Atmosphere-interior exchange on hot rocky exoplanets

We provide estimates of atmospheric pressure and surface composition on short-period rocky exoplanets with dayside magma pools and silicate vapor atmospheres.

Atmospheric pressure tends toward vapor-pressure equilibrium with surface magma, and magma-surface composition is set by the competing effects of fractional vaporization and surface-interior exchange. We use basic models to show how surface-interior exchange is controlled by the planet’s temperature, mass, and initial composition. We assume that mantle rock undergoes bulk melting to form the magma pool, and that winds flow radially away from the substellar point.

With these assumptions, we find that: (1) atmosphere-interior exchange is fast when the planet’s bulk-silicate FeO concentration is low, and slow when FeO concentration is high; (2) magma pools are compositionally well-mixed for substellar temperatures ? 2400 K, but compositionally variegated and rapidly variable for substellar temperatures ? 2400 K; (3) currents within the magma pool tend to cool the top of the solid mantle (“tectonic refrigeration”); (4) contrary to earlier work, many magma planets have time-variable surface compositions.

Edwin S. Kite, Bruce Fegley Jr., Laura Schaefer, Eric Gaidos
(Submitted on 21 Jun 2016)

Comments: Accepted for publication by ApJ, 21 pages, 19 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:1606.06740 [astro-ph.EP] (or arXiv:1606.06740v1 [astro-ph.EP] for this version)
Submission history
From: Edwin Kite Edwin Kite
[v1] Tue, 21 Jun 2016 20:00:04 GMT (5943kb,D)
http://arxiv.org/abs/1606.06740