Organic hazes will impact JWST observations of water-rich exoplanets
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-023-02141-3.pdf
Reference5 articles.
1. Kreidberg, L. et al. Clouds in the atmosphere of the super-Earth exoplanet GJ1214b. Nature 505, 69–72 (2014). This paper reports the presence of clouds and/or hazes in the sub-Neptune exoplanet, GJ1214b.
2. Gao, P. et al. Aerosol composition of hot giant exoplanets dominated by silicates and hydrocarbon hazes. Nat. Astron. 4, 951–956 (2020). In this paper the authors show that exoplanet atmospheres with planetary equilibrium temperatures below 950 K are dominated by organic hazes.
3. Hörst, S. M. et al. Haze production rates in super-Earth and mini-Neptune atmosphere experiments. Nat. Astron. 2, 303–306 (2018). This paper reports great diversity in haze production rates in super-Earth and mini-Neptune atmospheres.
4. Khare, B. N. et al. Optical constants of organic tholins produced in a simulated Titanian atmosphere: From soft X-ray to microwave frequencies. Icarus 60, 127–137 (1984). This paper reports the optical constants of Titan haze analogues across a wide wavelength range.
5. He, C. et al. Sulfur-driven haze formation in warm CO2-rich exoplanet atmospheres. Nat. Astron. 4, 986–993 (2020). This paper describes the PHAZER chamber used to simulate complex exoplanet atmospheric conditions.
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