The Transmission Spectrum of the Planet WASP-32 b
Abstract
The transmission spectrum of the exoplanet WASP-32 b, obtained from observations on the 10-m GTC telescope, is presented. Based on the results of spectrum analysis, evidence was found for the presence of Na and K chemical elements in the shell around the planet. The presence of hydrogen H I is also possible. Analysis of the height scale shows that the detected elements are significantly higher than exoplanet's atmospheric layers.
- Publication:
-
Physics of Magnetic Stars
- Pub Date:
- July 2019
- Bibcode:
- 2019ASPC..518..225V