of the gradient curve point to details of the structure. Different from the gradient
contour maps the line gradient dY/dX has positive and negative sign.
Undoubtedly, the today's crater topography and cross section reflect details of the
formation process, which in particular holds true for very young structures. Likewise
undoubtedly, there is not any morphological feature that enables the unambiguous diagnosis
of the trigger mechanism. A bomb crater, a chemical explosion crater, a sand explosion crater
from strong rock liquefaction (see e.g., Ernstson and Neumair 2011), or a meteorite impact
crater, here of course in the foreground, may leave craters of the form shown in Fig. 10. The
most intriguing potential of studying precise crater profiles is
a) to see close similarities suggesting common genesis,
b) to see differences suggesting common genesis under different constraints, and
c) to see basic differences suggesting that a certain formation process can be excluded.
Before respective examples will later be discussed for selected craters, a simple case a) is
shown in Fig. 11. Diametrical cross sections for two craters roughly 2 km apart near the town
of Emmerting have been stacked to reveal practically identical matching even in very detail, if
a general small shift of only 50 cm is being neglected. Excluding a highly unlikely
coincidence the same origin is obvious and at the same time a man-made construct irrelevant.
Fig. 11. Comparison of diametrical cross sections for the #004 and Emmerting Siedlung
craters. Considering a slight shift of 0.5 m the crater profiles are practically congruent
differing no more than 20 cm.
4 Examples
4.1 Small craters in the DTM
The Kaltenbach crater
The Kaltenbach crater located roughly 2 km north of the Lake Tüttensee so far most
prominent crater in the strewn field (e.g., Ernstson et al 2010), is exemplary for a very small
crater of only 8 m diameter that even overgrown in a forest area can clearly be identified by
the DTM (Fig. 12, 13). It goes without saying that despite the nice rimmed crateriform shape
the meteorite impact nature has to be verified in the field. In fact a geophysical survey (Fig.
13) showed typical magnetic anomalies already known from other small craters in the strewn
field (Neumair and Ernstson 2011), and analyses of excavated rock samples proved a short-
term, high-temperature overprint of the ground when the crater was formed, basically
excluding an anthropogenic origin (Neumair and Ernstson 2011, Procházka and Kletetschka
Fig. 12. DTM shaded relief of the 8 m-diameter Kaltenbach crater in a forest area (see Fig. 5).
Crater diameter in all cases means rim crest diameter.
Fig. 13. The Kaltenbach crater in nature, overgrown by a tree and brushwood. Magnetometer
The Schatzgrube (#001) crater
The somewhat larger Schatzgrube crater (also named #001 crater) in the northern part of the
strewn field located also in a forest area is manifested by the DTM as a clear bowl-shaped
depression with a distinct circular wall (Fig. 14, 15). Melt rocks and strong deformation of the
target material and in particular diaplectic glass in a quartzite cobble as in proof of shock
metamorphism (Ernstson 2012) give impact evidence.
Fig. 14. DTM shaded relief and 3D surface of the 14 m-diameter Schatzgrube crater in a
forest area.
The result of an earlier performed optical leveling on a diametrical profile provided an
instructive comparison with the DTM data. As is shown in Fig. 15b the differences are
minimal nowhere exceeding a few decimeters along the 40 m long profile, although the
leveling yardstick had to be placed on the relatively soft forest floor.
Changing from the DTM two-dimensional topographic map in Fig. 15a to diametrical
cross sections marked in that figure, a remarkable result is obtained for the crater structure
ultimately due to the high DTM resolving power. In Fig. 15c the cross sections for the four
profiles have been plotted from the DTM data, and by also plotting horizontally mirrored
copies a stacking of in total eight radial cross sections could be performed. From Fig. 15c the
amazingly nearly congruent shape along all eight radial profiles is evident. In the crater
interior and along most part of the rim wall the height differences don't exceed 20 - 30
centimeters, and only outside the rim wall they reach a few decimeters more. Perhaps more
impressively the horizontal gradient curves in Fig. 15 d show that even minor topographic
features can be traced around the inner crater wall.
