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2013•Astronomy and AstrophysicsOpen access

Study of the impact of the post-MS evolution of the host star on the orbits of close-in planets

M. I. Jones, J. S. Jenkins, P. Rojo, C. Melo, P. Bluhm

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Abstract

Context. More than 40 planets have been found around giant stars, revealing a lack of systems orbiting interior to ~0.6 AU. This observational fact contrasts with the planetary population around solar-type stars and has been interpreted as the result of the orbital evolution of planets through the interaction with the host star and/or because of a different formation/migration scenario of planets around more massive stars.

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Context. More than 40 planets have been found around giant stars, revealing a lack of systems orbiting interior to ~0.6 AU. This observational fact contrasts with the planetary population around solar-type stars and has been interpreted as the result of the orbital evolution of planets through the interaction with the host star and/or because of a different formation/migration scenario of planets around more massive stars.

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Available abstract

Context. More than 40 planets have been found around giant stars, revealing a lack of systems orbiting interior to ~0.6 AU. This observational fact contrasts with the planetary population around solar-type stars and has been interpreted as the result of the orbital evolution of planets through the interaction with the host star and/or because of a different formation/migration scenario of planets around more massive stars.

Key concepts: Planet, Physics, Stars, Planetary system, Context (archaeology), Habitability of orange dwarf systems, Astronomy, Astrobiology

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