A Lack of Variability Between Repeated Spitzer Phase Curves of the Hot Jupiter WASP-43b
Abstract
We present empirical constraints on atmospheric variability in a hot Jupiter, enabled by three repeated phase curve observations of WASP-43b. We place upper limits on WASP-43b's phase curve varability, and constrain how much WASP-43b's clouds vary.
- Publication:
-
Exoplanets in Our Backyard 2
- Pub Date:
- November 2022
- Bibcode:
- 2022LPICo2687.3039M