Apparently the best-fit face-on orbit of HR 8799d is too eccentric to be stable. Seems that it may not be coplanar with the outer two planets and debris disk.
Sirius_Alpha Admin
Number of posts : 4320 Location : Earth Registration date : 2008-04-06
Subject: Re: HR 8799 astrometry 4th March 2011, 8:07 pm
Interestingy, the inclination constraints assuming a circular orbit for d seem to be consistent with the asteroseismically derived inclination axis of the star.
What is going on?
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