Eleonora Ammannito’s research while affiliated with ASI Science Data Centre and other places

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Publications (39)


The quest for habitats in the outer Solar System and how to protect exotic pristine environments
  • Article

April 2025

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28 Reads

Acta Astronautica

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Maxim Zaitsev

(a) Satellite view of the Gobi Valley in Mongolia, showing the vast tectonic depression located between the Hangay and Gobi Altai mountain ranges. (b) Detail of the Gobi Valley with specification of the areas of interest (ROI). ROI1 and ROI2 are located near Lake Orog, while ROI3 is located near Lake Böön Tsagaan. “ROI 1: 45°0.424′N 100°44.235′E”, “ROI 2: 45°2.668′N 100°45.967′E” and “ROI 3: 45°26.781′N 99°59.717′E”, (QGIS source).
(a) Geologic units of Mongolia. Data: USGS geological survey [19]. The white box indicates the area containing the three ROIs. (b) Location of the three analyzed ROIs. The three areas of interest are situated within the Quaternary basalt fields (Q) of the blue unit, which form gently undulating surfaces.
Caption for the extracted geological map of the Dalinouer delta area, originally published at a scale of 1:1,500,000 by the Geological Publishing House. N1 l = Formation Laoliangdi Fm Greyish yellow, dark grey clastics (Mesozoic-Cenozoic); E1 + 2 = Sedimentary Rock (Tertiary-Palaeogene).
Left: RGB (red = 645.9 nm, green = 550.9, blue = 475.3 nm) visualization of the PRISMA acquisition over the Gobi Lake area studied here. Right: Map of the mineral distribution on the same area, using PRISMA hyperspectral data: Cyan is for quartz (the full spectral range), blue for chlorite (absorptions at 2.25 and 2.33 μm), yellow for albite (all the spectral range), green for montmorillonite, and red for illite (these latter at 2.19 and 2.20 μm, distinguished by the absorption width). PRISMA Product—©ASI—Agenzia Spaziale Italiana—(2020). All rights reserved.
Left: RGB (red = 645.9 nm, green = 550.9, blue = 475.3 nm) visualization of the PRISMA acquisition over the Dalinouer area studied here. Right: Map of the mineral distribution on the same area, using PRISMA hyperspectral data: Red is for illite/montmorillonite (absorptions at 2.20 μm), blue for femic minerals (olivine/pyroxenes) (absorptions at 1 μm), and magenta for a combination of them. PRISMA Product—©ASI—Agenzia Spaziale Italiana—(2023). All rights reserved.

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Terrestrial and Martian Paleo-Hydrologic Environment Systematic Comparison with ASI PRISMA and NASA CRISM Hyperspectral Instruments
  • Article
  • Full-text available

February 2025

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36 Reads

The comparative analysis of hyperspectral data from different instruments can provide detailed information on the composition and geology of similar environments on different planets. This study aims to compare data acquired from the PRISMA satellite, used for Earth observation, with those collected by the CRISM spectrometer onboard the Mars Reconnaissance Orbiter, orbiting Mars, in order to analyze the geological and mineralogical differences between the morphologies present on the two planets of interest. The comparison of these data will allow us to examine the mineralogical composition, highlighting the similarities and differences between the terrestrial and Martian environments. In particular, in this study, we present a method to refine the interpretation of spectral features of minerals commonly found in paleo-hydrological environments on Mars and identified also by field analysis of similar terrestrial sites, thus allowing us to improve the Martian sites’ characterization. Thanks to this approach, we have been able to find spectral similarities (e.g., band positions, band ratios) among specific Earth and Mars sites, thus demonstrating that it could be further expanded, by systematically using Earth-observation orbiting instruments to better characterize and constrain Martian spectral data.

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A focus on Chemical Equilibria of Saline Aqueous Solutions Freezing under Ceres’ Surface

