Kepler-62 e Archives

PANEL (A): Diagram of the net tidal accelerations acting on the planetary surface (caused by the host star’s gravity field). The planet is represented with a top view (i.e., as seen from above). Accelerations are computed in the reference frame of the planetary center. PANEL (B): Representation of the tidal bulge. The planet is represented with a top view. Planetary spinning (black arrow) is counterclockwise, as is the orbital motion around the star (red arrow). -- astro-ph.EP

Astronomy & Telescopes, Atmospheres, Climate, Weather, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Status Report

Simulation Of The Spin Evolution Of Some Selected Exoplanets And Inferences On Their Climate

by Keith CowingMay 20, 2026May 20, 2026

In this work, using the simulator VPLanet, we analyze the spin evolution of some selected exoplanets due to the tidal interaction with their host star.

Kepler-62 e

Simulation Of The Spin Evolution Of Some Selected Exoplanets And Inferences On Their Climate

A Search For Narrowband Technosignatures From LTT 3780 With The Allen Telescope Array And The Karl G. Jansky Very Large Array

Tricorder Tech: Identifying Proteins, Molecule By Molecule

First Completed Rocky Worlds Program Observations Open New Era in Exoplanet Studies

Pioneer 10/11 Telemetry Explanatory Almanac

Diverse Organic Molecules Discovered Surrounding A Newly Formed Star