stsci_2010-01c January 5th, 2010
Credit: NASA, ESA, R. Windhorst, S. Cohen, M. Mechtley, and M. Rutkowski (Arizona State University, Tempe), R. O'Connell (University of Virginia), P. McCarthy (Carnegie Observatories), N. Hathi (University of California, Riverside), R. Ryan (University of California, Davis), H. Yan (Ohio State University), and A. Koekemoer (Space Telescope Science Institute)
NASA's Hubble Space Telescope has imaged a portion of the southern field of a large galaxy census called the Great Observatories Origins Deep Survey (GOODS), a deep-sky study by several observatories to trace the formation and evolution of galaxies. The image shows a rich tapestry of galaxies stretching back through most of the universe's history. The galaxies range from the mature spirals and ellipticals in the foreground, to smaller, fainter, irregularly shaped galaxies, most of which are farther away, and therefore existed farther back in time. These smaller galaxies are considered the building blocks of the larger galaxies we see today. The closest galaxies seen in the foreground emitted their observed light about a billion years ago. The farthest galaxies, a few of the very faint red specks, are seen as they appeared more than 13 billion years ago, or roughly 650 million years after the Big Bang.
Provider: Space Telescope Science Institute
Image Source: https://hubblesite.org/contents/news-releases/2010/news-2010-01
Curator: STScI, Baltimore, MD, USA
Image Use Policy: http://hubblesite.org/copyright/
Telescope | Spectral Band | Wavelength | |
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Hubble (WFC3) | Infrared (I) | 98.0 nm |
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Hubble (WFC3) | Infrared (I) | 98.0 nm |
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Hubble (WFC3) | Infrared (J) | 125.0 nm |
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Hubble (WFC3) | Infrared (H) | 160.0 nm |
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Hubble (WFC3) | Optical (U) | 225.0 nm |
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Hubble (WFC3) | Optical (U) | 275.0 nm |
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Hubble (WFC3) | Optical (U) | 336.0 nm |
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Hubble (ACS) | Optical (B) | 435.0 nm |
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Hubble (ACS) | Optical (V) | 606.0 nm |
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Hubble (ACS) | Optical (i) | 775.0 nm |
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Hubble (ACS) | Optical (z) | 850.0 nm |
WFC3: Sept. 6, 2009 - Oct. 11, 2009;ACS: Sept. 2002 - Dec. 2004 |
Detailed color mapping information coming soon...
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