Selected wavelength region of a GIANO-B spectrum where many CO2 absorption lines are found. The original spectrum (orange line) is composed both by the telluric and the Martian CO2 lines,
(A) Spectral variation of the benzene:CO mixture before and after photon exposure. The dark blue line corresponds to the IR spectra before photon exposure, and the lighter blue corresponds to
Line profiles of ionized emission from the outflow in the nuclear region of W2246- 0526, marked with a red circle in the inserted figure showing the extended Hα emission in
Image gallery of all HST observations of IRAS23077. The top row shows images taken with the WFC3/UVIS filters F438W, F606W, and F814W, while the bottom row shows images taken with
Phase folded transits of TOI-2345 b (purple) and TOI-2345 c (green) with the best-fit model from the joint fit in juliet in the top panel. The bottom panel shows the
This artist’s impression shows the evolution of heavy water molecules (H2O, HDO, and D2O) as they have been observed in giant molecular clouds, a planet forming-disk, and comets—before they eventually
Lava-covered proto-Earth – Grok via Astrobiology.com Scientists at MIT and elsewhere have discovered extremely rare remnants of “proto Earth,” which formed about 4.5 billion years ago, before a colossal collision
Enhanced view of Enceladus’ South pole region showing the locations of organic-rich geysers in blue Saturn’s moon Enceladus is an exciting destination for future exploration missions due to
Latitude-longitude maps of surface temperature overlaid with the wind field at the bottom layer, and surface precipitation. The black contours indicate where the surface temperature is 50◦ Celsius.
Snapshots of VGS-calculated surface water mass (in units of Earth’s ocean mass) for TRAPPIST-1 analogs, shown as a function of total planet mass (M⊕) and final orbital distance (AU). Panel
