Ross 508

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Tomruen (talk | contribs) at 00:49, 2 August 2022. The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

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 superearth, Ross 508b, orbiting every 10.77 days, detected by doppler spectroscopy.[2]

References

  1. ^ https://ui.adsabs.harvard.edu/abs/1925AJ.....36...96R/abstract
  2. ^ https://academic.oup.com/pasj/advance-article/doi/10.1093/pasj/psac044/6623879

Template:Ross objects

Stub icon

This article about a red dwarf is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Ross_508&oldid=1101824905"