These three close-up views show the rich variety of galaxies that appear in the new panoramic, full-color image of the Great Observatories Origins Deep Survey (GOODS) field, taken by NASA's Hubble Space Telescope. The full field reveals 7,500 galaxies in various stages of assembly and stretching back through most of the universe's history.
Astronomers combined new observations taken by the Wide Field Camera 3 (WFC3) and data taken by the Advanced Camera for Surveys (ACS) to make this mosaic.
The image combines a broad range of colors, from the ultraviolet, through visible light, and into the near-infrared. Such a detailed multi-color view of the universe has never before been assembled in such a combination of color, clarity, accuracy, and depth.
Hubble's sharp resolution and new color versatility, produced by combining data from the two cameras, are allowing astronomers to sort out the various stages of galaxy formation. These three views reveal galaxy shapes that appear increasingly chaotic at each earlier epoch, as galaxies grew through accretion, collisions, and mergers. 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.
Ultraviolet light taken by WFC3 shows the blue glow of hot, young stars in galaxies teeming with star birth. The orange light reveals the final buildup of massive galaxies about 8 billion to 10 billion years ago. The near-infrared light displays the red glow of very distant galaxies – in a few cases as far as 12 billion to 13 billion light-years away – whose light has been stretched, like a toy Slinky, from ultraviolet light to longer- wavelength infrared light due to the expansion of the universe.
The WFC3 observations were taken in September and October 2009; the ACS observations in 2004. The view covers 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 evolution of galaxies.
Credits
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)| About The Object | |
|---|---|
| Object Name | GOODS South Field WFC3/ERS Details |
| Object Description | Cosmological Survey |
| R.A. Position | 03h 32m 40.23s |
| Dec. Position | -27° 43' 9.86" |
| Constellation | Fornax |
| About The Data | |
| Data Description | The image was created from Hubble WFC3 data from proposal , R. O'Connell (University of Virginia) and collaborators, combined with the HST/ACS , which includes data from proposals and , P.I. M. Giavalisco; , P.I. Saul Perlmutter; , , and , P.I. A. Riess. |
| Instrument | HST>ACS/WFC, HST>WFC3/UVIS, and HST>WFC3/IR |
| Exposure Dates | Sept. 2002 - Dec. 2004, Exposure Time: 96 orbits (ACS) and Sept. 6, 2009 - Oct. 11, 2009, Exposure Time: 104 orbits (WFC3) |
| Filters | WFC3/IR: F098M, F125W, and F160W ACS/WFC: F435W, F606W, F775W, and F850LP WFC3/UVIS: F225W, F275W, and F336W |
| About The Image | |
| Color Info | The image is a composite of separate exposures made by the WFC3 and ACS instruments on the Hubble Space Telescope. In total, 10 filters were used to sample a very wide wavelength range. The color results from assigning different hues (colors) to combinations of the monochromatic images. In this case, the assigned colors are: Red: WFC3/IR F125W + F160W Green: ACS/WFC F606W + F775W + F850LP + WFC3/IR F098M Blue: WFC3/UVIS F225W + F275W + F336W + ACS/WFC F435W |
| About The Object | |
|---|---|
| Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
| Object Description | The type of astronomical object. |
| R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
| Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
| Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
| Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
| Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
| About The Data | |
| Data Description |
|
| Instrument | The science instrument used to produce the data. |
| Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
| Filters | The camera filters that were used in the science observations. |
| About The Image | |
| Image Credit | The primary individuals and institutions responsible for the content. |
| Publication Date | The date and time the release content became public. |
| Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
| Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |
