Literature DB >> 9743493

Implications of Mars Pathfinder data for the accretion history of the terrestrial planets.

C M Bertka1, Y Fei.   

Abstract

Accretion models of the terrestrial planets often assume planetary bulk compositions with nonvolatile element abundance ratios equivalent to those of C1 carbonaceous chondrites. The moment of inertia factor of Mars reported by the Pathfinder team is inconsistent with a bulk planet C1 Fe/Si ratio or Fe content, which suggests that C1 chondrite accretion models are insufficient to explain the formation of Mars and the other terrestrial planets. Future planetary accretion models will have to account for variations in bulk Fe/Si ratios among the terrestrial planets.

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Year:  1998        PMID: 9743493     DOI: 10.1126/science.281.5384.1838

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  2 in total

1.  Core Formation and Geophysical Properties of Mars.

Authors:  Matthew C Brennan; Rebecca A Fischer; Jessica C E Irving
Journal:  Earth Planet Sci Lett       Date:  2019-11-11       Impact factor: 5.255

2.  Toward a mineral physics reference model for the Moon's core.

Authors:  Daniele Antonangeli; Guillaume Morard; Nicholas C Schmerr; Tetsuya Komabayashi; Michael Krisch; Guillaume Fiquet; Yingwei Fei
Journal:  Proc Natl Acad Sci U S A       Date:  2015-03-16       Impact factor: 11.205

  2 in total

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