Suggested Searches

1 min read

Distant Galaxies of Abell 2218 Viewed Through a Cosmic Lens

Distant Galaxies of Abell 2218 Viewed Through a Cosmic Lens
This NASA Hubble Space Telescope image of the rich galaxy cluster, Abell 2218, is a spectacular example of gravitational lensing. The arc-like pattern spread across the picture like a spider web is an illusion caused by the gravitational field of the cluster. The cluster is so massive and compact that light rays passing through it are deflected by its enormous gravitational field, much as an optical lens bends light to form an image. The process magnifies, brightens and distorts images of objects that lie far beyond the cluster. This provides a powerful "zoom lens" for viewing galaxies that are so far away they could not normally be observed with the largest available telescopes. Hubble's high resolution reveals numerous arcs which are difficult to detect with ground-based telescopes because they appear to be so thin. The arcs are the distorted images of a very distant galaxy population extending 5-10 times farther than the lensing cluster. This population existed when the universe was just one quarter of its present age. The arcs provide a direct glimpse of how star forming regions are distributed in remote galaxies, and other clues to the early evoution of galaxies. Hubble also reveals multiple imaging, a rarer lensing event that happens when the distortion is large enough to produce more than one image of the same galaxy. Abell 2218 has an unprecedented total of seven multiple systems. The abundance of lensing features in Abell 2218 has been used to make a detailed map of the distribution of matter in the cluster's center. From this, distances can be calculated for a sample of 120 faint arclets found on the Hubble image. These arclets represent galaxies that are 50 times fainter than objects that can be seen with ground-based telescopes. Studies of remote galaxies viewed through well-studied lenses like Abell 2218 promise to reveal the nature of normal galaxies at much earlier epochs than was previously possible. The technique is a powerful combination of Hubble's superlative capabilities and the "natural" focusing properties of massive clusters like Abell 2218. The image was taken with the Wide Field Planetary Camera 2.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    16h 35m 53.99s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    66° 13' 0.0"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Abell 2218
  • Release Date
    April 5, 1995
  • Science Release
    Hubble Views Distant Galaxies through a Cosmic Lens
  • Credit
    Credits: W.Couch (University of New South Wales), R. Ellis (Cambridge University), and NASA

Downloads

  • 1288 × 655
    jpg (127.38 KB)
  • 1288 × 655
    tif (827.14 KB)
  • 200 × 200
    jpg (5.54 KB)
  • 375 × 191
    jpg (11 KB)
  • 800 × 475
    jpg (52.66 KB)

Share

Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov