TOI-1386 Archives

The attributes of planet TOI-1386 b (Panels A–D) and star TOI-1386 (Panels E & F) compared to the population of sub-Saturn planets. TOI-1386 b’s position is indicated by the cross. Planets with a measured mass between 6 – 60 M⊕ are included in our sub-Saturn population. The colorbar for each plot indicates the TSM value of the planet, with TOI-1386 b having a TSM of 42.5. Compared to the rest of the sub-Saturn population, TOI-1386 b is a massive, cool, moderately eccentric planet orbiting a metal rich sun-like star. -- astro-ph.EP

The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog

by Keith CowingFebruary 7, 2024February 7, 2024

The Transiting Exoplanet Survey Satellite (TESS) continues to dramatically increase the number of known transiting exoplanets, and is optimal for monitoring bright stars amenable to radial velocity (RV) and atmospheric […]

TOI-1386

The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog

Survival and Detectability of Mars-Derived Organic Carbon in Phobos Regolith: A Quantitative Hardness Taxonomy for MMX Sample Analysis

Lava World Recon: Juno Studies Io’s Volcanoes

New Exomoon Detection Challenges Cosmic Labels

Discrimination of Tectonic, Swarm And Impact-related Marsquakes Using Spectral Characteristics

Mapping Alien Continents: Achieving Optical VLBI For Exoplanet Imaging