Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2010-02-24
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Accepted to Nature, 14 pages, 1 figure
Scientific paper
The class of exotic Jupiter-mass planets that orbit very close to their parent stars were not explicitly expected before their discovery. The recently found transiting planet WASP-12b has a mass Mp = 1.4(+/-0.1) Jupiter masses (MJ), a mean orbital distance of only 3.1 stellar radii (meaning it is subject to intense tidal forces), and a period of 1.1 days. Its radius 1.79(+/- 0.09) RJ is unexpectedly large and its orbital eccentricity 0.049(+/-0:015) is even more surprising as such close orbits are in general quickly circularized. Here we report an analysis of its properties, which reveals that the planet is losing mass to its host star at a rate ~ 10^-7 MJ yr^-1. The planets surface is distorted by the stars gravity and the light curve produced by its prolate shape will differ by about ten per cent from that of a spherical planet. We conclude that dissipation of the stars tidal perturbation in the planets convective envelope provides the energy source for its large volume. We predict up to 10mJy CO band-head (2.292 micron) emission from a tenuous disk around the host star, made up of tidally stripped planetary gas. It may also contain a detectable resonant super-Earth, as a hypothetical perturber that continually stirs up WASP-12b's eccentricity.
Fortney Jonathan J.
Li Shu-lin
Lin Douglas N. C.
Miller Neil
No associations
LandOfFree
WASP-12b as a prolate, inflated and disrupting planet from tidal dissipation 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 WASP-12b as a prolate, inflated and disrupting planet from tidal dissipation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and WASP-12b as a prolate, inflated and disrupting planet from tidal dissipation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-261090