Ross 508: Difference between revisions
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'''Rose 508''' is a 13th magnitude [[red dwarf]] star, 11.2183 [[parsecs]] away. In 2022 it was discovered to have a [[superearth]], ''Ross 508b'', orbiting every 10.77 days, detected by [[doppler spectroscopy]].<ref>https://academic.oup.com/pasj/advance-article/doi/10.1093/pasj/psac044/6623879</ref> |
'''Rose 508''' is a 13th magnitude [[red dwarf]] star, 11.2183 [[parsecs]] away. The Ross catalog is named after [[Frank Elmore Ross]] who published a list of 86 high proper motion starts in 1925.<ref>https://ui.adsabs.harvard.edu/abs/1925AJ.....36...96R/abstract</ref> |
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In 2022 it was discovered to have a [[superearth]], ''Ross 508b'', orbiting every 10.77 days, detected by [[doppler spectroscopy]].<ref>https://academic.oup.com/pasj/advance-article/doi/10.1093/pasj/psac044/6623879</ref> |
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==References== |
==References== |
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Revision as of 00:47, 2 August 2022
Rose 508 is a 13th magnitude red dwarf star, 11.2183 parsecs away. The Ross catalog is named after Frank Elmore Ross who published a list of 86 high proper motion starts in 1925.[1]
In 2022 it was discovered to have a superearth, Ross 508b, orbiting every 10.77 days, detected by doppler spectroscopy.[2]
References
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