Talk:HD 117618
Latest comment: 9 years ago by 77.57.25.250 in topic Wittenmyer et al. (2013)
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Wittenmyer et al. (2013) edit
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)