skip to content
 
ROSAT Guest Observer Facility

3C 273

Quasar 3C 273
Image credit: Max-Planck-Institut für extraterrestrische Physik (MPE)

3C 273 is a rather historic quasar. In fact, the history of the word "quasar": itself might bear some explaining. In the early 1960's, a class of mysterious radio-loud objects with an ultraviolet excess in color was discovered by Alan Sandage. At that time, no one knew what these strange objects could be, as they were star-like in size and had variable brightness, yet were radio sources. It wasn't until 3C 273 was identified as one of these bizarre radio sources that things began to happen. Maartin Schmidt discovered that its spectral lines were shifted by 16%; this translates to a redshift of .16. 3C 273 was 1.5 billion light years away from the sun, and was receding even further at a rate of 47,000 kilometers per SECOND. This odd object was further away and more luminous than most known galaxies!

The first of these objects discovered were all very strong radio sources and were called "quasi-stellar radio sources"; this was shortened to "quasar" by a NASA physicist. Later on, Alan Sandage realized that other strange blue objects that had been previously discounted because they were radio-quiet, were most likely quasars as well. Not all quasars were radio sources! So in modern astrophysics, quasars are usually referred to more correctly as QSOs, or "Quasi-Stellar Objects".

Curator: Michael Arida (SP Sys); arida@milkyway.gsfc.nasa.gov
HEASARC Guest Observer Facility


Please use the Feedback link if you have questions on ROSAT.

This file was last modified on Thursday, 04-Oct-2007 12:10:11 EDT

NASA Astrophysics

  • FAQ/Comments/Feedback
  • Education Resources
  • Download Adobe Acrobat
  • A service of the Astrophysics Science Division (ASD) at NASA/ GSFC

    ROSAT Project Scientist: Dr. Robert Petre

    Responsible NASA Official: Phil Newman

    Privacy Policy and Important Notices.