Astrobiology75- Page

Field of view for WASP-135 b (image scale in arcsec/pix: 0.299772). Example image from 09 May 2024, with the target star, WASP-135, and the comparison star labeled in green and

NASA’s Mars 2020 Rover’s SHERLOC Instrument, located at the end of the robotic arm on NASA’s Mars 2020 rover. SHERLOC (short for Scanning Habitable Environments with Raman & Luminescence for

a) Illustration of a firefly flash sequence and a pulsar pulse sequence, which serves as the basis of the model discussed in this paper. b) Conceptualization of how the model

Model spectra (top) and Kp-voffset maps for the combination of all nights (bottom) of H2O, H2S, and CH4 for KELT-11 b. The grey shaded areas show the wavelength regions of

Left panel: Multiple observations of proper motion of Sirius B from 1980 to 2022. From Earth, the separation between Sirius A and B varies between 3 and 11 arcsec on

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

The new study constrained the Enceladus’ global conductive heat flow by studying its seasonal temperature variations at its north pole (yellow). These results, when combined with existing ones of its

Kaiser Crater hosts a large field of sand dunes. Every winter the dunes are covered with a layer of seasonal carbon dioxide ice (dry ice). In early spring the ice

The visual representation of the parameters used for modelling the SN II explosion. The progenitor system (top) can evolve into two distinct end states (bottom): the planet-moon system can stay

Upper: TESS TPF (Target Pixel Files) of Sector 17 for TOI-1472, and Sector 25 for TOI-1648. The color scale represents electron counts per pixel. Orange squares mark the pixels selected