Astrobiology226- Page

3D structure of CH2CCN with spin density distribution, generated with Avogadro 1.2.0.90 The spin density is visualized using an isosurface of value 0.02 (in au). — astro-ph.GA Cyanopolyynes, a family

M-a distribution, updated from Figure from Kempton and Knutson (2024). The solid-colored points have atmospheric spectra as of April 28, 2025 and the transparent points do not. The additional data

The HOMO of the charged ASW cluster (a), only showing the closest interacting water molecules for clarity. (b) Shows the LUMO of a neutral water molecule. — astro-ph.GA The interstellar

Recurring slope lineae on Mars’s surface. (a) RSL at a crater on the floor of Valles Marineris, near the Martian equator, captured by the HiRISE (High Resolution Imaging Science Experiment).

Summary plots for observations of TOI3124 (a) and TOI3163 (b). The TESS Sector 64 TPF, normalized light curves and periodogram plots are shown for each target. Cutouts of the stacked

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

“Strange New World” – Star Trek Enterprise episode 104 – Enterprise passes a previously unknown Minshara-class (M-class) planet with an Earth-like atmosphere and surface. – Paramount/CBS Our paper fills this

This is the ‘beauty shot version’ of Perpetual Ocean 2: Western Boundary Currents. The visualization starts with a rotating globe showing ocean currents. The camera then zooms into the Kuroshio

Optical microscopy image of the clastic matrix region in LAR 12252 that was studied using S-XANES. Notable phases include enstatite (examples outlined in red), sulphides (example outlined in yellow), a

HWO Science Case Portal The HWO Science Working Groups are excited to share draft science cases that will help shape the top-level science goals, instrument needs, and mission architecture for