Several hundred images taken with NASA's Hubble Space Telescope have been woven together into a rich tapestry of at least 50,000 galaxies. The Hubble view is yielding new clues about the universe's youth, from its "pre-teen" years to young adulthood.The snowstorm of galaxies in the Hubble panorama does not appear evenly spread out. Some galaxies seem to be grouped together. Others are scattered through space. This uneven distribution of galaxies traces the concentration of dark matter, an invisible web-like structure stretching throughout space. Galaxies form in areas rich in dark matter.Among the discoveries so far in this galactic tapestry are a giant red galaxy with two black holes at its core; several new gravitational lenses — galaxies whose gravity bends the light from background galaxies into multiple images; and a rogues' gallery of weird galaxies that should keep astronomers busy for a long time trying to explain them.

Hubble's wide view — achieved by weaving together many separate exposures into a mosaic — still only covers a comparatively small slice of sky. The entire width of the image, in angular size, is no bigger on the sky than the apparent width of your finger held at arm's length. To astronomers, however, this seemingly small area is a big piece of celestial real estate. To cover even this much of the sky, Hubble's Advanced Camera for Surveys snapped more than 500 separate exposures, at 63 different pointings, spread out over the course of one year. The final mosaic is 21 images long by 3 images tall. (The dimensions in degrees are about 1.1 by 0.15 degrees. For comparison, the Moon is about 0.5 degrees in angular size)."These images reveal a wealth of galaxies at many stages of their evolution through cosmic time," said astronomer Anton Koekemoer of the Space Telescope Science Institute in Baltimore, Md., who combined all the Hubble observations to create the final panoramic image, which contains over 3 billion pixels.

The Hubble observation is part of a larger project to study galaxies in a moderately small area of sky, which provides a representative sample of the universe. The study, called the All-wavelength Extended Groth Strip International Survey (AEGIS), utilized four orbiting telescopes and four ground-based telescopes. The five-year project involved the cooperation of more than 50 researchers from around the world observing the same small region of sky in the radio, infrared, visible, ultraviolet, and X-ray regions of the electromagnetic spectrum. The Extended Groth Strip is named for Princeton University physicist Edward Groth. The project is jointly led by Sandra Faber, professor of physics and astronomy at the University of California at Santa Cruz, and Marc Davis, professor of astronomy at the University of California at Berkeley. "The goal was to study the universe as it was when it was about half as old as it is at present, or about 8 billion years ago, a time when youthful galaxies undergoing active formation were becoming quieter mature adults," said Davis.

The Hubble telescope images reveal a time when galaxies were starting to reach their mature shapes, looking like the nearby galaxies we see today. A wide diversity of galaxies can be seen throughout the images. Some are beautiful spirals or massive elliptical galaxies like those seen in the nearby universe, but others look like random assemblages of material, the leftovers from violent mergers of young galaxies. These resemble some of the most distant, youngest galaxies observed, AEGIS team members said.Hubble may have spied tens of thousands of galaxies — many of them odd and chaotic — but other telescopes observing at wavelengths other than the visible over wider areas have pinpointed more extreme and exotic objects, including supermassive black holes and energetic starburst galaxies. In a summary paper now posted online in the Astrophysical Journal Letters, Davis and his colleagues note that AEGIS is providing a unique combination of deep, intensive observations over a comparatively wide area, yielding large samples even of rare types of galaxies. They contrast their work with the Sloan Digital Sky Survey, which has observed the local universe in great detail, but focuses on only the last 2 billion years of cosmic evolution. "As of this time, there is no other region this large on the sky that has been looked at so deeply in so many different wavelengths," Faber said.

A total of 19 papers based on the Groth Strip survey will appear in a special issue of ApJ Letters. All currently are posted online at journals.uchicago.edu/ApJ/

AEGIS provides many windows on this time of transition. Ultraviolet and long-wavelength infrared light from newly born stars, observed by the GALaxy Evolution eXplorer (GALEX) and the Spitzer Space Telescope, respectively, shows that stars were being formed at a much higher rate than today. Shorter-wavelength infrared light measures the total mass of the stars in each galaxy, allowing astronomers to see how galaxies grow larger over time, while X-ray and radio observations by the Chandra X-ray Observatory and the Very Large Array in New Mexico, respectively, can reveal the presence of powerful black holes at galaxies' centers.