It is concluded that this 3D exact circularity with a diameter of nearly 20 m could have
formed only by a more or less punctuate impact or/and explosion event. Particularly and
reasonably it considers every man-made activities practically impossible.
Fig. 15. The Schatzgrube crater. a: DTM, contour interval 0.2 m. b: DTM cross section along
a north - south profile compared with ground optical leveling with 1 m spacing. c: DTM cross
sections for four diametrical profiles (see a) which have additionally been mirrored to show
the stacking of eight radial cross sections. d: Horizontal gradient profiles for the cross sections
in c (compare Fig. 10B). Please note that even minor elevation features along the eight radial
profiles can be traced around the crater (arrows).
The crater is of particular importance because of its nearly identical size and shape
when compared with the recently (2007) formed Carancas meteorite crater in Peru (e.g.,
Tancredi et al. 2009, Kenkmann et al. 2008, 2009) (Fig. 16). The Carancas crater featured
something totally unexpected because according to the till then established “laws of impact”
such a crater created by a hypervelocity impact of an estimated 0.5-1 m stony meteorite
seemed completely impossible (as claimed by e.g., Reimold 2006, 2007). And consequently
Schultz et al. (2008) in their LPSC abstract article on the Carancas impact are beginning their
text with the nice statement: “The Carancas impact crater (just before noon on September 15,
2007) should not have happened.” We need not especially emphasize that this statement
concerns the arguments earlier formulated with unshakeable conviction that the Chiemgau
impact with lots of small craters (among them the Schatzgrube crater) cannot exist (e.g.,
Reimold 2006, 2007, Wünnemann et al. 2007).
Fig. 16. Cross section of the Schatzgrube crater in comparison with the nearly identical cross
section of the Carancas meteorite crater. Carancas section and data redrawn from Kenkmann
et al. 2009).
4.2 Peripheral depressions around small craters
The enormous resolution of the DTM points to a possibly impact-specific peculiarity. As is
marked in Fig. 17, the in each case clearly visible rim wall for four smaller craters is
surrounded by a roughly concentric ring depression a few decimeters deep only, giving the
structures a total size of more than 30 m. Similar ring-like depressions are found also for
several other small craters, but because of general rough terrain conditions they often lack the
exemplary geometry seen in Fig. 17.
In the meteorite impact terminology one would speak of a peak-ring crater as a typical
exponent of large complex impact structures, and the formation is largely understood to be the
result of transient crater collapse and elastic rebound (e.g., Melosh 1989). This cratering
process is of course a long way from being a model for the small craters under discussion here
although at least the #004 and Schatzgrube #001 structures because of strong shock
metamorphism are established meteorite craters. Although for the time being a reasonable
explanation is lacking, the mere existence of this peculiar crater structure highlights once
more the enormous potential of the DTM terrain evaluation.
Fig. 17. Peripheral depressions around small crater seen in contour maps and on diametrical
cross sections.
4.3 Medium-sized craters in the DTM
The Purkering crater
The Purkering 75 m-diameter crater (photo in Fig. 19) is a paragon and owes its first impact
recognition when T. Marx (pers. comm.) saw the structure rather accidentally during his
studies of the freely in the web available DTM shaded relief map (Fig. 18, left) in the east of
the town of Trostberg. Later a complete digital data set (DGM 1) was acquired for a more
detailed data processing (Figs. 17, to the right; 20, 21 and 22).
Meanwhile, the impact nature is substantiated not only by the circular wall hardly
compatible with another origin but also by geophysical measurements (ground penetrating
radar GPR, geomagnetics) only recently performed, and by a curtain of ejected gravelly
material (Fig. 22).
Fig. 18. DTM: shaded relief (to the left) and 3D surface of the 75 m-diameter Purkering
Fig. 19. In the field: the 75 m-diameter Purkering crater with a slight rampart. The Alpine
foothills in the background.
Fig. 20. DTM contour map of the Purkering crater. Contour interval 20 cm.
Fig. 21. Cross section of the Purkering crater from DTM data.
