Spectral properties of Titan's impact craters imply chemical weathering of its surface

We examined the spectral properties of a selection of Titan's impact craters that represent a range of degradation states. The most degraded craters have rims and ejecta blankets with spectral characteristics that suggest that they are more enriched in water ice than the rims and ejecta blanket...

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Détails bibliographiques
Publié dans:Geophysical research letters. - 1984. - 42(2015), 10 vom: 28. Mai, Seite 3746-3754
Auteur principal: Neish, C D (Auteur)
Autres auteurs: Barnes, J W, Sotin, C, MacKenzie, S, Soderblom, J M, Le Mouélic, S, Kirk, R L, Stiles, B W, Malaska, M J, Le Gall, A, Brown, R H, Baines, K H, Buratti, B, Clark, R N, Nicholson, P D
Format: Article
Langue:English
Publié: 2015
Accès à la collection:Geophysical research letters
Sujets:Journal Article Titan erosion and weathering impact cratering