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pro vyhledávání: '"Bond, Jade C."'
The Gao-Guenie H5 chondrite that fell on Burkina Faso (March 1960) has portions that were impact-melted on an H chondrite asteroid at similar to 300 Ma and, through later impact events in space, sent into an Earth-crossing orbit. This article present
Externí odkaz:
http://hdl.handle.net/10150/621226
http://arizona.openrepository.com/arizona/handle/10150/621226
http://arizona.openrepository.com/arizona/handle/10150/621226
Prior work has found that a variety of terrestrial planetary compositions are expected to occur within known extrasolar planetary systems. However, such studies ignored the effects of giant planet migration, which is thought to be very common in extr
Externí odkaz:
http://arxiv.org/abs/1209.5125
Autor:
Carter-Bond, Jade C., O'Brien, David P., Mena, Elisa Delgado, Israelian, Garik, Santos, Nuno C., Hernandez, Jonay I. Gonzalez
Simulations have shown that a diverse range of extrasolar terrestrial planet bulk compositions are likely to exist, based on the observed variations in host star elemental abundances. Based on recent studies, it is expected that a significant proport
Externí odkaz:
http://arxiv.org/abs/1201.1939
Autor:
Mena, Elisa Delgado, Israelian, Garik, González-Hernández, Jonay I., Bond, Jade C., Santos, Nuno C., Udry, Stephane, Mayor, Michel
Theoretical studies suggest that C/O and Mg/Si are the most important elemental ratios in determining the mineralogy of terrestrial planets. The C/O ratio controls the distribution of Si among carbide and oxide species, while Mg/Si gives information
Externí odkaz:
http://arxiv.org/abs/1009.5224
Extrasolar planet host stars have been found to be enriched in key planet-building elements. These enrichments have the potential to drastically alter the composition of material available for terrestrial planet formation. Here we report on the combi
Externí odkaz:
http://arxiv.org/abs/1004.0971
No terrestrial planet formation simulation completed to date has considered the detailed chemical composition of the planets produced. While many have considered possible water contents and late veneer compositions, none have examined the bulk elemen
Externí odkaz:
http://arxiv.org/abs/0911.0426
Publikováno v:
Proceedings of the International Astronomical Union. Aug2012 Supplement, Vol. 8 Issue S293, p229-234. 6p.
Publikováno v:
Proceedings of the International Astronomical Union. 08/05/2009, Vol. 5 Issue S265, p399-402. 4p.
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