Archivo de imágenes de Hubble
Nubes en la atmósfera del exoplaneta GJ 1214b (vista del artista)
This is an illustration of the hypothetical appearance of the exoplanet GJ 1214b, which is known as a "super-Earth" type planet because it is slightly more than six Earth masses. Spectroscopic observations with NASA's Hubble Space Telescope provide evidence of high clouds blanket...
- Fecha
- Jan 1, 2014
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2014-06-3303-image
This is an illustration of the hypothetical appearance of the exoplanet GJ 1214b, which is known as a "super-Earth" type planet because it is slightly more than six Earth masses. Spectroscopic observations with NASA's Hubble Space Telescope provide evidence of high clouds blanketing the planet. These clouds hide any information about the composition and behavior of the world's lower atmosphere and surface. The composition of the clouds is unknown. GJ1214b is located 40 light-years from Earth, in the constellation Ophiuchus.
Credits
Artwork: NASA, ESA, and G. Bacon (STScI);Science: NASA, ESA, L. Kreidberg and J. Bean (University of Chicago), and H. Knutson (California Institute of Technology)
Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | GJ 1214b |
| Object Description | Extrasolar Planet |
| R.A. Position | 17h 15m 18.93s |
| Dec. Position | 04° 57' 49.71" |
| Constellation | Ophiuchus |
| Distance | 40 light-years (12.3 parsecs) |
| About The Data | |
| Data Description | The Hubble data are from proposal : J. Bean (University of Chicago), J.-M. Desert (California Institute of Technology), S. Seager (Massachusetts Institute of Technology), D. Deming (University of Maryland), B. Benneke (Massachusetts Institute of Technology), Z. Berta-Thompson (Harvard University), K. Stevenson (University of Chicago), and D. Homeier (Lyon Centre for Astrophysics Research). The science team includes: L. Kreidberg and J. Bean (University of Chicago), J.-M. Desert (California Institute of Technology), B. Benneke (Massachusetts Institute of Technology), D. Deming (University of Maryland), K. Stevenson (University of Chicago), S. Seager (Massachusetts Institute of Technology), Z. Berta-Thompson (Harvard University), A. Seifahrt (University of Chicago), and D. Homeier (Lyon Centre for Astrophysics Research). |
| Instrument | HST>WFC3 |
| Exposure Dates | September 27, 2012 - August 4, 2013 |
| Filters | Grim: G141 |
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Fuente
La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.
Ver en NASA.gov