Astrobiology10- Page

A self-portrait of NASA’s Curiosity rover taken on June 15, 2018, when a Martian dust storm had reduced sunlight and visibility at the rover’s location in Gale Crater. NASA/JPL-Caltech/MSSS In

James Webb Space Telescope Near-infrared Camera (JWST NIRCam) false colour image of IRAS07251-0248, made by combining exposures with the 2 mm (Blue), 2.77 mm (Green) and 3.56 mm (Red) wide

Left panel: Map of the normalized XUV flux in the habitable zone, FXUV,HZ/FHZ, in the Galactic R-Z plane. Right panel: Map of the normalized XUV flux in the habitable zone,

Photos of tested material surfaces and their corresponding three-dimensional (3D) topography. Z-axis labels represent the surface height range. Some 3D scan lengths were limited to 100 µm due to data

NASA’s Mars rover Curiosity acquired this image using its Mast Camera (Mastcam); it shows the “Nevado Sajama” drill site from November, right next to the location of this weekend’s drill.

A planet with a magma ocean — Grok via Astrobiology.com Sub-Neptunes with hydrogen-rich envelopes are expected to sustain long-lived magma oceans that continuously exchange volatiles with their overlying atmospheres. Capturing

Infrared spectrum of Ser-emb7 after continuum removal and peak fitting. The original spectrum (dark gray) is fit with color-coded peaks, which are identified in the legend, that sum to an

Comparison of host star masses and metallicities of N ≥3 categories of exoplanet systems (black points), compared with two of our potential source populations: all exoplanet hosts with jupiters (red)

Transmission spectra of solid methanol and its five deuterated isotopologues at 10 K. The region between 650 to 590 cm−1 (15.4 to 16.9 µm), affected by increased noise from the