October 2024

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12 Reads

Earth and Planetary Science

On Ceres’ surface, the region including Kupalo and Juling was selected, in this study, for the geological aspects characterizing the area. Spectral data revealed that, at surface, the two craters show the presence of different carbonates: Na-carbonates (Kupalo) and Ca-Mg-carbonates (Juling). We think that the distinct geology at surface may be the result of the freezing of different subsurface aqueous reservoirs, characterized by different compositions and initial P-T conditions. The first step was to characterize the initial composition of aqueous solutions which, after freezing/precipitation processes, by using FREZCHEM code, delivered salts which can better approximate the surface compositions found by spectral analysis. Our potential brines were alkaline aqueous solutions, and they differ for the Na- and Cl- amounts (higher at Kupalo, rather than Juling solutions). The formation of hydrated sodium carbonate (natron, Na2CO3·10H2O) is highly favored in Na-enriched solution (e.g., Kupalo); instead, it could form only after water ice precipitation in Na-depleted solutions (e.g., in Juling). Natrite (Na2CO3) was found in Kupalo’s surface layers, and, in our simulations, it did not directly precipitate from the solutions. We suggest that it could have been formed from natron and nahcolite (Na2CO3·10H2O and NaHCO3 respectively) at 1 bar of total pressure. Furthermore, we discussed the stability of the carbonates formed including MgCO3 (magnesite) and CaMg(CO3)2 (dolomite). Finally, we investigated on the transport dynamics of brines suggesting that, already in the subsurface, there could be the physical processes to bring solid material (precipitated from the solutions) to the surface.



Preliminary spectroscopic investigation of a potential Mars analog site: Lake Bagno dell’Acqua, Pantelleria, Italy

April 2024

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92 Reads

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5 Citations

Planetary and Space Science

The sediments in Lake Bagno dell’Acqua in Pantelleria (Italy) are characterized by a co-occurence of Mg-smectites and carbonates associated with a rich microbic community (i.e., Firmicutes, Chloroflexi, Proteobacteria and others). Presence of carbonates together with smectites is also observed on Mars and therefore the Lake Bagno dell’Acqua can be useful as a Mars analog site. The presence of a rich microbial communities and related organic products allows to study the interactions between microbes and sediments.


HYPERSPECTRAL ANALYSIS OF TERRESTRIAL PLANETARY-ANALOG SITES: PRELIMINARY RESULTS FROM ANCIENT FLUVIAL ENVIRONMENTS IN THE GOBI AREA

February 2024

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6 Reads

This investigation aims to improve our under-standing and characterization of Martian sites by examining spectral features in contexts involving water. By doing so, we leverage similarities be-tween the two planets to better interpret data col-lected on Mars, providing a more comprehensive and detailed picture of the geological and miner-alogical conditions on the Martian surface.



Fig. 3 Dotted lines= USGS library spectra; Solid lines=ratioed PRISMA spectra.
EXPLOITING PRISMA HYPESPECTRAL DATA TO SUPPORT CRISM MEASUREMENTS ON PALEO-HYDROLOGICAL ENVIRONMENTS ON MARS

January 2024

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5 Reads

The comparative analysis of hyperspectral data from different instruments can provide detailed information on the composition and geology of similar environments on different planets. This study aims to compare data acquired from the PRISMA satellite (Caporusso et al., 2020), used for Earth observation, with those collected by the CRISM spectrometer onboard the Mars Reconnaissance Orbiter, orbiting Mars, in order to analyze the geological and mineralogical differences between the morphologies present on the two planets of interest. The comparison of these data will allow us to examine the mineralogical composition, highlighting the similarities and differences between the terrestrial and Martian environments. In particular, in this study, we present a method to refine the interpretation of spectral features of minerals commonly found in paleo-hydrological environments on Mars and identified also by field analysis of similar terrestrial sites, thus allowing us to improve the Martian sites characterization.




Citations (12)


... We carried out this survey in context with the development of the Ma_MISS instrument (e.g., De De Angelis et al., 2022;Altieri et al., 2023). Whilst we are collecting further information on the infrared signatures of extensive clay-bearing outcrops found in several key regions on Mars (see Table 3), some lab measurements are being conducted to enable more comparative analyses, notably on Martian meteorites (e.g., De Angelis et al., 2023) and samples collected in analogous sites (e.g., Ferrari et al., 2023a;Ferrari et al., 2023b;Bruschini et al., 2024). Putting together these complementary studies will indubitably enhance our understanding of aqueous weathering on Mars and constrain the environmental processes taking place on the planet through its history, which are of great relevance for planetary evolution and astrobiology. ...

Reference:

Clay mineralogy in west Chryse Planitia, Mars: Comparison with present and future landing sites
Preliminary spectroscopic investigation of a potential Mars analog site: Lake Bagno dell’Acqua, Pantelleria, Italy

Planetary and Space Science

... Beyond Earth, the colonization of habitable, but uninhabited envir onments potentiall y has ethical implications, including those impinging on planetary protection protocols that militate against 'harmful' contamination of extraterrestrial environments (Coustenis et al. 2023 ). Planetary protection has been largely focused on protecting the scientific potential of extr aterr estrial environments (including deleterious impacts of contamination on the search for life), but in recent years discussion has expanded to ethical concerns (Rummel et al. 2012 ). ...

