Schematic image of three types of protoplanetary systems and their contribution to the radius-eccentricity profile and radius valley. — astro-ph.EP While recent planet-formation models broadly reproduce the observed population of

Distribution of our found planets in period–radius space (left) and instellation–radius space (right). Each planet and its associated errors are are marked with the red points, while the background grid

The Vera C. Rubin Observatory sits on its mountain peak in Chile during observation activities in April 2025. The observatory will soon begin real-time nightly monitoring of the entire Southern

Effect of mec-4 mutations on neuromuscular aging and muscular calcium transients in a terrestrial 1G environment. (A) Heatmap analysis of log2(FC) ratio of autophagy/aggrephagy genes between D01 wild type and

ID: ESP_072042_1330, date: 8 December 2021,altitude: 251 km larger image NASA/JPL-Caltech/University of Arizona The dark sand dune at the center of this observation is covered in a blanket of white

Exoplanets, -moons, -comets Status Report astro-ph.EP) March 2, 2026 Schematic diagram for classifying planets according to their masses and orbital periods. The various categories of planets are labelled. The boundary

Two-dimensional wireframe representation of the atmospheric geometry implemented in the Geant4 simulations. The model consists of four concentric spherical layers corresponding to the altitude ranges 15–20 km, 20–25 km, 25–30