Luminosity and temperature relationships for extrasolar planets

Details Luminosity and temperature relationships for extrasolar planets Luminosity and temperature relationships for extrasolar planets

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.325.1497d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 325, Issue 4, pp. 1497-1499.

Astronomy and Astrophysics

Astronomy

Hertzsprung-Russell (Hr) Diagram, Planetary Systems

Scientific paper

A simple discussion of the final equilibrium state of extrasolar planetary evolution allows the determination of the luminosity and effective temperature of each planet which, in turn, allows the construction of a Hertzsprung-Russell diagram. The slope of the resulting line is found to be 4.5, similar to that which might be expected for isolated low-mass stars.

Affiliated with

Also associated with

No associations

Rating

Luminosity and temperature relationships for extrasolar 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 Luminosity and temperature relationships for extrasolar planets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminosity and temperature relationships for extrasolar planets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-802377