Haze evolution in temperate exoplanet atmospheres through surface energy measurements-Reference-Cited by-同舟云学术

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Haze evolution in temperate exoplanet atmospheres through surface energy measurements

Published:2021-07-12 Issue:8 Volume:5 Page:822-831
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Yu Xinting^ORCID,He Chao^ORCID,Zhang Xi,Hörst Sarah M.^ORCID,Dymont Austin H.,McGuiggan Patricia,Moses Julianne I.^ORCID,Lewis Nikole K.,Fortney Jonathan J.,Gao Peter,Kempton Eliza M.-R.^ORCID,Moran Sarah E.^ORCID,Morley Caroline V.,Powell Diana^ORCID,Valenti Jeff A.,Vuitton Véronique^ORCID

Funder

Heising-Simons Foundation: 51 Pegasi b Postdoctoral Fellowship

National Aeronautics and Space Administration

3M Nontenured Faculty Grant

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01375-3.pdf

Reference67 articles.

1. Zhang, X., Strobel, D. F. & Imanaka, H. Haze heats Pluto’s atmosphere yet explains its cold temperature. Nature 551, 352–355 (2017).

2. Hörst, S. M. et al. Haze production rates in super-Earth and mini-Neptune atmosphere experiments. Nat. Astron. 2, 303–306 (2018).

3. Arney, G. et al. The pale orange dot: the spectrum and habitability of hazy Archean Earth. Astrobiology 16, 873–899 (2016).

4. Gao, P. et al. Aerosol composition of hot giant exoplanets dominated by silicates and hydrocarbon hazes. Nat. Astron. 4, 951–956 (2020).

5. Knutson, H. A., Benneke, B., Deming, D. & Homeier, D. A featureless transmission spectrum for the Neptune-mass exoplanet GJ 436b. Nature 505, 66–68 (2014).

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