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Split, Distorted Light From Quasar PG1115+080 (left) and a Stretched Ring of Galactic Light (right)

Split, Distorted Light From Quasar PG1115+080 (left) and a Stretched Ring of Galactic Light (right)

Left: The light from the single quasar PG 1115+080 is split and distorted in this infrared image. PG 1115+080 is at a distance of about 8 billion light years in the constellation Leo, and it is viewed through an elliptical galaxy lens at a distance of 3 billion light years. The NICMOS frame is taken at a wavelength of 1.6 microns and it shows the four images of the quasar (the two on the left are nearly merging) surrounding the galaxy that causes the light to be lensed. The quasar is a variable light source and the light in each image travels a different path to reach the Earth. The time delay of the variations allows the distance scale to be measured directly. The linear streaks on the image are diffraction artifacts in the NICMOS instrument (NASA/Space Telescope Science Institute).

Right: In this NICMOS image, the four quasar images and the lens galaxy have been subtracted, revealing a nearly complete ring of infrared light. This ring is the stretched and amplified starlight of the galaxy that contains the quasar, some 8 billion light years away. (NASA/Space Telescope Science Institute).

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    11h 18m 16.98s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    07° 45' 59.4"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    PG1115+080
  • Release Date
    October 26, 1998
  • Science Release
    New Research That Uses Gravitationally Lensed Quasars to Measure Universe is Good News, Bad News for Cosmologists
  • Credit
    Christopher D. Impey (University of Arizona)

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Details

Last Updated
Mar 28, 2025
Contact
Media

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