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I'm going to pick out my five favorite abstracts and post one per day this week!

Next HAZMAT paper! Predicting the evolution of the unobservable extreme-UV radiation from early M stars, which drives planetary atmospheric escape and directly impacts a planet's potential for habitability, by Peacock et al. arxiv.org/abs/2005.01687

Another #SPUV highlight: This question has been on my find for a while. Teal et al. have been testing what uncertainties in stellar UV spectra mean for photochemical models of planetary atmospheres. Can we fudge the UV or not? I hope to find out at the rescheduled SPUV 2021!

Another #SPUV highlight: Fleury et al. are making hot giant planet atmospheres in the lab!

A reminder from Moore & Cowan a la #SPUV that the lower boundary condition to a planetary atmosphere is not as simple as we scientists often like to make it. In short: rocks "breathe."

School of Earth and Space Exploration Team Dynamos' annual retreat at Lowell Observatory, outdoors and social distancing - research intensive *and* therapeutic. It was great to see the team in 3D, again! Including Parke Loyd, Joe Llama, Dr. Tyler Richey-Yowell.

#exo3 Glad Dr. Günther highlighted the link between flares and the habitability of M dwarf planets! Flares can be sneaky. The widely acclaimed "boring" M dwarf GJ 887 looks flare-less in TESS data, but not so in the far ultraviolet! iopscience.iop.org/article/10.384…