The chemical composition of impact craters on Titan: I. Implications for exogenic processing
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F60460709%3A41330%2F20%3A82261" target="_blank" >RIV/60460709:41330/20:82261 - isvavai.cz</a>
Result on the web
<a href="https://www.aanda.org/articles/aa/abs/2020/09/aa37866-20/aa37866-20.html" target="_blank" >https://www.aanda.org/articles/aa/abs/2020/09/aa37866-20/aa37866-20.html</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202037866" target="_blank" >10.1051/0004-6361/202037866</a>
Alternative languages
Result language
angličtina
Original language name
The chemical composition of impact craters on Titan: I. Implications for exogenic processing
Original language description
We investigate the spectral behavior of nine Titan impact craters in order to constrain their composition. Past studies that have examined the chemical composition of impact craters on Titan have either used qualitative comparisons between craters or combined all craters into a single unit, rather than separating them by geographic location and/or degradation state. Here, we use Visual and Infrared Mapping Spectrometer (VIMS) data and a radiative transfer code to estimate the atmospheric contribution to the data, extract the surface albedos of the impact craters, and constrain their composition by using a library of candidate Titan materials, including essentially water ice, tholin, a dark component, and other possible ices at different grain sizes. Following a general characterization of the impact craters, we study two impact crater subunits, the crater floor and the ejecta blanket. The results show that the equatorial dune craters-Selk, Ksa, Guabonito, and the crater on Santorini Facula-appear to
Czech name
—
Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GJ20-27624Y" target="_blank" >GJ20-27624Y: Synthetic and Comparative Hydrology of Earth, MArs and TitAn (SCHEMATA)</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
ASTRONOMY & ASTROPHYSICS
ISSN
0004-6361
e-ISSN
1432-0746
Volume of the periodical
641
Issue of the periodical within the volume
A16
Country of publishing house
CZ - CZECH REPUBLIC
Number of pages
14
Pages from-to
1-14
UT code for WoS article
000571554300004
EID of the result in the Scopus database
2-s2.0-85091334645