Astrobiology19- Page

Portion of the spectra of ortho- (top), meta- (middle), and para- (bottom) deuterated benzonitrile (DBCN) recorded in the 75- 110 GHz range. The experimental spectra are shown in black above

Conceptual diagram of the theory of multi-spheric interaction-driven hydrocarbon formation and enrichment. Credit ©Science China Press The multi-spheric structure of the Earth forms its skeleton, and the geological molten fluids

Genesis Solar Wind Sample Collection After careful consideration and thorough evaluation of our current work priorities, resources, and budget constraints, we have decided to transition the Genesis collection from an

Towards the Habitable Worlds Observatory Description We are pleased to announce the inaugural open community event for NASA’s Habitable Worlds Observatory, to be held at the Johns Hopkins Bloomberg Center

Extraterrestrial Materials Analysis Group (ExMAG) The Extraterrestrial Materials Analysis Group (ExMAG) meeting is scheduled for September 15–19, 2025, at the Lunar and Planetary Institute (LPI) in Houston, Texas. The Second

The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window. Hasenstein KH, Moinuddin SGA, Berim A, Davin LB, Lewis NG.Glucosinolate

Earth biosignatures through time and their reflected light spectra. The left subplot shows estimates of Earth’s bulk atmospheric composition through time (advancing from top to bottom), and the figures on

The black line shows the IRTF/SpeX spectrum of 3I/ATLAS, normalized at 1.2 µm. Colored lines and shaded regions represent the mean and ±σ ranges for S-type (blue), D-type (red), and

Left: Planet-to-star mass ratio as a function of the planet semi-major axis for all planets orbiting M-dwarf stars. Darker coloured symbols correspond to planetary masses above 0.2 MJup. Horizontal dotted