Physics
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..799n&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.799
Physics
Scientific paper
We present interior models of the outer planets in the solar system. We find that none of these planets can have a constant metallicity throughout the interior. For Uranus we find a significantly smaller outer envelope metallicity than for Neptune. The cooling time of Uranus can be brought into agreement with the age of the solar system if the deep interior is assumed to have a lower heat flux than along an adiabatic gradient. For Saturn, our models predict an atmospheric He/H mass fraction of 0.1, i.e. smaller than Jupiter's.
Fortney Jonathan J.
Helled Ravit
Nettelmann Nadine
Redmer Ronald
No associations
LandOfFree
Our inhomogeneous and unique outer planets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Our inhomogeneous and unique outer planets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Our inhomogeneous and unique outer planets will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1480648