Probabilistic Constraints on the Mass and Composition of Proxima b
Recent studies regarding the habitability, observability, and possible orbital evolution of the indirectly detected exoplanet Proxima b have mostly assumed a planet with M similar to 1.3 M-circle plus, a rocky composition, and an Earth-like atmosphere or none at all. In order to assess these assumpt...
Main Authors: | Bixel, Alex, Apai, Dániel |
---|---|
Other Authors: | Univ Arizona, Dept Planetary Sci, Lunar & Planetary Lab |
Language: | en |
Published: |
IOP PUBLISHING LTD
2017
|
Subjects: | |
Online Access: | http://hdl.handle.net/10150/623234 http://arizona.openrepository.com/arizona/handle/10150/623234 |
Similar Items
-
Chemical diversity of the atmospheres and interiors of sub-Neptunes: a case study of GJ 436 b
by: Guzmán-Mesa, A., et al.
Published: (2022) -
NO THERMAL INVERSION AND A SOLAR WATER ABUNDANCE FOR THE HOT JUPITER HD 209458B FROM HST /WFC3 SPECTROSCOPY
by: Line, Michael R., et al.
Published: (2016) -
Structure and Evolution of Internally Heated Hot Jupiters
by: Komacek, Thaddeus D., et al.
Published: (2017) -
An Observational Diagnostic for Distinguishing between Clouds and Haze in Hot Exoplanet Atmospheres
by: Kempton, Eliza M.-R., et al.
Published: (2017) -
Composition of Jupiter irregular satellites sheds light on their origin
by: Bhatt, M., et al.
Published: (2017)