Hundreds of TESS Exoplanets Might Be Larger than We Thought
The radius of a planet is a fundamental parameter that probes its composition and habitability. Precise radius measurements are typically derived from the fraction of starlight blocked when a planet transits its host star. The wide-field Transiting Exoplanet Survey Satellite (TESS) has discovered hu...
Saved in:
Main Authors: | Te Han, Paul Robertson, Timothy D. Brandt, Shubham Kanodia, Caleb Cañas, Avi Shporer, George Ricker, Corey Beard |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/ade794 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Oxidation of the Interiors of Carbide Exoplanets
by: H. W. Horn, et al.
Published: (2020-01-01) -
Characterizing Exoplanets for Assessing Their Potential Habitability
by: J. M. Rodríguez-Mozos, et al.
Published: (2025-01-01) -
Exoplanet Atmospheric Refraction Effects in the Kepler Sample
by: Déreck-Alexandre Lizotte, et al.
Published: (2025-01-01) -
Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. VI. Confirmation of a Long-period Giant Planet Discovered with a Single TESS Transit
by: Zahra Essack, et al.
Published: (2025-01-01) -
Hunting for Cold Exoplanets via Microlensing
by: Beaulieu, Jean-Philippe
Published: (2023-08-01)