Planetary protection: an international concern and responsibility

Frontiers in Astronomy and Space Sciences

... These have been corrected according to the method implemented by F. G. Carrozzo et al. (2016). Residual slope effects have been corrected as discussed in A. Raponi et al. (2023). The observed spectra of Ceres's surface are affected by thermal emissions longward of 3.2 μm, which hides the absorption bands and prevents comparison with laboratory reflectance spectra of analogous materials. ...

Ceres as Seen by VIR/Dawn: Spectral Modeling and Laboratory Measurements Suggest Altered and Pristine Silicates Within Carbon Chemistry
  • Citing Chapter
  • September 2023

... In addition, essential elements to consider are not only human safety but planetary protection as well. In this study, we define planetary protection as the responsibility to avoid the unwanted contamination of habitable sites of interest with terrestrial microorganisms also known as forward contamination, as well as the contamination of Earth with dangerous material, known as backward contamination (Coustenis et al., 2023). ...

Planetary protection: Updates and challenges for a sustainable space exploration
  • Citing Article
  • March 2023

Acta Astronautica

... According to L. A. Yarzábal et al. (2021), ice sheet melt and permafrost thaw induced by global warming could release pathogenic microorganisms, and expose human population to a risk of biological contamination. Regarding pathogens of extraterrestrial origin, the risk of biological contamination is taken very seriously by organizations such as NASA and ESA for all space missions (Glavin et al., 2004(Glavin et al., & 2010Zorzano et al., 2023). The main kind of risks identified are the contamination from Earth on other planets (including their possible moons), as well as contamination of extraterrestrial origin upon return from certain missions, for example, in anticipation of future return missions to Mars. ...

The COSPAR Planetary Protection Requirements for Space Missions to Venus
  • Citing Article
  • February 2023

Life Sciences in Space Research

... The science operations team had to reconcile the science goals of assessing habitability and biosignature preservation with the Icelandic terrestrial field site. Although the initial site selection process (Basu et al. 2022) avoided exploration zones that would be classified as "special regions" on Mars, referring to regions of specific water and temperature activity that may be contaminated by terrestrial organisms and may sustain extant Martian life (Olsson- Francis et al. 2023), the team was asked to be cautious of and ignore any such features during the mission. The team also ignored "Earth-isms" that would not exist on the Martian surface, including meteoric water and any vegetation (e.g., lichen). ...

The COSPAR Planetary Protection Policy for robotic missions to Mars: A review of current scientific knowledge and future perspectives
  • Citing Article
  • December 2022

Life Sciences in Space Research

... all related to space science activities. One of the core activities of COSPAR since the earliest days of space exploration has been to develop, maintain, and promote an international Policy on Planetary Protection (referred to as "the Policy" hereafter) with its associated requirements (Coustenis et al., 2021e;2022f). This Policy constitutes the primary scientifically authoritative international reference standard to guide compliance with Article IX of the Outer Space Treaty and is the only internationally agreed planetary protection standard available for reference and use by all States and is based on the latest available scientific data. ...

Planetary Protection: an international concern and responsibility
  • Citing Conference Paper
  • October 2021

... Callegari et al. [34] review how optical tweezers have been successfully used to quantitatively study critical Casimir forces acting on particles in suspensions. Finally, Polimeno et al. (space tweezers collaboration) [35] describe how optical tweezers could be used to trap and characterize extraterrestrial particulate matter opening perspectives for optical tweezers applications in space, on planetary bodies surface, or in curator facilities designed for the uncontaminated handling and preliminary characterization of extraterrestrial samples returned by space probes. ...

Correction to: Optical tweezers in a dusty universe

The European Physical Journal Plus

... To manage the high computational demands, a multilevel particle size simulation is used, with thermal sieves placed between zones to assess the impact of specific heat capacity and thermal conductivity. The results from these simulations, which use the central composite design technique [88], reveal temperature variations based on the distance from the heat source and depth, as illustrated in Fig. 11. ...

Subsurface Thermal Modeling of Oxia Planum, Landing Site of ExoMars 2022

... Neither, we do not know of any research that has specifically looked at this topic-the distribution of potential S-type impactor material on Ceres. Another point to note is that the organic-rich areas in the Ernutet region contain higher-than-background amounts of ammoniated compounds and carbonates (De Sanctis & Ammannito, 2021;De Sanctis et al., 2019), and even organic-amines . Amines are known to exist on comets (Glavin et al., 2008), while evidence for ammoniated salts have been found on 67/P (Altwegg et al., 2020), and carbonates on 9P/Tempel 1 (Lisse et al., 2006). ...

Organic Matter and Associated Minerals on the Dwarf Planet Ceres