Literature DB >> 17611535

Hyperion's sponge-like appearance.

P C Thomas1, J W Armstrong, S W Asmar, J A Burns, T Denk, B Giese, P Helfenstein, L Iess, T V Johnson, A McEwen, L Nicolaisen, C Porco, N Rappaport, J Richardson, L Somenzi, P Tortora, E P Turtle, J Veverka.   

Abstract

Hyperion is Saturn's largest known irregularly shaped satellite and the only moon observed to undergo chaotic rotation. Previous work has identified Hyperion's surface as distinct from other small icy objects but left the causes unsettled. Here we report high-resolution images that reveal a unique sponge-like appearance at scales of a few kilometres. Mapping shows a high surface density of relatively well-preserved craters two to ten kilometres across. We have also determined Hyperion's size and mass, and calculated the mean density as 544 +/- 50 kg m(-3), which indicates a porosity of >40 per cent. The high porosity may enhance preservation of craters by minimizing the amount of ejecta produced or retained, and accordingly may be the crucial factor in crafting this unusual surface.

Entities:  

Year:  2007        PMID: 17611535     DOI: 10.1038/nature05779

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


  1 in total

1.  Detection of a strongly negative surface potential at Saturn's moon Hyperion.

Authors:  T A Nordheim; G H Jones; E Roussos; J S Leisner; A J Coates; W S Kurth; K K Khurana; N Krupp; M K Dougherty; J H Waite
Journal:  Geophys Res Lett       Date:  2014-10-16       Impact factor: 4.720

  1 in total

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