Periods and mass ratios for planets detected using different methods. Data points show all exoplanets catalogued on 30 July 2023 (41) and are color-coded by detection method (see legend). The

Schematic of topography on an icy satellite. Equations shown for the evolution of Newtonian viscous ice with shell thickness H. The parameters and equations shown on the figure are described

Val Finlayson (left) and Paulo Galvan recovering rock samples from a dredge from a 2013 expedition. Credit: Val Finlayson. Geologists led by the University of Maryland and the University of

Harvesting Lettuce at Kennedy Space Center Space Systems Processing Facility Image credit: NASA/Kim Shiflett Inside a laboratory in the Space Systems Processing Facility at NASA’s Kennedy Space Center in Florida,

MK0 − Teff plane (upper left left) and Gaia photometry color-magnitude diagram (upper right, bottom left and bottom right) for stars in APOGEE DR17. The local sample of dwarfs is

The retrieved spectra using the hybrid equilibrium chemistry model and machine learning approaches are shown. Observations from JWST instruments are illustrated with different colored error bars: green for NIRISS, blue

Exoplanetology: Exoplanets & Exomoons Status Report astro-ph.EP May 2, 2025 The frequency of quality flagged cadences as they occur in year 1 light curves. The most commonly occurring quality flags

Dust temperature (colorscale) and N(H2) column density (contours: 1, 2, 3, 4, 5, 6, 7, and 8 × 1022 cm−2 ) Herschel maps of NGC1333 region in Perseus (Pezzuto et