Archivo de imágenes de Hubble
Mapa de temperatura global de WASP-43b
This is a temperature map of exoplanet WASP-43b. The gas giant planet orbits very close to its parent star with a period of 19.5 hours. Because the planet keeps one side facing its star, there are huge temperature extremes between the day and night sides. The white-colored region...
- Fecha
- Jan 1, 2014
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2014-28-3382-image
This is a temperature map of exoplanet WASP-43b. The gas giant planet orbits very close to its parent star with a period of 19.5 hours. Because the planet keeps one side facing its star, there are huge temperature extremes between the day and night sides. The white-colored region on the daytime side is 2,800 degrees Fahrenheit. The nighttime-side temperatures drop below 1,000 degrees Fahrenheit. This steep gradient is in stark contrast to the predominantly uniform temperatures of the solar system's giant planets. Infrared observations with the Hubble Space Telescope measured how temperatures change with both altitude and longitude on the planet.
Credits
NASA, ESA, and K. Stevenson, L. Kreidberg, and J. Bean (University of Chicago)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | WASP-43b |
| Object Description | Extrasolar Planet |
| R.A. Position | 10h 19m 38s.01 |
| Dec. Position | -09° 48' 22".61 |
| Constellation | Sextans |
| Distance | 260 light-years (80 parsecs) |
| About The Data | |
| Data Description | The image was created from Hubble data from the following proposal: PI: J. Bean (University of Chicago) et al. Members of the science team include: K. Stevenson (University of Chicago), J.-M. Désert (CASA/University of Colorado), M. Line (University of California, Santa Cruz), J. Bean (University of Chicago), J. Fortney (University of California, Santa Cruz), A. Showman and T. Kataria (University of Arizona), L. Kreidberg (University of Chicago), P.R. McCullough (STScI/JHU), G. Henry (Tennessee State University), D. Charbonneau (Harvard University), A. Burrows (Princeton University), S. Seager (MIT), N. Madhusudhan (University of Cambridge, UK), M. Williamson (Tennessee State University), and D. Homeier (CNRS/University of Lyons). |
| Instrument | HST>WFC3/IR |
| Exposure Dates | November - December, 2013 |
| Filters | Grating: G141 |
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La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.
Ver en NASA.gov