| Revision as of 05:24, 21 December 2024 editAngilbas (talk | contribs)Extended confirmed users3,032 edits Correction: Not 127 light years but 127 parsecs.← Previous edit | Revision as of 07:21, 21 December 2024 edit undoIdoghor Melody (talk | contribs)Autopatrolled, Event coordinators, Extended confirmed users, Page movers, IP block exemptions, New page reviewers, Pending changes reviewers32,603 editsm clean up, added uncategorised tagTag: AWBNext edit → | ||
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| HIP 67522 is a G-class star which is slightly larger (1.38 R Sun) and cooler (5675ºK vs. 5772ºK for Sun). It lies about 127 ] away from the Solar System and in Earth's sky it is at Right Ascension 13h50m06s, Declination -40º51'09". Its visual magnitude of 9.8 makes it much too faint to be seen by the unaided eye. | '''HIP 67522''' is a G-class star which is slightly larger (1.38 R Sun) and cooler (5675ºK vs. 5772ºK for Sun). It lies about 127 ] away from the Solar System and in Earth's sky it is at Right Ascension 13h50m06s, Declination -40º51'09". Its visual magnitude of 9.8 makes it much too faint to be seen by the unaided eye. | ||
| Two exoplanets, ] and ], are known to orbit the star and transit its face as seen from Earth. Their orbital periods are much less than Mercury's 88 days around the Sun, being 6.96 days for ''b'' and 14.33 days for ''c''.<ref>https://exoplanetarchive.ipac.caltech.edu/overview/HIP%2067522 NASA Exoplanet Archive</ref> | Two exoplanets, ] and ], are known to orbit the star and transit its face as seen from Earth. Their orbital periods are much less than Mercury's 88 days around the Sun, being 6.96 days for ''b'' and 14.33 days for ''c''.<ref>https://exoplanetarchive.ipac.caltech.edu/overview/HIP%2067522 NASA Exoplanet Archive</ref> | ||
| ==References== | |||
| {{Reflist}} | |||
| {{Uncategorized|date=December 2024}} | |||
Revision as of 07:21, 21 December 2024
HIP 67522 is a G-class star which is slightly larger (1.38 R Sun) and cooler (5675ºK vs. 5772ºK for Sun). It lies about 127 parsecs away from the Solar System and in Earth's sky it is at Right Ascension 13h50m06s, Declination -40º51'09". Its visual magnitude of 9.8 makes it much too faint to be seen by the unaided eye.
Two exoplanets, HIP 67522 b and HIP 67522 c, are known to orbit the star and transit its face as seen from Earth. Their orbital periods are much less than Mercury's 88 days around the Sun, being 6.96 days for b and 14.33 days for c.
References
- https://exoplanetarchive.ipac.caltech.edu/overview/HIP%2067522 NASA Exoplanet Archive
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