Fig. 22. Purkering crater: Horizontal gradient map from DTM data indicating a smaller
companion structure at the southeastern rim.
Fig. 23. The Purkering crater and its curtain of impact-ejected gravelly material. Google Earth
The enormous possibilities of the DTM data processing become evident when the map
of the computed horizontal gradient for the Purkering crater is taken as an example (Fig. 22).
More than all others DTM images the gradient on the one hand outlines the absolute
circularity of the main depression and, on the other hand, points to an additional
morphological anomaly at the southeastern rim that may have resulted from the synchronous
impact of a smaller separate companion projectile. This impressively fits the distinctly
asymmetric distribution of the ejected gravelly material (Fig. 23).
The Hochfelln crater
So far, the Hochfelln crater (Fig. 24 - 26) has been recognized by non-geologists' hiking tours
only and needs verification by geologic and geophysical field work. It is the first established
probable meteorite crater with a characteristic rim wall in the Alpine foothills (see Fig. 10),
after a Chiemgau impact overprint of the mountainous region had long before been predicted.
This is based on an in part very peculiar landscape, unusually widely scattered fractured rocks
and the occurrence of microtektites in the upper soil layers chemically reflecting the local
rocks (Ruhpolding Fm.) (Ernstson et al. 2014).
Fig. 24. The Hochfelln 55 m-diameter crater. DTM contour map; counter interval 0.2 m. Red:
cross section profiles in Fig. 25.
Fig. 25. Cross sections of the Hochfelln crater from DTM data. Profiles in Fig. 24.
Fig. 26. DTM 3D surface of the Hochfelln crater revealing a distinct crater wall obviously
merging into a curtain of flow structures downhill, which in the case of an impact crater may
be attributed to ejecta.
As mentioned before, the crater needs verification by geologic field work, which will have to
focus also on the peculiar morphological signature crater downhill (Fig. 26), which in highest
DTM 3D surface resolution may trace excavated and ejected target rock material.
Likewise eye-catching in the DTM 3D surface map of the crater environment (Fig.
27), one big landslide and a few smaller suspected ones may be considered a possible result of
nearby impact cratering and related seismic shattering in the Chiemgau impact event.
Fig. 27 Landslides possibly impact-induced in the Chiemgau event. DTM 3D surface.
The doublet (? triplet) Punzenpoint crater
One more impressive example for the efficiency of the DTM data processing is given by the
Punzenpoint structure (Fig. 28), which has only recently been discovered some kilometers to
the northwest of the town of Obing and still lacks a geologic-geophysical verification. In the
official topographic map, 1 : 25,000 scale (Fig. 29), one cannot even guess the existence of
such a special feature. There are strong points for an impact crater given by the distinct
circularity of both the depression and the obvious wall belonging to it, which excludes any
sinkhole formation, also by virtue of its size alone. The distinct bulge in the southeastern rim
wall is without doubt related with the neighboring 50 m-diameter rimmed depression, and a
synchronous formation of both structures to feature a possible impact doublet crater seems
obvious. Moreover, a third depression may possibly contribute to a triplet crater with
overlapping rim wall crests (Fig. 28).
Fig. 28. DTM 3D surface of the 120 m-diameter Punzenpoint main crater, an about 50 m-
diameter companion crater and a possible third 20 m-diameter crater. The dotted lines are
delineating the particular rim crests.
Fig. 29. The Location of the Punzenpoint crater on the official topographic map
1 : 25,000. Source TOP10.
The Aiching semi crater
The Aiching crater near the town of Marktl, marked number #024 in the original list of the
discoverers, is not easily recognized in the field (Fig. 30) and not at all on the official
topographic map. The early discoverers became aware of it by making a photo from a plane in
wintertime when the trees were free of leaves. The meteorite impact nature of this semi crater
was substantiated by abundant finds of the strange iron silicide matter (Ernstson et al. 2010)
in the field adjacent to the semi crater.
Fig. 30. The Aiching semi crater (arrow) located in the steep bank of the Inn River near the
town of Marktl. Dense tree growth and a big stable right in the middle of the crater are largely
masking its impressive shape that becomes evident in the DTM data (Fig. 31 -34).
