On equilibrium tides in fully convective planets and stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

The size of the shown abstract is reduced. Submitted to MNRAS

Scientific paper

10.1111/j.1365-2966.2004.08136.x

We consider the tidal interaction of a fully convective primary star and a point mass. Using a normal mode decomposition we calculate the evolution of the primary angular velocity and orbit for arbitrary eccentricity e. The dissipation acting on the tidal perturbation is associated with convective turbulence. A novel feature of the Paper is that, to take into account of the fact that there is a relaxation time t_{c}, being the turn-over time of convective eddies, associated with the process, this is allowed to act non locally in time, producing a dependence of the dissipation on tidal forcing frequency. Results are expressed in terms of the Fourier coefficients of the tidal potential. We find analytical approximations for these valid for $e>0.2$. When the tidal response is frequency independent, our results are equivalent to those obtained in the standard constant time lag approximation. When there is the frequency dependence of the dissipative response, the evolution can differ drastically. In that case the system can evolve through a sequence of spin-orbit corotation resonances with Omega_{r}/Omega_{orb}=n/2, where Omega_{r} and Omega_{orb} are the rotation and orbital frequencies and n is an integer. We study this case analytically and numerically.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

On equilibrium tides in fully convective planets and stars 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 On equilibrium tides in fully convective planets and stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On equilibrium tides in fully convective planets and stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-322642

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.