April 2025
·
28 Reads
Acta Astronautica
This page lists works of an author who doesn't have a ResearchGate profile or hasn't added the works to their profile yet. It is automatically generated from public (personal) data to further our legitimate goal of comprehensive and accurate scientific recordkeeping. If you are this author and want this page removed, please let us know.
April 2025
·
28 Reads
Acta Astronautica
February 2025
·
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.
October 2024
·
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.
October 2024
·
28 Reads
·
1 Citation
International Journal of Impact Engineering
April 2024
·
92 Reads
·
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.
February 2024
·
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.
February 2024
·
11 Reads
January 2024
·
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.
January 2024
·
12 Reads
January 2024
·
3 Reads
... 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. ...
April 2024
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 ). ...
Reference:
Where the microbes aren't
May 2023
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. ...
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). ...
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. ...
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). ...
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. ...
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. ...
November 2021
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. ...
September 2021
... 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). ...
July 2021