Abstract
We present a secondary eclipse observation for the hot Jupiter HD
189733b across the wavelength range 290-570 nm made using the Space
Telescope Imaging Spectrograph on the Hubble Space Telescope. We measure
geometric albedos of Ag = 0.40 ± 0.12 across 290-450
nm and Ag <0.12 across 450-570 nm at 1σ confidence.
The albedo decrease toward longer wavelengths is also apparent when
using six wavelength bins over the same wavelength range. This can be
interpreted as evidence for optically thick reflective clouds on the
dayside hemisphere with sodium absorption suppressing the scattered
light signal beyond ~450 nm. Our best-fit albedo values imply that HD
189733b would appear a deep blue color at visible wavelengths.
Original language | English |
---|---|
Journal | The Astrophysical Journal Letters |
Volume | 772 |
Issue number | 2 |
DOIs | |
Publication status | Published - 01 Aug 2013 |
Externally published | Yes |
Keywords
- planets and satellites: atmospheres
- stars: individual: HD 189733
- techniques: photometric