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DGA571045
![Galaxy has 13 billion years - light in cluster CL1358+62 - Galaxy 13 billion light - years away - Image obtained by the Hubble space telescope of the galaxy cluster CL1358+62. This cluster reveals to us, by a gravitational mirage effect, the deformed image of a galaxy, located behind the cluster at a distance of 13 billion years - light (the red crescent at the bottom right of the image). At the top right, a close-up of this arc reveals brighter points, indicating a strong star-forming activity within this galaxy. At the bottom right, a modeling of this arc. A NASA Hubble Space Telescope image of the galaxy cluster CL1358+62 has uncovered a gravitationally - lensed image of a more distant galaxy located far beyond the cluster. The gravitationally - lensed image appears as a red crescent to the lower right of center. The galaxy's image is brightened, magnified, and smeared into an arc - shape by the gravitational influence of the intervening galaxy cluster, which acts like a gigantic lens. Exact measurement of the distance from spectroscopic observations with the W. M. Keck Observatory in Hawaii show the lensed galaxy is one of the farthest ever seen. Its light is only reaching us now from a time when the universe was but 7% its current age of approximately 14 billion years. This places the young galaxy as far as 13 billion light - years away. The lensing foreground cluster is 5 billion light - years from us. [UPPER RIGHT] A close - up of the gravitationally - lensed image shows why astronomers are excited about this unique opportunity to study the distant galaxy's structure. The stretched - out image reveals tiny knots of vigorous starbirth activity. This provides a first detailed look at the early construction phase of a galaxy undergoing training. [LOWER RIGHT] A theoretical model of the cluster lens is used to “” unsmear””” the gravitationally - lensed image back into the galaxy's normal appearance. The corrected image gives a highly](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.35886540.7055475/4565674.jpg?old-wm)
![GOODS Chandra Deep Field South (CDF - S) - Image of distant galaxies obtained by the Hubble space telescope in the constellation of the furnace. Several thousand galaxies, some of which are more than 10 billion light years old, are visible in this image. Some closer galaxies also appear, including two colliding galaxies (middle left). This image is a detail (1/10th) of the complete field observed by Hubble (which contains about 25,000 galaxies) in the framework of the GOODS programme, an extensive program of study of primordial galaxies in a field of the Boreal Constellation of the Great Bear and in a field of the southern hemisphere in the constellation of the furnace. This image, taken with Hubble's Advanced Camera for Surveys, shows several thousand galaxies, many of which appear to be interacting or in the process of forming. Some of these galaxies existed when the cosmos was less than about 2 billion years old. The foreground galaxies, however, are much closer to Earth. Two of them [the white, elongated galaxies, left of center] appear to be colliding. This image represents less than one - tenth of the entire field surveyed by Hubble. The full field, consisting of about 25,000 galaxies, is part of a larger survey called the Great Observatories Origins Deep Survey (GOODS), the most ambitious study of the early universe yet undertaken with the Hubble telescope. This survey targeted two representative spots in the sky - one in the Northern Hemisphere and the other in the Southern Hemisphere. This image represents the southern field, located in the constellation Fornax. The entire GOODS survey reveals roughly 50,000 galaxies. Astronomers have identified more than 2,000 of them as infant galaxies, observed when the universe was less than about 2 billion years old. This image of the southern field was assembled from observations taken between July 2002 and February 2003. 5 days exposure](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.45961640.7055475/4613775.jpg?old-wm)
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