Results of the pRT retrievals for the atmosphere of HD 86226 c. Left: PACMAN spectrum (black data) and 1, 2, and 3σ percentiles of the spectra from the posteriors of
Synthetic atmospheric transmission spectra of Ross 176 b. Left: Fiducial models for clear or hazy H/He atmospheres with scaled solar abundances. Right: Model for a steam H2O atmosphere. Simulated measurements
Transit spectra of the best fit non-equilibrium 1D model at resolution 200 (black solid line). This is the approximate best fit on the simulated grid of metallicity, C/O and Kzz.
Keith Cowing Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻 Follow on
Astrobiology Spectral Database Wednesday, July 23rd from 10AM – 4PM CT Are you interested in organics for the origin of life, returned samples, life detection, or machine learning? Do you
Graphical Abstract — chemrxiv.org We present a physicochemical framework for understanding the emergence of catalytic logic at the origin of life. In this view, early catalytic systems did not depend
6300.304 ˚A line from 6296.5-6305.8 ˚A, and the 6363.776 ˚A line from 6361.2-6365.7 ˚A Enhanced red-doublet maps, from 15 May 2021 to 09 March 2022. Red
Ongoing research explores potential for Jupiter’s frozen moon to support life, habitability Courtesy: NASA/JPL-Caltech/DLR Southwest Research Institute experiments offer a new view on a hydrogen peroxide chemical cycle on Europa.
The image to the left, taken with ESO’s Very Large Telescope (VLT), shows a possible planet being born around the young star HD 135344B. This star, located around 440 light-years
A: Bioreactor setup of A. manzaensis grown on ESAE-01 basalt analog material. B: Exposure wells with desiccated A. manzaensis cells and ESAE-01 basalt pellets. C: Successful recultivation of A. manzaensis
