Photochemistry of Venus-like Planets Orbiting K- and M-dwarf Stars

@article{Jordan2021PhotochemistryOV,
  title={Photochemistry of Venus-like Planets Orbiting K- and M-dwarf Stars},
  author={Sean Jordan and Paul B. Rimmer and Oliver Shorttle and Tereza Constantinou},
  journal={The Astrophysical Journal},
  year={2021},
  volume={922}
}
Compared to the diversity seen in exoplanets, Venus is a veritable astrophysical twin of the Earth; however, its global cloud layer truncates features in transmission spectroscopy, masking its non-Earth-like nature. Observational indicators that can distinguish an exo-Venus from an exo-Earth must therefore survive above the cloud layer. The above-cloud atmosphere is dominated by photochemistry, which depends on the spectrum of the host star and therefore changes between stellar systems. We… 

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