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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

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • 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