A giant planet orbiting the ‘extreme horizontal branch’ star V 391 Pegasi
A giant planet orbiting the ‘extreme horizontal branch’ star V 391 Pegasi
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Author / Creator
Silvotti, R. , Schuh, S. , Janulis, R. , Solheim, J.-E. , Bernabei, S. , Østensen, R. , Oswalt, T. D. , Bruni, I. , Gualandi, R. , Bonanno, A. , Vauclair, G. , Reed, M. , Chen, C.-W. , Leibowitz, E. , Paparo, M. , Baran, A. , Charpinet, S. , Dolez, N. , Kawaler, S. , Kurtz, D. , Moskalik, P. , Riddle, R. and Zola, S.
Publisher
London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Contents
Planets in the red
Most of the more than 200 known extrasolar planets orbit main sequence stars similar to our Sun. When the hydrogen in their cores runs out, they will become red giants that can easily reach and engulf inner planets. This will happen to the Sun in about five billion years. After that the fate of Earth is uncertain, but the disc...
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Full title
A giant planet orbiting the ‘extreme horizontal branch’ star V 391 Pegasi
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Record Identifier
TN_cdi_proquest_miscellaneous_68269697
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_68269697
Other Identifiers
ISSN
0028-0836
E-ISSN
1476-4687,1476-4679
DOI
10.1038/nature06143
