Astrobiology48- Page

Mars craterfill deposits showing varying intensities and topographies (cross sections). Crater locations are shown in Figure 2A. (A) Thin and laterally restricted fill with deposits concentrated in the southwestern region

Radius evolution for a metal-enriched planet (Z=0.1) as computed with our approach (square points) versus the planetsynth models of M¨uller & Helled (2021) (solid curves; note that they employ a

Schematic showing the reset approach applied for the close-in four-planet system. The left graphic shows “exaggerated” orbits of the four planets after the encounter when they are on slightly eccentric,

Scatter plot of Laromatic/LIR as a function of LIR for the AGNdominated (red circles) and AGN-SF-composite galaxies (red triangles). The gray circles show the relationship for the SFG sample. —

Simulated PRIMA/FIRESS spectrum of the PAH emission based on the model spectrum for a galaxy with log(LIR/L⊙)= 13.6 in Fig.7(b) for selective redshifts (z = 3, 5, 7, 10). In

Retrieval results on the full spectrum for three difference MIRI pixel shifts. The top panel shows the transit spectrum with the median retrieved spectral model and representative 1σ and 2σ

Fluidic Telescopes – We present a conceptual framework for optically designing space-assembled telescopes whose primary mirror is formed in situ via the enabling, scale-invariant technology of fluidic shaping. — astro-ph.IM

Mapped CBs (channel belts) outlined in black and the putative shorelines in blue. Yellow outlines indicate avulsed CB paths. The backwater/belt-width window for each CB is shown in orange. Avulsion