Archivo de imágenes de Hubble
Imagen de brújula y escala para SN Refsdal y MACS J1149.6+2223
The powerful gravity of a massive cluster of galaxies in this Hubble Space Telescope image is producing multiple images of a single distant supernova behind it.The foreground cluster is acting like a giant cosmic lens, bending and magnifying light from the exploding star in an ef...
- Fecha
- Jan 1, 2015
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2015-08-3497-image
The powerful gravity of a massive cluster of galaxies in this Hubble Space Telescope image is producing multiple images of a single distant supernova behind it.
The foreground cluster is acting like a giant cosmic lens, bending and magnifying light from the exploding star in an effect called gravitational lensing.
The enlarged inset view reveals four images of the supernova, spotted on Nov. 11, 2014, arranged around a giant elliptical galaxy within the cluster. The light from the supernova passes so closely to the galaxy's dense core that several light paths are redirected and focused toward Earth. The result is that astronomers see four images that form a cross-shaped pattern called an Einstein Cross. The blue streaks wrapping around the galaxy are the stretched images of the supernova's host spiral galaxy, which has been distorted by the warping of space.
Computer models of the cluster predict that another image of the stellar blast will appear within five years. The red circle marks the possible location of the next supernova image. Astronomers may have missed an earlier appearance of the supernova in 1995, as marked by the blue circle. These multiple appearances of the exploding star are due to the various paths its light is taking through the maze of clumpy dark matter in the galactic grouping. Each image takes a different route through the cluster and arrives at a different time, due, in part, to differences in the length of the pathways the light follows to reach Earth.
The elliptical galaxy and its galaxy cluster, MACS J1149.6+2223, are 5 billion light-years away from Earth. The supernova, dubbed Supernova Refsdal, is 9.3 billion light-years away.
This image combines data from three months' worth of observations, taken in visible light by the Advanced Camera for Surveys and in near-infrared light by the Wide Field Camera 3.
Credits
NASA, ESA, and S. Rodney (JHU) and the FrontierSN team; T. Treu (UCLA), P. Kelly (UC Berkeley), and the GLASS team; J. Lotz (STScI) and the Frontier Fields team; M. Postman (STScI) and the CLASH team; and Z. Levay (STScI)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | SN Refsdal, SN HFF14Ref (supernova), MACS J1149.6+2223 (cluster) |
| Object Description | Multiply Imaged, Gravitationally Lensed Supernova and Lensing Galaxy Cluster |
| R.A. Position | 11h 49m 35.08s |
| Dec. Position | 22° 24' 10.94" |
| Constellation | Leo |
| Distance | 9.3 billion light-years or 2.9 billion parsecs (supernova); 5 billion light-years or 1.5 billion parsecs (cluster) |
| About The Data | |
| Data Description | This image is created from data from the following HST proposals: T. Treu (UCLA) et al. and the GLASS team, J. Lotz (STScI) et al. and the Frontier Fields team, S. Rodney (JHU) et al. and the FrontierSN team, and P. Kelly (UCLA) et al. and the Refsdal team. The science team includes: P. Kelly (UC Berkeley), S. Rodney (JHU), T. Treu (UCLA), R. Foley (University of Illinois at Urbana-Champaign), G. Brammer (STScI), K. Schmidt (UC Santa Barbara), A. Zitrin (Caltech), A. Sonnenfeld (UCLA), L.-G. Strolger (Western Kentucky University/STScI), O. Graur (New York University/American Museum of Natural History), A. Filippenko (UC Berkeley), S. Jha (Rutgers University), A. Riess (JHU/STScI), M. Bradac (UC Davis), B. Weiner (Steward Observatory/UA), D. Scolnic (University of Chicago), M. Malkan (UCLA), A. von der Linden (Dark Cosmology Centre, Copenhagen/KIPAC, Stanford), M. Trenti (University of Melbourne), J. Hjorth (Dark Cosmology Centre, Copenhagen), R. Gavazzi (Institut d'Astrophysique de Paris), A. Fontana (INAF-OAR), J. Merten (Caltech), C. McCully and T. Jones (UC Santa Barbara), M. Postman (STScI), A. Dressler (Carnegie Observatories), B. Patel (Rutgers University), S. B. Cenko (NASA/GSFC), M. Graham (UC Berkeley), and B. Tucker (UC Berkeley/Australia National University). |
| Instrument | HST>ACS/WFC and HST>WFC3/IR |
| Exposure Dates | November 3, 2014 - December 14, 2014 |
| Filters | ACS/WFC: F606W and F814W WFC3/IR: F105W, F125W, F140W, and F160W |
| About The Image | |
| Color Info | These images are composites of separate exposures acquired by the ACS and WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F606W+F814W Green: F105W+F125W Red: F140W+F160W |
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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
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