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NASA SMD – Research and Development of Initiatives of Advanced New Technologies (RADIANT) B.5 Research and Development of Initiatives of Advanced New Technologies (RADIANT) seeks innovative adaptations and applications of

The ≈1000 au environment of RW Aur at different wavelengths, as observed by ALMA and JWST. Panel (a): compact dust continuum emission at 1.3 mm wavelength (see Kurtovic et al.

Evidence for recent LGT and non-homologous recombination of an organophosphate transporter operon phnCDEubiE between HIMB59 and Pelagibacter. (A) Presence of phnCDEubiE genes in only one of the two Pelagibacter genomes

An SwRI-led team used Webb telescope observations (white) to detect methane gas on the distant dwarf planet Makemake. Sharp emission peaks near 3.3 microns reveal methane in the gas phase

Dust clouds reflect starlight around the star R Doradus. As it nears the end of its life, the star is shedding its outer layers, forming clouds of gas and dust

Detection maps of β Pic b with MATISSE. The maps show the reduced χ2 values after fitting the stellar contamination for each tested planet astrometry (∆α, ∆δ) in the grid.

Illustration of the soot line and water ice line structure of protoplanetary disks, and the three chemically distinct planet archetypes. — astro-ph.EP Some low-density exoplanets are thought to be water-rich