Misplaced Pages

HIP 67522: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactivelyNext edit →Content deleted Content addedVisualWikitext
Revision as of 05:18, 21 December 2024 editAngilbas (talk | contribs)Extended confirmed users3,038 edits New article with reference.  Revision as of 05:24, 21 December 2024 edit undoAngilbas (talk | contribs)Extended confirmed users3,038 edits Correction: Not 127 light years but 127 parsecs.Next edit →
Line 1: Line 1:
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 light-years 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>

Revision as of 05:24, 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.

  1. https://exoplanetarchive.ipac.caltech.edu/overview/HIP%2067522 NASA Exoplanet Archive