Ross 508: Difference between revisions
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Revision as of 20:10, 3 August 2022
Ross 508 is a 13th magnitude red dwarf star, 11.2183 parsecs away. The Ross catalog is named after Frank Elmore Ross who published a first list of 86 high proper motion stars in 1925.[1] In 2022 it was discovered to have a super-Earth, Ross 508b, orbiting every 10.77 days, detected by doppler spectroscopy.[2]
References
- ^ Ross, Frank E. (November 1, 1925). "New proper-motion stars, (first list)". The Astronomical Journal. 36: 96–99. Bibcode:1925AJ.....36...96R. doi:10.1086/104687.
- ^ Harakawa, Hiroki; et al. (2022). "A super-Earth orbiting near the inner edge of the habitable zone around the M4.5 dwarf Ross 508". Publications of the Astronomical Society of Japan. arXiv:2205.11986. Bibcode:2022PASJ..tmp...72H. doi:10.1093/pasj/psac044.
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