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Organic composition of C/1999 S4 (LINEAR): a comet formed near Jupiter?
Mumma, M J; Dello Russo, N; DiSanti, M A; Magee-Sauer, K; Novak, R E; Brittain, S; Rettig, T; McLean, I S; Reuter, D C; Xu, L H.
Afiliação
  • Mumma MJ; Laboratory for Extraterrestrial Physics, Code 690, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. mmumma@kuiper.gsfc.nasa.gov
Science ; 292(5520): 1334-9, 2001 May 18.
Article em En | MEDLINE | ID: mdl-11359002
In the current paradigm, Oort cloud comets formed in the giant planets' region of the solar nebula, where temperatures and other conditions varied greatly. The measured compositions of four such comets (Halley, Hyakutake, Hale-Bopp, and Lee) are consistent with formation from interstellar ices in the cold nebular region beyond Uranus. The composition of comet C/1999 S4 (LINEAR) differs greatly, which suggests that its ices condensed from processed nebular gas, probably in the Jupiter-Saturn region. Its unusual organic composition may require reevaluation of the prebiotic organic material delivered to the young Earth by comets.
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Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Science Ano de publicação: 2001 Tipo de documento: Article País de afiliação: Estados Unidos
Buscar no Google
Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Science Ano de publicação: 2001 Tipo de documento: Article País de afiliação: Estados Unidos