Talk:HD 117618

Wittenmyer et al. (2013)
Wittenmyer et al. (2013) demonstrates that an eccentric planet can be modelled as two low-eccentricity planets (this is in fact a known degeneracy). Nevertheless these orbital solutions are not widely-accepted and are misleading to the general reader. I have therefore reverted the article back to the accepted one-planet solution. 77.57.25.250 (talk) 18:15, 2 July 2014 (UTC)