Astrobiology95- Page

This picture of Mars is a colorized composite of several images captured by Europa Clipper’s thermal imager. Warm colors represent relatively warm temperatures; red areas are about 32 degrees Fahrenheit

A molecular-size dependent transition in the likelihood of achiral (A) and chiral (C) molecules within chemical space. (A) As heavy atoms are added to molecular graphs in an expanding chemical

Caleb Rosen traveled to Mt. Erebus, Antarctica to collect gas and rock samples. Caleb is in the bottom-left stamp, right figure. — USC Earth Sciences Ph.D. student, Caleb Rosen, traveled

Mars Curiosity rover Credit: NASA/JPL-Caltech/MSSS Over the past decade, the Tunable Laser Spectrometer (TLS) on NASA’s Curiosity rover has reported several detections of methane on Mars, attracting attention due to

This image of Uranus from NIRCam (Near-Infrared Camera) on the NASA/ESA/CSA James Webb Space Telescope shows the planet and its rings in new clarity. The Webb image exquisitely captures Uranus’s

Venus — JAXA Venus, our neighboring planet, is an open-air laboratory that can be used to study why Earth and Venus evolved in such different ways. Noble gases in planetary

Saturn-type ringed planet – Grok via Astrobiology.com Photometric surveys for exoplanetary ring systems have not confirmed any object with Saturn-sized ring. We systematically analyse 308 TESS planet candidates, mainly comprised

Color-contour visualization of density at the disk midplane (the X-Y plane), combined with a vertical slice (the x-z plane), and a cylindrical segment (ϕ coordinate at r = 1) at

Schematic illustration of chemical interaction between an hydrogen-dominated atmosphere and a magma ocean in sub-Neptune with an oxidized FeO-containing magma ocean (left panel) and a reduced FeO-free magma ocean. Note

2018-07-17. Image taken with the Asiago Schmidt telescope with B, g, r filters. Comet Giacobini-Zinner moves fast in a very starrich field in the constellation Cygnus. The dust tail,