Prevalence of short-lived radioactive isotopes across exoplanetary systems inferred from polluted white dwarfs
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 515:1 (2022) 395-406
Modeling Thermal Emission under Lunar Surface Environmental Conditions
The Planetary Science Journal American Astronomical Society 3:7 (2022) 180
Water observed in the atmosphere of τ Boötis Ab with CARMENES/CAHA
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 514:3 (2022) 4160-4172
Charon’s refractory factory
Science Advances American Association for the Advancement of Science 8:24 (2022) eabq5701
Abstract:
We combine novel laboratory experiments and exospheric modeling to reveal that “dynamic” Ly-α photolysis of Plutonian methane generates a photolytic refractory distribution on Charon that increases with latitude, consistent with poleward darkening observed in the New Horizons images. The flux ratio of the condensing methane to the interplanetary medium Ly-α photons, φ, controls the distribution and composition of Charon’s photoproducts. Mid-latitude regions are likely to host complex refractories emerging from low-φ photolysis, while high-φ photolysis at the polar zones primarily generate ethane. However, ethane being colorless does not contribute to the reddish polar hue. Solar wind radiolysis of Ly-α–cooked polar frost past spring sunrise may synthesize increasingly complex, redder refractories responsible for the unique albedo on this enigmatic moon.Water observed in the atmosphere of {\tau} Bootis Ab with CARMENES/CAHA
(2022)