This is an old revision of this page, as edited by Idoghor Melody (talk | contribs) at 07:21, 21 December 2024 (clean up, added uncategorised tag). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
Revision as of 07:21, 21 December 2024 by Idoghor Melody (talk | contribs) (clean up, added uncategorised tag)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)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
 | This article has not been added to any content categories. Please help out by adding categories to it so that it can be listed with similar articles. (December 2024) |