Observational Constraints on Late Heavy Bombardment Episodes Around Young Solar Analogs

Gaidos, E. J.

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