THERMAL PHASE VARIATIONS OF WASP-12b: DEFYING PREDICTIONS
We report Warm Spitzer full-orbit phase observations of WASP-12b at 3.6 and 4.5 μm. This extremely inflated hot Jupiter is thought to be overflowing its Roche lobe, undergoing mass loss and accretion onto its host star, and has been claimed to have a C/O ratio in excess of unity. We are able to meas...
Những tác giả chính: | Cowan, Nicolas B., Machalek, Pavel, Shekhtman, Louis M., Burrows, Adam, Deming, Drake, Greene, Tom, Hora, Joseph L., Croll, Bryce J. |
---|---|
Tác giả khác: | Massachusetts Institute of Technology. Department of Physics |
Định dạng: | Bài viết |
Ngôn ngữ: | en_US |
Được phát hành: |
IOP Publishing
2015
|
Truy cập trực tuyến: | http://hdl.handle.net/1721.1/95620 |
Những quyển sách tương tự
-
The Apparently Decaying Orbit of WASP-12b
Bằng: Patra, Kishore C., et al.
Được phát hành: (2017) -
SECONDARY ECLIPSE PHOTOMETRY OF THE EXOPLANET WASP-5b WITH WARM SPITZER
Bằng: Baskin, Nathaniel J., et al.
Được phát hành: (2015) -
Mass Loss from the Exoplanet WASP-12b Inferred from Spitzer Phase Curves
Bằng: Bell, Taylor J, et al.
Được phát hành: (2021) -
Mass Loss from the Exoplanet WASP-12b Inferred from Spitzer Phase Curves
Bằng: Bell, Taylor J, et al.
Được phát hành: (2022) -
DAY-SIDE z ′-BAND EMISSION AND ECCENTRICITY OF WASP-12b
Bằng: Lopez-Morales, Mercedes, et al.
Được phát hành: (2015)