TOI-733 b Archives

RV (top panel) and FWHM (bottom panel) time-series. The purple markers in each panel represent the HARPS RV and FWHM measurements with inferred offsets extracted. The inferred multi-GP model is shown as a solid black curve, where the dark and light shaded areas show the 1- and 2- sigma credible intervals from said model, and can also explain the data but with a correspondingly lower probability. The solid red line in the top panel shows the star-only model, while the teal sine curve – the Keplerian for TOI-733 b. In both panels the nominal error bars are in solid purple, and the jitter error bars (σHARPS) are semi-transparent purple. -- astro-ph.EP

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

TOI-733 b – A Planet In The Small-planet Radius Valley Orbiting A Sun-like Star

by Keith CowingApril 17, 2023April 17, 2023

We report the discovery of a hot (Teq ≈ 1055 K) planet in the small planet radius valley transiting the Sun-like star TOI-733, as part of the KESPRINT follow-up program […]

TOI-733 b

TOI-733 b – A Planet In The Small-planet Radius Valley Orbiting A Sun-like Star

Astrobiologist Dale Andersen’s Antarctic Field Report: 6 November 2026: Setting Up Lake Untersee Basecamp

Scott Base: Lessons For A Mars Exploration Program

Pre-Accretion Formation of Sulfuric Acid in Interstellar Ice Analogs: Implications for Sulfate in Ryugu and Bennu

Deep Evolutionary History Of Land Plants’ Closest Algal Relatives

Microbes Can Grow In Mars-like Conditions. What That Means For The Search For Life