FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3214048552> ?p ?o ?g. }

• W3214048552 endingPage "2177" @default.
• W3214048552 startingPage "2166" @default.
• W3214048552 abstract "Abstract The scientific aims of the ExoMars Raman laser spectrometer (RLS) include identifying biological signatures and evidence of mineralogical processes associated with life. The RLS instrument was optimised to identify carbonaceous material, including reduced carbon. Previous studies suggest that reduced carbon on the Martian surface (perhaps originating from past meteoric bombardment) could provide a feedstock for microbial life. Therefore, its origin, form, and thermal history could greatly inform our understanding of Mars' past habitability. Here, we report on the Raman analysis of a Nakhla meteorite analogue (containing carbonaceous material) that was subjected to shock through projectile impact to simulate the effect of meteorite impact. The characterisation was performed using the RLS Simulator, in an equivalent manner to that planned for ExoMars operations. The spectra obtained verify that the flight‐representative system can detect reduced carbon in the basaltic sample, discerning between materials that have experienced different levels of thermal processing due to impact shock levels. Furthermore, carbon signatures acquired from the cratered material show an increase in molecular disorder (and we note that this effect will be more evident at higher levels of thermal maturity). This is likely to result from intense shearing forces, suggesting that shock forces within basaltic material may produce more reactive carbon. This result has implications for potential (past) Martian habitability because impacted, reduced carbon may become more biologically accessible. The data presented suggest the RLS instrument will be able to characterise the contribution of impact shock within the landing site region, enhancing our ability to assess habitability." @default.
• W3214048552 created "2021-11-22" @default.
• W3214048552 creator A5000922772 @default.
• W3214048552 creator A5001831052 @default.
• W3214048552 creator A5005312067 @default.
• W3214048552 creator A5022116869 @default.
• W3214048552 creator A5027037508 @default.
• W3214048552 creator A5028353549 @default.
• W3214048552 creator A5029903417 @default.
• W3214048552 creator A5037616158 @default.
• W3214048552 creator A5038855683 @default.
• W3214048552 creator A5045225369 @default.
• W3214048552 creator A5054362408 @default.
• W3214048552 creator A5070711597 @default.
• W3214048552 creator A5080703826 @default.
• W3214048552 creator A5087046444 @default.
• W3214048552 date "2021-11-14" @default.
• W3214048552 modified "2023-10-16" @default.
• W3214048552 title "Raman analysis of a shocked planetary surface analogue: Implications for habitability on Mars" @default.
• W3214048552 cites W102890565 @default.
• W3214048552 cites W1515758462 @default.
• W3214048552 cites W1569975934 @default.
• W3214048552 cites W1627138883 @default.
• W3214048552 cites W1910285401 @default.
• W3214048552 cites W1968713120 @default.
• W3214048552 cites W1974789074 @default.
• W3214048552 cites W1986165420 @default.
• W3214048552 cites W1993866574 @default.
• W3214048552 cites W1995418678 @default.
• W3214048552 cites W1999462954 @default.
• W3214048552 cites W1999611029 @default.
• W3214048552 cites W1999917630 @default.
• W3214048552 cites W2000554912 @default.
• W3214048552 cites W2007830908 @default.
• W3214048552 cites W2008060407 @default.
• W3214048552 cites W2010120004 @default.
• W3214048552 cites W2013086764 @default.
• W3214048552 cites W2013915611 @default.
• W3214048552 cites W2015461311 @default.
• W3214048552 cites W2021211105 @default.
• W3214048552 cites W2026006742 @default.
• W3214048552 cites W2027356372 @default.
• W3214048552 cites W2031336265 @default.
• W3214048552 cites W2043580782 @default.
• W3214048552 cites W2055493473 @default.
• W3214048552 cites W2058272047 @default.
• W3214048552 cites W2063109427 @default.
• W3214048552 cites W2075695772 @default.
• W3214048552 cites W2077714491 @default.
• W3214048552 cites W2088201877 @default.
• W3214048552 cites W2103142455 @default.
• W3214048552 cites W2125419520 @default.
• W3214048552 cites W2136334331 @default.
• W3214048552 cites W2138345137 @default.
• W3214048552 cites W2149517079 @default.
• W3214048552 cites W2152008139 @default.
• W3214048552 cites W2292799737 @default.
• W3214048552 cites W2317113369 @default.
• W3214048552 cites W2321654347 @default.
• W3214048552 cites W2342146731 @default.
• W3214048552 cites W2489768456 @default.
• W3214048552 cites W2520881360 @default.
• W3214048552 cites W2586944994 @default.
• W3214048552 cites W2591369712 @default.
• W3214048552 cites W2732794720 @default.
• W3214048552 cites W2735137573 @default.
• W3214048552 cites W2736984421 @default.
• W3214048552 cites W2737269925 @default.
• W3214048552 cites W2738005120 @default.
• W3214048552 cites W2744625907 @default.
• W3214048552 cites W2757563417 @default.
• W3214048552 cites W2792696357 @default.
• W3214048552 cites W2801808652 @default.
• W3214048552 cites W2890114096 @default.
• W3214048552 cites W2913089787 @default.
• W3214048552 cites W2947998320 @default.
• W3214048552 cites W2969676768 @default.
• W3214048552 cites W3118242898 @default.
• W3214048552 cites W3153678752 @default.
• W3214048552 cites W3087608634 @default.
• W3214048552 doi "https://doi.org/10.1002/jrs.6263" @default.
• W3214048552 hasPublicationYear "2021" @default.
• W3214048552 type Work @default.
• W3214048552 sameAs 3214048552 @default.
• W3214048552 citedByCount "2" @default.
• W3214048552 countsByYear W32140485522021 @default.
• W3214048552 countsByYear W32140485522023 @default.
• W3214048552 crossrefType "journal-article" @default.
• W3214048552 hasAuthorship W3214048552A5000922772 @default.
• W3214048552 hasAuthorship W3214048552A5001831052 @default.
• W3214048552 hasAuthorship W3214048552A5005312067 @default.
• W3214048552 hasAuthorship W3214048552A5022116869 @default.
• W3214048552 hasAuthorship W3214048552A5027037508 @default.
• W3214048552 hasAuthorship W3214048552A5028353549 @default.
• W3214048552 hasAuthorship W3214048552A5029903417 @default.
• W3214048552 hasAuthorship W3214048552A5037616158 @default.
• W3214048552 hasAuthorship W3214048552A5038855683 @default.
• W3214048552 hasAuthorship W3214048552A5045225369 @default.

• next