The Cloverleaf quasar is a bright, gravitationally lensed quasar discovered by Hazard, Morton, Terlevich and McMahon in 1984. It receives its name because of gravitational lensing splitting the single
ESO image of the Cloverleaf quasar
CCD image of the Cloverleaf quasar taken in March 1988 by the ESO/MPI 2.2m telescope. The four separated images are part of the quasar.
An Einstein ring, also known as an Einstein–Chwolson ring or Chwolson ring, is created when light from a galaxy or star passes by a massive object en route to the Earth. Due to gravitational lensing,
Cloverleaf quasar
…around the black hole has been detected suggesting outflow wind. Data from NICMOS and a special algorithm resolved the lensing galaxy and a partial Einstein ring. The Einstein ring represents the host galaxy of the lensed quasar. The Cloverleaf quasar was discovered in 1988. Data on the Cloverleaf collected by…
Einstein ring, created by a nearer galaxy (NGC 6505) distorting light of a distant galaxy. Four images of the distant galaxy, corresponding to four bright spots, can be seen in this picture.
"Smiley" or "Cheshire Cat" image of galaxy cluster (SDSS J1038+4849) and gravitational lensing (an "Einstein ring") discovered by an international team of scientists, imaged with HST
JWST false-color image of SPT0418-47, a high-redshift galaxy rich in organic molecules, which appears as a nearly-perfect Einstein ring
SDSSJ0946+1006 is a Double Einstein Ring. Credit: HST/NASA/ESA