Fig. 31. Aiching semi crater in the DTM; 1 m grid and 0.5 m contour interval. The crater was
punched in the steep valley border and today is conserved at half only because of the
destruction by the nearby Inn River erosion. The white line traces the cross section of the
crater in Fig. 32.
Today, with the aid of the high resolution of the pure DTM digital topographic data
(Fig. 31, 33) details of this remarkable crater have become evident. For the first time, precise
depth and diameter data were attained, and a (semi) circular rim wall of no more than 1 m
height (Fig. 32, 34) could be established. In the very beginning a seemingly lacking rim wall
had been attributed to a radical leveling by the farmers.
Fig. 32. Cross section of the semi crater along the white line in Fig. 22. From the eccentric
course of profile the rim crest distance brings about a crater diameter of at least 56 m and a
depth of more than 7 m.
Fig. 33. The map of the horizontal gradient computed from the DTM data in particular
highlights the crater to be a foreign body in the Inn River landscape.
Fig. 34. The Aiching semi crater in a DTM 3D meshed surface image. It accentuates a
rimmed crater as a discrete, originally circular object that stands out against the scarp of the
4.4 Mistaken structures
So far, the DTM data processing has been used to evaluate known craters in the Chiemgau
strewn field and to look for promising new structures. On the other hand, the potential of the
DTM should not be underestimated to bring doubtful candidates into question or to even
eliminate them. An interesting example is shown in Fig. 35 focusing on two distinctly circular
structures of some 30 - 50 m diameter that about 15 years ago in the early phase of the
Chiemgau impact research were discovered in satellite imagery and considered probable
impact points, and they got the numbers #52 and #53 in the original crater list.
Fig. 35. Suspected craters from satellite imagery (to the right) lack any indication on the
ground (DTM shaded relief, to the left).
Today, with the aid of the high-resolution DTM (Fig. 35, to the left), both suspected sites
amazingly are completely unidentifiable in the shaded relief map. Hence, Nos. #52 and #53
lack any indication on the ground, and the original circular ground features remain enigmatic.
The case shown in Fig. 36 is different. Near the Lake Tüttensee crater a group of three
or four bowl-shaped depressions in the ground have been considered possible candidates for
the Chiemgau meteorite crater strewn field, and different from Fig. 35 the holes are reality.
Selected DTM sections, in each case forming a cross over the depressions, don't however
speak in favor of such an origin. This corresponds with the result of a geomagnetic survey
revealing not any noteworthy anomalies otherwise regularly found with the typical proven or
suspected impact craters. The origin of the holes is obscure, but because of their location very
near to the 600 m-diameter Tüttensee crater a formation in the course of strong impact rock
liquefaction leading to local sand explosions (see Ernstson et al. 2011) could be a reasonable
Fig. 36. DTM 3D surface map and cross sections of three roundish depressions near the Lake
Tüttensee crater: Probably no impact craters but possibly rock liquefaction sand explosion
5 A possible large-sized crater in the DTM
The Eglsee structure
It is said that some astronomers after having visited the Chiemgau impact crater strewn field
pointed to a suspicious near-circular structure with a diameter of about 1 km located not far
from Lake Chiemsee, which they had studied from satellite imagery. The in fact casual hint to
a possible further crater in the strewn field swiftly fell into oblivion until the DTM high-
resolution maps and data processing enabled a closer view and study of that structure. First
fieldwork revealed abundant finds of deformed rocks well known from e.g., the Tüttensee
meteorite crater. Also the extremely steep flanks of the impressive rim wall encircling a
peculiar large circular depression attracted our attention and caused serious problems to relate
them to a glacial moraine deposition more than 10,000 years ago. In fact this Eglsee structure
so far had simply been incorporated in the ridge of terminal moraines around Lake Chiemsee
attributed to the Inn-Chiemsee glacier (Darga 2009, Doppler et al. 2011) without giving it
further particular consideration.
