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  • sun evolution  (1)
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    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 73 (1996), S. 187-192 
    ISSN: 1573-0794
    Keywords: Mars ; planetary evolution ; sun evolution
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Recently, the possibility of strong mass loss from an early sun has been proposed in connection with the lithium depletion problem along with early solar system problems. However, the time scale for this enhanced mass loss is uncertain. Using an empirical relation for the dependence of the Martian surface temperature on solar luminosity and surface pressure, we find that the mass loss time scale for a 1.1 M⊙ sun should be about 1 × 109 years or longer if Mars had liquid water on its surface 3.8 billion years ago. The minimum surface pressure on early Mars should be about 5 bars of CO2.
    Type of Medium: Electronic Resource
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