Astrobiology113- Page

Target pixel file from the TESS observation of Sector 54 and Sector 55, centered respectively on TOI-5800 (top panel) and TOI-5817 (bottom panel). The SPOC pipeline aperture is shown by

Prot as a function of Porb for the 88 non-transiting-exoplanet candidate systems. The size of the dots is a function of the Kepler apparent magnitude of the host star, sourced

Left: Image of the Sun with Earth superimposed on the same scale. Upper-right: Radial-velocity time-series of the Sun (green points), obtained with the HARPS-N solar telescope (Dumusque et al., 2021),

Image of a portion of M51; RGB=F1800W/F1130W/F560W (18µm, 11.3µm, 5.6µm). Areas where we have obtained complete 1 − 28µm spectroscopy are indicated. Expanded cutouts are Brα (4.05µm) images of these

Exoplanets with masses error and radii error less than 25%. Symbol size is proportional to mass. Colors correspond to equilibrium temperatures calculated with bond albedos of 0.3 and redistribution factors

A cryo-electron microscopy (cryo-EM) structure of Photosystem I isolated from the bacterium Anthocerotibacter panamensis. — Credit Han-Wei Jiang et al./PNAS. An international team of scientists have unlocked a key piece

A simplified (HhH)2-Fold protein binding to natural and mirror-image dsDNA. The binding surface between the two binding modes is partially overlapping — Credit Liam M. Longo A new study led

A team of researchers led by Niccolò Maffezzoli, “Marie Curie” fellow at Ca’ Foscari University of Venice and the University of California, Irvine, and an associate member of the Institute

ALMA-images of the Milky Way’s Central Molecular Zone. The research team suspects that protoplanetary discs are forming in its clouds. Credit Fengwei XU (PKU); ALMA Partnership; Laura Pérez (NRAO) For