From the high-resolution DTM contour map in Fig. 37 a terminal-moraine origin for
the Eglsee structure would make no sense with regard to the three-quarter nearly perfect rim
circle and the contouring of the rim wall with a few sharp offsets. Hence, the original idea of
the astronomers about a meteorite impact structure revived the discussion and initiated
geophysical gravimetry and ground penetration radar (GPR) surveys currently under data
Tentatively, the idea of a meteorite crater is also illuminated by contrasting it with the
famous, nearly equally sized Barringer (or Meteor) crater in Arizona (Fig. 38, 39). In
particular the amazingly similar cross section of both rim walls is striking (Fig. 39), although
the markedly different depth has to be considered. The latter may possibly the result of the
basically different target rocks, which are solid rock in the case of the Barringer crater and
unconsolidated soft rock in the case of the Eglsee structure.
Meanwhile a competing formation of the Eglsee structure has been considered
possible with regard to impressive tsunami deposits (Ernstson 2016) that have been shown to
be related with the earlier established impact and impact doublet crater at the bottom of Lake
Chiemsee only 2.5 km apart (Ernstson et al. 2010). This powerful tsunami could possibly
have piled up the Eglsee structure rim wall, but at the same time it does not exclude a
meteorite crater that immediately was formed before the tsunami that carried huge masses of
rock material arrived. Such a coupled event may perhaps explain both the rim wall gap in the
direction of Lake Chiemsee (see Fig. 37) and the less deep Eglsee crater compared with the
Barringer crater. In particular the results of the geophysical measurements are expected to
clarify the true formation of this peculiar topographic anomaly.
Fig. 37. The Eglsee structure from DTM data. Contour interval 1 m.
Abb. 38. DTM 3D surface of the Eglsee structure and photo (NASA) of the equally sized
Barringer crater.
Abb. 39. Cross sections of the Barringer crater and the Eglsee structure. Same scale of length,
but note the different height scales. Barringer profile redrawn from LPI.
6 Discussion and conclusions
Astonishingly enough the use of digital LiDAR data in the form of the Digital Terrain Model
DTM has in the past only very hesitantly if at all found its way into the world of geologists,
engineers and geophysicists, which at least holds true for Germany (here the corresponding
Digitales Geländemodell DGM), although one can enormously profit from the various
possibilities the data processing is offering for many purposes. This article deals with the
applicability and efficiency of the DTM for a special field of research, the exploration of
meteorite craters and related phenomena. Established craters as well as presumptive craters in
the area of the Chiemgau impact served as test objects to show how impact research may
recognize interesting morphological details adding to mineralogical-petrographic,
geochemical, geologic and geophysical insight. The basic advantage of the DTM is that it sees
and measures the "naked" crater morphology with an unbelievably high precision and
resolution with mesh sizes, if desired, down to 1 m and contour resolution down to 20 cm.
This holds true at least for the DGM 1 in Germany (Bavaria). The significance of the DTM
meets well the very young age of roughly 2,500 - 3,000 B.P. of the craters, which means that
the structures have comparably well been preserved. But also some later overprints of e.g.,
agriculture and young erosion did not blur characteristic features like crater rim walls which is
exemplarily shown for the Aiching semi crater.
Morphological similarities or dissimilarities, for example depth-diameter ratios, which
are much more precise to be evaluated by the DTM, asymmetric ejecta distribution, prior
unseen details of the crater structures (e.g., the ring-like depressions around several craters),
are typical subjects making the DTM an essential tool. A particular merit of the DTM data
processing can be attributed to the recognition of multiple, doublet or even triplet, structures.
If they were produced by meteorite impact they could point to a fragmented projectile and
collective impact. These morphological peculiarities shown for the Punzenpoint and
Purkering sites but unsupported by any field evidence or topographic maps, benefit solely
from the DTM. Even processes like the Hochfelln landslides may make an alternate
explanation of their formation available to geologists if a possible connection with an impact
can be revealed by studying the processed DTM high-resolution maps.
