Astrobiology8- Page

Molecular composition of haze samples from the N2-rich/CH4 and H2O-rich/CH4 experiments. Left panels: Very high-resolution mass spectra (m/z 150–800) of haze particles produced from the N2-rich/CH4 and H2O-rich/CH4 experiments, acquired

ID: ESP_049028_2065 date: 10 January 2017 altitude: 287 km NASA/JPL-Caltech/University of Arizona Larger image The material on the floor of this crater appears to have flowed like ice, and contains

Raman images showing the distribution of OM (red) and titanite (Ttn, purple) inside spheroids immediately adjacent to apatite (Ap, turquoise) and lepidocrocite (Lpc, white) embedded in the basaltic glass fragment

Sky plot of nine cPIC targets that are present in all stellar reference samples. Their PIC names are indicated with labels. — astro-ph.IM A few weeks after launch, the PLATO

A summary of the CO and N2 reported in various comets with respect to parent molecule (top) and with respect to water (bottom). The CO/CO2 ratios are reported by O.

Terrain corrected DGPR profile at Galena Creek Rock Glacier. Location of the profile is shown in Fig. 3A. Uninterpreted data (top) and interpreted internal debris layers (bottom), with detected and

Artist’s conception of the gas giant planet TOI-5205 b orbiting a small, cool red dwarf star. Image courtesy of Katherine Cain, Carnegie Science. Massive exoplanet reveals new insights into the

Period-radius plot for planets in single-star (gray points) and binary-star (colored points) systems considered in this work. Colors correspond to log10(ρ), i.e. the projected physical binary separation in au. We