The GAPS programme at TNG: XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422
Context. Neptunes represent one of the main types of exoplanets and have chemical-physical characteristics halfway between rocky and gas giant planets. Therefore, their characterization is important for understanding and constraining both the formation mechanisms and the evolution patterns of plan...
Main Author: | Seager, Sara |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2023
|
Online Access: | https://hdl.handle.net/1721.1/148404 |
Similar Items
-
TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star
by: Seager, Sara
Published: (2023) -
TOI-220 b: a warm sub-Neptune discovered by TESS
by: Seager, Sara, et al.
Published: (2022) -
The TOI-763 system: sub-Neptunes orbiting a Sun-like star
Published: (2021) -
The TOI-763 system: sub-Neptunes orbiting a Sun-like star
Published: (2022) -
A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
by: Seager, Sara
Published: (2023)