When the unmissable merit of the DTM processing for the study of impact craters is
pointed out here it is likewise emphasized that it also facilitates to debunk or to query at least
previously suspected meteorite craters as could be shown for the Chiemgau strewn field. On
the other hand, it cannot be repeated often enough that in impact research the morphology of a
structure alone is not sufficient criterion for establishing a meteorite impact crater. Generally
accepted criteria are, apart from the direct observation of the impact (Carancas!) and remnants
of the projectile (macroscopic or geochemically measurable) diverse shock-metamorphic
This sheds some light on a strange notice. Early and a few remaining critics and
deniers of the Chiemgau impact event (Reimold 2006, 2007a,b, Wünnemann et al. 2007,
Koeberl 2008, Doppler and Geiss 2005, Reimold & Koeberl 2014, Reimold et al. 2014,
Doppler et al. 2011, Schmieder et al. 2011) have apart from ignoring all impact evidence like
shock metamorphism, impact melt rocks, impact ejecta, geophysical anomalies, and more,
always claimed the ice age, glacial processes and the glacial landscape, as well as
anthropogenic activities as unmistakably being behind all proposed impact features. In their
paper on "Impact structures in Africa: A review" Reimold and Koeberl (2014) are renewing
their attack against the Chiemgau impact research and claim that when discussing possible
new impact craters also the regional-geologic setting has to be taken into consideration. At
that they in particular accentuate a glacial overprint obviously aiming at the Chiemgau impact
strewn field that in their opinion is a cluster of glacially produced “holes”. In doing so they do
not at all realize that they are questioning their own and always propagated postulate – shock
as prerequisite for the acceptance of impact – and putting the case for all those regional
geologists who deny the existence of impact structures because these are incompatible with
the regional-geologic setting. Reimold and Koeberl are encouraged to take a look at the
"cluster of glacially produced holes" in the Digital Terrain Model DTM from which they may
possibly learn a lot for their own impact research.
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The location map for the sites discussed in this article: 1 = Kaltenbach, 2 = Schatzgrube, 3 =
Purkering, 4 = Hochfelln, 5 = Punzenpoint, 6 = Aiching, 7 = Leonberg, 8 = Einsiedeleiche, 9
= #004, 10 = Emmerting Siedlung, 11 = #002, 12 = Laubergraben, 13 = Mauerkirchen, 14 =
Burgstall, 15 = Tyrlaching, 16 = Thalham, 17 = Eglsee.
ResearchGate has not been able to resolve any citations for this publication.
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Introduction: The Holocene Chiemgau impact event is considered to have produced a large meteorite crater strewn field in southeast Germany in the Bronze Age/Celtic era ([1], and ref. therein). The impact is documented by impact melt rocks and various glasses, strong shock metamorphism, geophysical anomalies and ejecta deposits, and substantiated by the abundant occurrence of metallic, glass and carbon spherules. Enigmatic carbon matter containing carbynes and diamond-like/carbyne-like carbon allotropes also testify extreme temperatures and pressures [2, 3]. From the beginning of the discovery and investigation of the strewn field, extended finds of iron silicide particles in the subsoil mainly composed of xifengite and gupeiite and obviously associated with the craters played a significant role as possible meteoritic matter. New analytical SEM, TEM and EBSD have shown that the iron silicides when going down to micrometer scales are hosting a real «zoo» of more than 30 chemical elements, extremely rare minerals and peculiar textural features. Observations: Iron silicides (Fig. 1, A). — So far the minerals xifengite, gupeiite, fersilicite, ferdisilicite and hapkeite have been established to occur as a matrix of intimate intergrowth. Different from the cubic hapkeite found for the first time in the Dhofar 280 lunar meteorite [4], the Chiemgau hapkeite could be shown to be the trigonal polymorph. Carbides (Fig. 1, A). — The iron silicide matrix contains abundant extremely pure crystals of SiC, cubic moissanite, TiC, and (Ti, V, Fe) C, khamrabaevite. Calcium-aluminum inclusions, CAIs (Fig. 1, B). — The Chiemgau iron silicides contain the monoclinic high-temperature (>1.500 °C), low-pressure dimorph of CaAl 2 O 4 , mineral krotite, and the orthorhombic Ca 2 Al 2 O 5 dicalcium dialuminate high pressure phase with the brownmillerite-type structure. Zirconium and uranium (Fig. 1, C, D). — Zirconium (zircon or/and baddeleyite) shows as possible exsolution lamellae in iron silicide. Clusters of tiny (< 10 m) zircon crystals coated by uranium are interspersing the iron silicide matrix. EDX spectra show the uranium to be free of any decay products Fig. 1. A: Titanium carbide (dark gray) and silicon carbide (moissanite, black) crystals in a matrix of intergrowth of various iron silicides. B: Light edging CAIs (arrow) around black C (graphite, diamond?) film in iron silicide matrix. C: Zircon crystals in iron silicide matrix. The white tips on the crystals have been shown to be uranium. D: Zirconium (zircon or/and baddeleyite) possible exsolution lamellae in iron silicide. E: Rimmed micro-craters on the surface of an iron silicide particle. F: Strongly fractured titanium carbide crystal in iron silicide matrix. Note the open, tensile fractures pointing to dynamic (shock?) spallation
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A microtektite deposit in Alpine foreland soils reveals an unusual glass composition and suggests an origin from local rocks in a nearby Holocene impact event.
