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Observational Constraints on Late Heavy Bombardment Episodes Around Young Solar Analogs

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dc.contributor.author Gaidos, E. J. en_US
dc.date.accessioned 2004-09-25T17:31:34Z
dc.date.available 2004-09-25T17:31:34Z
dc.date.issued 1998-10 en_US
dc.identifier.citation Astrophysical Journal Letters en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-1752 en_US
dc.identifier.uri http://hdl.handle.net/2014/20695
dc.description.abstract The excess thermal infrared emission from 36 G and K stars with ages corresponding to the period of Late Heavy Bombardment on the Moon (prior to 3.8 Ga) is estimated. These stars are among 38 selected by analogy to the Sun at an age less than 0.8 Gyr. en_US
dc.format.extent 1045243 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other origin of life early earth planetary systems astrobiology en_US
dc.title Observational Constraints on Late Heavy Bombardment Episodes Around Young Solar Analogs en_US


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