Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-01-06
Science298:1756,2002
Astronomy and Astrophysics
Astrophysics
13 pages, 2 Figures. Text and artwork are slightly different from the version published on Science. More hi-res picture and mo
Scientific paper
10.1126/science.1077635
The evolution of gravitationally unstable protoplanetary gaseous disks has been studied with the use of three-dimensional smoothed particle hydrodynamics simulations with unprecedented resolution. We have considered disks with initial masses and temperature profiles consistent with those inferred for the protosolar nebula and for other protoplanetary disks. We show that long-lasting, self-gravitating protoplanets arise after a few disk orbital periods if cooling is efficient enough to maintain the temperature close to 50 K. The resulting bodies have masses and orbital eccentricities similar to those of detected extrasolar planets.
Mayer Lucio
Quinn Thomas
Stadel Joachim
Wadsley James
No associations
LandOfFree
Formation of giant planets by fragmentation of protoplanetary disks 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 Formation of giant planets by fragmentation of protoplanetary disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of giant planets by fragmentation of protoplanetary disks will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-722301