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More than 50 years of space and planetary exploration and concomitant studies of terrestrial impact structures have demonstrated that impact cratering has been a fundamental process – an essential part of planetary evolution – ever since the beginning of accretion and has played a major role in planetary evolution throughout the solar system and beyond. This not only pertains to the development of the planets but to evolution of life as well. The terrestrial impact record represents only a small fraction of the bombardment history that Earth experienced throughout its evolution. While remote sensing investigations of planetary surfaces provide essential information about surface evolution and surface processes, they do not provide the information required for understanding the ultra-high strain rate, high-pressure, and high-temperature impact process. Thus, hands-on investigations of rocks from terrestrial impact craters, shock experimentation for pressure and temperature calibration of impact-related deformation of rocks and minerals, as well as parameter studies pertaining to the physics and chemistry of cratering and ejecta formation and emplacement, and laboratory studies of impact-generated lithologies are mandatory tools. These, together with numerical modeling analysis of impact physics, form the backbone of impact cratering studies. Here, we review the current status of knowledge about impact cratering – and provide a detailed account of the African impact record, which has been expanded vastly since a first overview was published in 1994. No less than 19 confirmed impact structures, and one shatter cone occurrence without related impact crater are now known from Africa. In addition, a number of impact glass, tektite and spherule layer occurrences are known. The 49 sites with proposed, but not yet confirmed, possible impact structures contain at least a considerable number of structures that, from available information, hold the promise to be able to expand the African impact record drastically – provided the political conditions for safe ground-truthing will become available. The fact that 28 structures have also been shown to date NOT to be of impact origin further underpins the strong interest in impact in Africa. We hope that this review stimulates the education of students about impact cratering and the fundamental importance of this process for Earth – both for its biological and geological evolution. This work may provide a reference volume for those workers who would like to search for impact craters and their ejecta in Africa.
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Arguing from a critical reading of the text, and scientific evidence on the ground, the authors show that the myth of Phaethon – the delinquent celestial charioteer – remembers the impact of a massive meteorite that hit the Chiemgau region in Bavaria between 2000 and 428 BC.
