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Haze Formation in Warm H2-rich Exoplanet Atmospheres by He, Chao; Horst, Sarah M.; Lewis, Nikole K.; Yu, Xinting; Moses, Julianne I.; McGuiggan, Patricia; Marley, Mark S.; Kempton, Eliza M. -R.; Morley, Caroline V.; Valenti, Jeff A.; Vuitton, Veronique is a scholarly article available to read on EtoBox.

What is Haze Formation in Warm H2-rich Exoplanet Atmospheres about?

New observing capabilities coming online over the next few years will provide opportunities for characterization of exoplanet atmospheres. However, clouds/hazes could be present in the atmospheres of many exoplanets, muting the amplitude of spectral features. We use laboratory simulations to explore photochemical haze formation in H2-rich exoplanet atmospheres at 800 K with metallicity either 100 and 1000 times solar. We find that haze particles are produced in both simulated atmospheres with small particle size (20 to 140 nm) and relative low production rate (2.4 x 10-5 to 9.7 x 10-5 mg cm-3 h-1), but the particle size and production rate is dependent on the initial gas mixtures and the energy sources used in the simulation experiments. The gas phase mass spectra show that complex chemical processes happen in these atmospheres and generate new gas products that can further react to form larger molecules and solid haze particles. Two H2-rich atmospheres with similar C/O ratios (~0.5) yield different haze particles size, haze production rate, and gas products, suggesting both the elemental abundances and their bonding environments in an atmosphere can significantly affect the photoc

Author

He, Chao; Horst, Sarah M.; Lewis, Nikole K.; Yu, Xinting; Moses, Julianne I.; McGuiggan, Patricia; Marley, Mark S.; Kempton, Eliza M. -R.; Morley, Caroline V.; Valenti, Jeff A.; Vuitton, Veronique

Published

2020

Language

EN