A tidally destructed massive planet as the progenitor of the two light planets around the sdB star KIC 05807616
arXiv:1202.1168 · doi:10.1088/2041-8205/749/1/L14
Abstract
We propose that the two newly detected Earth-size planets around the hot B subdwarf star KIC 05807616 are remnant of the tidally destructed metallic core of a massive planet. A single massive gas-giant planet was spiralling-in inside the envelope of the red giant branch star progenitor of the extreme horizontal branch (EHB) star KIC 05807616. The released gravitational energy unbound most of the stellar envelope, turning it into an EHB star. The massive planet reached the tidal destruction radius of ~Ro from the core, where the planet's gaseous envelope was tidally removed. In our scenario the metallic core of the massive planet was tidally destructed into several Earth-like bodies immediately after the gaseous envelope of the planet was removed. Two, and possibly more, Earth-size fragments survived at orbital separations of >Ro within the gaseous disk. The bodies interact with the disk and among themselves and migrated to reach orbits close to a 3:2 resonance. These observed planets can have a planetary magnetic field about ten times as strong as that of Earth. This strong magnetic field can substantially reduce the evaporation rate from the planets and explain their survivability against the strong UV radiation of the EHB star.
Submitted
References in corpus (7)
- Stellar disruption by a supermassive black hole: is the light curve really proportional to ?
- The sdB+M Eclipsing System HW Virginis and its Circumbinary Planets
- A binary model for the UV-upturn of elliptical galaxies (MNRAS version)
- Circumbinary Planets Orbiting the Rapidly Pulsating Subdwarf B-type binary NY Vir
- Detection of a tertiary brown dwarf companion in the sdB-type eclipsing binary HS 0705+6700
- Stars Don't Eat Their Young Migrating Planets - Empirical Constraints On Planet Migration Halting Mechanisms
- Super-Earths: A New Class of Planetary Bodies
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