Hubble_Pans_Across-Heavens-Harvesting-50000-Evolving-Galaxies

ABOUT THIS IMAGE:
A narrow slice of sky near the Big Dipper yielded a goldmine of at least 50,000 galaxies, which were spied by NASA's Hubble Space Telescope. The Hubble view is yielding new clues about the universe's youth, from its "pre-teen" years to young adulthood.
The image at left, taken by Akira Fujii with a backyard telescope, shows the location of the Hubble observations near the Big Dipper. The long, narrow image in the center is Hubble's panoramic view of the area, made by assembling 500 photographs taken over a one-year period. The 50,000 galaxies spied in the image are scattered across a region that is equivalent to the apparent diameter of two full Moons. The dimensions of the final mosaic are 21 images long by 3 images tall.
The image at right is a section of the panoramic photo.
A wide diversity of galaxies can be seen throughout both Hubble images. Some are beautiful spirals or massive elliptical galaxies like those seen in the nearby universe, but others look like random assemblages of material, the leftovers from violent mergers of young galaxies. These resemble some of the most distant, youngest galaxies observed.
The Hubble observation, made with the Advanced Camera for Surveys, is part of the All-wavelength Extended Groth Strip International Survey, a collaborative effort using major ground-based and space-based telescopes to focus on a narrow swath of sky near the Big Dipper. The region offers a clear view of the distant universe.
Astronomers studying the Groth Strip find that star formation is largely driven by the supply of raw materials, such as gas and dust, collapsing under the force of gravity. More massive galaxies form stars early, whereas the smaller galaxies create their stars over longer timescales. Both normal-looking, undisturbed galaxies and those showing signs of catastrophic collisions were forming an abundance of stars 8 billion years ago. This evidence suggests that violent galaxy mergers were not required for rapid star formation.
The Groth Strip is an extension of an original survey of part of the same region executed in 1994 by Princeton University astronomer Edward J. Groth, who created a mosaic of 28 overlapping fields with the Hubble Wide Field Planetary Camera 2.
The Hubble Advanced Camera for Surveys images were taken from June 2004 to March 2005.
Object Name: Extended Groth Strip (EGS)
Image Type: Astronomical/Illustration
Credit: NASA, ESA, M. Davis (University of California, Berkeley), S. Faber (University of California, Santa Cruz), and A. Koekemoer (STScI)

Cool Nice zooming flash picture can be found here: hubblesite.org/newscenter/archive/releases/2007/06/image/c/format/zoom/

Technical facts about this news release:
About the Object Object Name: Extended Groth Strip, EGS
Object Description: Optical Survey
Position (J2000): R.A. 14h 17m
Dec. +52° 30'
Constellation: Ursa Major
Dimensions: The Extended Groth Strip is 1.1 degrees long by 0.15 degrees wide (70.5 x 10.1 arcminutes, respectively).
 
About the Data Data Description: The Hubble image was created from HST data from proposal 10134: M. Davis (University of California, Berkeley), M. Ashby (Harvard-Smithsonian Center for Astrophysics), T. Small (California Institute of Technology), P. Guhathakurta (University of California, Santa Cruz), L. Simard (Dominion Astrophysical Observatory), K. Noeske (University of California, Santa Cruz), S. Kwok, J. Mader, and P. Amico (California Association for Research in Astronomy (CARA)), A. Koekemoer and R. Somerville (STScI), S. Faber (University of California, Santa Cruz), J. Newman (Lawrence Berkeley National Laboratory), D. Koo (University of California, Santa Cruz), S. White, G. Kauffmann, and V. Springel (Max Planck Institute for Astrophysics, Garching), M. Cooper (University of California, Berkeley), A. Metevier and B. Weiner (University of California, Santa Cruz), and K. Bundy (California Institute of Technology).
Instrument: ACS
Exposure Date(s): June, 2004 - March, 2005
Exposure Time: 3.2 days (76 hours)
Filters: F555W (V) + F814W (I)
 
About the Image Image Credit: NASA, ESA, M. Davis (University of California, Berkeley), S. Faber (University of California, Santa Cruz), and A. Koekemoer (STScI)
Release Date: March 6, 2007
Color: This image is a composite of many separate exposures made by the WFPC2 instrument on the Hubble Space Telescope using two different filters to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are:

F606W (V) blue
F555W (V) + F814W (I) green
F814W (I) red 
 


 

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2009-12-13 17:56:40  sjakiedoedelzak
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Source: hubblesite.org/newscenter/archive/releases/2007/06/


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