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The 600 m-diameter Lake Tüttensee structure is so far considered the largest meteorite crater in the strewn field of the Holocene Chiemgau impact, although there is strong evidence of a 900 m x 400 m rimmed doublet crater at the bottom of Lake Chiemsee. Shape and depth of the water body of Lake Tüttensee have been controversially disputed, which is probably related with the deposit of a layer of thick consolidated organic material. A gravity survey on the frozen lake and in its surroundings had the principal aim to get knowledge of the crater shape. The maximum gravity anomaly of Lake Tüttensee is about -0,8 milligals mainly resulting from the density contrast of water/organic material and rock. Modeling of the gravity anomaly with respect to the water (plus organic material) body, however, reveals unsatisfactory results related with a complex density distribution in the target rocks. Gravity also shows that the true crater is smaller than the lake extent. Surprisingly, a ring of relatively positive anomalies is measured surrounding the Tüttensee negative anomaly. The positive anomalies are modeled by a 1000 m-diameter flat lens of slightly enhanced density. It is explained by a model of soil liquefaction and post-liquefaction densification well known from large earthquakes. Moreover, mass flow behind the impact shock front could have contributed to the compaction of the unconsolidated, highly porous and water-saturated target rocks. In addition to impact melt rocks, shock metamorphism (PDFs), high pressure/short term deformations in rocks from the Tüttensee ring wall, and a catastrophic impact ejecta layer, the geophysical measurements provide a further argument against the hitherto favored origin of Lake Tüttensee from glacial dead-ice melting. Further studies of impact shock liquefaction may be interesting for the understanding of impact cratering in targets composed of loose and extremely water-rich rocks as has been discussed for near-surface sediments on Mars.
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Carbynes and DLC in naturally occurring carbon matter from the Alpine Foreland, South-East Germany: Evidence of a probable new impactite S. Isaenko (1), T. Shumilova (1), K. Ernstson (2), S. Shevchuk (1), A. Neumair (3), and M. Rappenglück (3) (1) Institute of Geology Komi SC UB RAS, Syktyvkar, Russian Federation (, (2) Faculty of Philosophy, University of Würzburg, Würzburg, Germany (, (3) Institute for Interdisciplinary Studies, Gilching, Germany ( Unusual carbonaceous matter (UCM) in the form of mostly centimeter-sized lumps and cobbles has been sampled in the southeast Bavarian Alpine Foreland. It is a highly porous blackish material with a glassy luster on freshly crushed surfaces. In some cases aerodynamically shaped cobbles like volcanic bombs were sampled. The material is unknown from any industrial or other anthropogenic processes and thus appears to have a natural origin, which is underlined by findings on a small island in the large Lake Chiemsee and at some altitude in the pre-Alps mountains. Here we report a detailed analysis of this strange matter by a complex of high resolu-tion Raman spectroscopy, X-Ray diffraction, electron scanning and atomic force microscopy, transmission electron microscopy and differential thermal analysis. We have found that the carbon matter is presented by the association of different carbon phases. The matrix is consisting of fully amorphous black glass-like carbon with a porous struc-ture and almost pure carbon content with traces of O, S, Si, Al. Inside of the matter monocrystal-line carbyne and amorphous diamond-like carbon (DLC) inclusions are found. The first is pre-sented by flattened particles of a-carbyne (predominantly) and in a single case by cooriented in-tergrowths of a- and b-carbyne modifications (Shumilova et al., 2012). The DLC is characterized by optically transparent particles of generally flattened irregular shape and rare bulk particles sometimes of trigonal form and octahedrons. The typical DLC Raman spectrum is decomposed into three general wide bands – around 1400-1500, 1325-1370 and 1580-1600 cm-1 and two bands at down-shoulder side – around 1070-1090 and 1200-1250 cm-1. Among known carbon substances there are no exactly equal spectra. However, the listed Raman features could be interpreted as sp2-3 glass-like carbon containing some quantity of DLC, while the wide bands 1325-1370 and 1580-1600 cm-1 are rather expected to correspond to D and G Raman bands of carbon materials. The other features should be attributed to the presence of amorphous carbon with high content of tetrahedral carbon bonds (Ferrari & Robertson, 2004; Wei & Sankar, 2000; Robertson, 2002; Osswald et al., 2009). Following Xu-Li et al. (2009), the analyzed optically transparent amorphous inclusions are pre-sented by DLC formed under high temperature. The observed carbon phases association and carbon state diagram are pointing to a process of very high pressures and temperatures to produce the UCM. We suggest the material to be a new impactite that was probably formed in the shock event of the proposed Chiemgau impact (Ernstson et al., 2010) with the formation of a large crater strewn field only a few thousand years ago.
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Peculiar finds have been attributed to a possible Holocene meteorite impact. They show absolutely identical parallels to impact features from the Chiemgau impact. If the sites can be dated synchronous a 500 km sized impact event might be targeted.