The Hottest Neptunes Orbit Metal-rich Stars
The Neptune desert is no longer empty. A handful of close-in planets with masses between those of Neptune and Saturn have now been discovered, and their puzzling properties have inspired a number of interesting theories on the formation and evolution of desert-dwellers. While some studies suggest th...
Saved in:
Main Authors: | Shreyas Vissapragada, Aida Behmard |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astronomical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-3881/ada143 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Formation of Super-Earths and Mini-Neptunes from Rings of Planetesimals
by: Sho Shibata, et al.
Published: (2025-01-01) -
The Reception of Neptune’s Discovery in British and American Protestant Theology
by: Zenon Roskal, et al.
Published: (2024-09-01) -
The Influence of General Relativity on the Spins of Celestial Bodies in Inclined Orbits
by: Huan-Rong Yuan, et al.
Published: (2025-01-01) -
Gaia-4b and 5b: Radial Velocity Confirmation of Gaia Astrometric Orbital Solutions Reveal a Massive Planet and a Brown Dwarf Orbiting Low-mass Stars
by: Gudmundur Stefánsson, et al.
Published: (2025-01-01) -
Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-hydrodynamic Code
by: Riley Rosener, et al.
Published: (2025-01-01)