Astrobiology225- Page

Comparison between the database EHS masses with recomputed values adopting the database stellar radii and surface gravities (see text for details). The grey dotted line is the (1:1)-relation. If the

Carbon-I (a) optical ray trace and (b) the proposed structural design. — physics.optics The proposed Carbon Investigation (Carbon-I) Imaging Spectrometer is designed to measure variations of greenhouse gases in Earth’s

Estimated total mass of transiting compact systems, Mtot, scaled to the stellar mass, M∗. a, (Mtot/M∗) for compact systems having ≥ 3 known planets that orbit a single star within

Total O3 abundances for models with high N2O (left) and low N2O (right) normalized to models with modern levels of N2O from Kozakis et al. (2022). Overall the high N2O

Examples of spectral synthesis used in this work. The black dots are the observed spectra and the red lines are the theoretical spectra. From right to left, the gray areas

Artist’s view of the Kepler-725 system. The small planet in the lower right is the newly discovered super-Earth in the habitable zone. (Image by GU Shenghong) “Are we alone?” This

Maps showing Callisto’s bolometric albedo (a; from Camarca et al. 2023) compared with the spectral slope from 360 to 410 nm (b), which measures the strength of the near-UV downturn

Left panel: simulated, noise-free spectra of water ice (dashed dark-blue curve) and selected trace species of interest. Middle panel: simulated spectra of non-water-ice species mixed with water ice, at an

Flowchart of the experimental design. The DNA was extracted from C. antarcticus colonies and divided into two 1.5 mL Eppendorf tubes, one containing a Martian regolith analogue and the other

The Pacific Ocean As Seen From Space — NASA Call for Applicants The NASA Astrobiology Program is hosting a Mission Ideation Factory focused on the search for life on Ocean