Literature DB >> 11599179

Contributions of icy planetesimals to the Earth's early atmosphere.

T C Owen1, A Bar-Nun.   

Abstract

Laboratory experiments on the trapping of gases by ice forming at low temperatures implicate comets as major carriers of the heavy noble gases to the inner planets. These icy planetesimals may also have brought the nitrogen compounds that ultimately produced atmospheric N2. However, if the sample of three comets analyzed so far is typical, the Earth's oceans cannot have been produced by comets alone, they require an additional source of water with low D/H. The highly fractionated neon in the Earth's atmosphere may also indicate the importance of non-icy carriers of volatiles. The most important additional carrier is probably the rocky material comprising the bulk of the mass of these planets. Venus may require a contribution from icy planetesimals formed at the low temperatures characteristic of the Kuiper Belt.

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Year:  2001        PMID: 11599179     DOI: 10.1023/a:1011809412925

Source DB:  PubMed          Journal:  Orig Life Evol Biosph        ISSN: 0169-6149            Impact factor:   1.950


  28 in total

1.  Fractionated martian atmosphere in the nakhlites?

Authors:  M J Drake; T D Swindle; T Owen; D S Musselwhite
Journal:  Meteoritics       Date:  1994

2.  Martian gases in an antarctic meteorite?

Authors:  D D Bogard; P Johnson
Journal:  Science       Date:  1983-08-12       Impact factor: 47.728

3.  A low-temperature origin for the planetesimals that formed Jupiter.

Authors:  T Owen; P Mahaffy; H B Niemann; S Atreya; T Donahue; A Bar-Nun; I de Pater
Journal:  Nature       Date:  1999-11-18       Impact factor: 49.962

4.  Possible cometary origin of heavy noble gases in the atmospheres of Venus, Earth and Mars

Authors:  T Owen; A Bar-Nun; I Kleinfeld
Journal:  Nature       Date:  1992-07-02       Impact factor: 49.962

5.  The spectrum of comet Hale-Bopp (C/1995 O1) observed with the Infrared Space Observatory at 2.9 astronomical units from the sun.

Authors:  J Crovisier; K Leech; D Bockelée-Morvan; T Y Brooke; M S Hanner; B Altieri; H U Keller; E Lellouch
Journal:  Science       Date:  1997-03-28       Impact factor: 47.728

6.  Composition and structure of the venus atmosphere: results from pioneer venus.

Authors:  J H Hoffman; R R Hodges; M B McElroy; T M Donahue; M Kolpin
Journal:  Science       Date:  1979-07-06       Impact factor: 47.728

7.  Water on Mars: Clues from Deuterium/Hydrogen and Water Contents of Hydrous Phases in SNC Meteorites.

Authors:  L L Watson; I D Hutcheon; S Epstein; E M Stolper
Journal:  Science       Date:  1994-07-01       Impact factor: 47.728

8.  Release of juvenile water on Mars: estimated amounts and timing associated with volcanism.

Authors:  R Greeley
Journal:  Science       Date:  1987-06-26       Impact factor: 47.728

9.  Retention of Solar Helium and Neon in IDPs in Deep Sea Sediment.

Authors:  H Hiyagon
Journal:  Science       Date:  1994-03-04       Impact factor: 47.728

10.  Deuterium on Mars: The Abundance of HDO and the Value of D/H.

Authors:  T Owen; J P Maillard; C de Bergh; B L Lutz
Journal:  Science       Date:  1988-06-24       Impact factor: 47.728

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  1 in total

Review 1.  Setting the scene: what did we know before Rosetta?

Authors:  K J Meech
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2017-07-13       Impact factor: 4.226

  1 in total

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