HUBBLE ATLAS
Hubble Illuminates Cluster of Diverse Galaxies (ESO 325-G004, Abell S0740) — image from the Hubble Space Telescope

Deep fields & lensing

Hubble Illuminates Cluster of Diverse Galaxies

February 5, 2007 · NASA · ESO 325-G004, Abell S0740 · Centaurus

Zoom to full resolution See where it is in the 3D sky Original on NASA ↗

This image from NASA's Hubble Space Telescope shows the diverse collection of galaxies in the cluster Abell S0740 that is over 450 million light-years away in the direction of the constellation Centaurus.

The giant elliptical ESO 325-G004 looms large at the cluster's center. The galaxy is as massive as 100 billion of our suns. Hubble resolves thousands of globular star clusters orbiting ESO 325-G004. Globular clusters are compact groups of hundreds of thousands of stars that are gravitationally bound together. At the galaxy's distance they appear as pinpoints of light contained within the diffuse halo.

Other fuzzy elliptical galaxies dot the image. Some have evidence of a disk or ring structure that gives them a bow-tie shape. Several spiral galaxies are also present. The starlight in these galaxies is mainly contained in a disk and follows along spiral arms.

This image was created by combining Hubble science observations taken in January 2005 with Hubble Heritage observations taken a year later to form a 3-color composite. The filters that isolate blue, red, and infrared light were used with Hubble's Advanced Camera for Surveys .

About the colours

This image is a composite of many separate exposures made by the ACS instrument on the Hubble Space Telescope using several different filters. Three filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F475W (g) Green: F625W (r) Red: F814W (I)

About the data

The Hubble image was created from HST data from proposal 10429 : PI: J. Blakeslee (Washington State University), J. Lucey and R. Smith (University of Durham), J. Tonry (University of Hawaii), and S. Mei (Johns Hopkins University); and 10710: K. Noll, H. Bond, C. Christian, L. Frattare, F. Hamilton, Z. Levay, M. Mutchler, W. Januszewski, and T. Royle (Hubble Heritage Team/STScI), and J. Blakeslee (Washington State University).