Exoplanets around Red Giants: Distribution and Habitability

Author:

Chen Ruixuan E.12,Jiang Jonathan H.2ORCID,Rosen Philip E.3,Fahy Kristen A.2,Chen Yanbei4

Affiliation:

1. Arcadia High School, Arcadia, CA 91006, USA

2. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91099, USA

3. Independent Researcher, Vancouver, WA 98662, USA

4. Theoretical Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA

Abstract

As the search for exoplanets continues, more are being discovered orbiting Red Giant stars. We use current data from the NASA Exoplanet Archive to investigate planet distribution around Red Giant stars and their presence in the host’s habitable zone. As well, we explore the distribution of planet mass and orbital semi major axis for evolved stars with increasing stellar radii. From the distance distribution of the planets, we found evidence of engulfment during the post-Main Sequence evolution of the star. We found 9 Red Giant-hosted exoplanets, and 21 Subgiant-hosted exoplanets to be in the optimistically calculated habitable zone, 5 and 17 of which are in a more conservatively calculated habitable zone. All the planets detected within their habitable zone orbit stars that are in early stages of evolution. We believe that with more powerful instrumentation, more habitable planets may be found around stars that are in later stages of evolution.

Funder

NASA Exoplanet Research Program NNH22ZDA001N-XRP

Publisher

MDPI AG

Subject

Astronomy and Astrophysics

Reference46 articles.

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