Recent findings of NO near Gale Crater on Mars have been explained by two pathways: formation of nitric acid (HNO3) in a warm climate or formation of peroxynitric acid (HO2NO2) in a cool climate. Here
Literature on the theory of exoplanet atmospheric disequilibrium chemistry is rich, although its ob- servational counterpart has yet to emerge beyond the hints provided by a few targets in dedicated s
PDS 70 recently became an object of immense interest following the discovery of two newly forming planets orbiting in a gap in the star.s protoplanetary disc. The system is close enough to be directly
These data support the findings of PHAZER Hörst Lab publication “Triton Haze Analogues: the Role of Carbon Monoxide in Haze Formation” by S.E. Moran et al. These include raw and processed mass spectro
Johns Hopkins Research Data Repository2021-12-21 更新80
Photochemical hazes are important opacity sources in temperate exoplanet atmospheres, hindering current observations from characterizing exoplanet atmospheric compositions. The haziness of an atmosphe
