Astrobiology6- Page

Top Panel: Absorption cross sections for a temperature of 650K and pressure of 1 bar used in the retrieval analysis from Hood et al. (2024). Bottom Panel: The complete SED

GJ 357 b NIRISS white light curve fit results. Top panel: Raw GJ 357 b order 1 white light curve, with the best-fitting astrophysical transit + systematics model overplotted in

Magnification of Rhinocladiella Simili cells in PDB culture medium, showing pseudohypha behavior –NPJ Microgravity via PubMed Studying the survival of terrestrial microorganisms under Martian conditions, particularly in the presence of

Planning diagram showing variation in latitude range (between heavy black lines) vs. season (solar longitude, LS) for SHARAD standard VLR observations wherein all associated spacecraft maneuvers occur when the MRO

Distribution of simulated EEC yield (solid contours) and underlying planet population (dotted contours) around FGK-type stars within 20 pc. We show the planetary radius over incident flux distribution, where the

χ2 maps for the CS RT models. The free parameters f0 and Re are on the x− and y−axes, respectively. The red + sign denotes the best-fit model, and the

MUSE and NIRCam images of d203-504 environment. Left: MUSE NFM composite image of both d203-506 (bottom left) and d203-504 (top). Red: the (λ8727˚A) map showing disk contributions from both

By delving into ancient rock records, scientists have uncovered new clues that sharpen the timeline of Earth’s oxygenation—shedding fresh light on one of the most transformative chapters in our planet’s

Taken on 28 May 2025, this image of the preparative zone of cultured tobacco cells with visualized microtubules (yellow: microtubules , magenta: nuclei). For the Effects of the Space

Numerical simulations of lava planets interior dynamics with no rotation. The dimensionless temperature scale is the maximum super-adiabatic temperature contrast: temperature is 1 at the base of the magma ocean,