Ross 508: Difference between revisions

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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 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]

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-'''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 first list of 86 high [[proper motion]] stars in 1925.<ref>https://ui.adsabs.harvard.edu/abs/1925AJ.....36...96R/abstract</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 first list of 86 high [[proper motion]] stars in 1925.<ref>{{Cite journal|url=https://ui.adsabs.harvard.edu/abs/1925AJ.....36...96R|title=New proper-motion stars, (first list)|first=Frank E.|last=Ross|date=November 1, 1925|journal=The Astronomical Journal|volume=36|pages=96–99|via=NASA ADS|doi=10.1086/104687}}</ref>
 In 2022 it was discovered to have a [[super-Earth]], ''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>