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  2. SDSSJ0946+1006 - Wikipedia

    en.wikipedia.org/wiki/SDSSJ0946+1006

    The main lens lies at redshift z = 0.222, with the inner ring at z = 0.609 with an Einstein radius R E = 1.43 ± 0.01" and magnitude m = 19.784 ± 0.006, the outer ring is at z ≲ 6.9 with R E = 2.07 ± 0.02" and magnitude m = 23.68 ± 0.09 [1] The lensing galaxy is also known as SDSSJ0946+1006 L1, with the nearer lensed galaxy as SDSSJ0946 ...

  3. Gravitational lens - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lens

    In 2009, weak gravitational lensing was used to extend the mass-X-ray-luminosity relation to older and smaller structures than was previously possible to improve measurements of distant galaxies. [29] As of 2013 the most distant gravitational lens galaxy, J1000+0221, had been found using NASA's Hubble Space Telescope.

  4. Tests of general relativity - Wikipedia

    en.wikipedia.org/wiki/Tests_of_general_relativity

    Astronomers using the Hubble Space Telescope and the Very Large Telescope have made precise tests of general relativity on galactic scales. The nearby galaxy ESO 325-G004 acts as a strong gravitational lens, distorting light from a distant galaxy behind it to create an Einstein ring around its centre. By comparing the mass of ESO 325-G004 (from ...

  5. Eddington experiment - Wikipedia

    en.wikipedia.org/wiki/Eddington_experiment

    Einstein's 1911 paper predicted deflection of star light on the limb of the Sun to be 0.83 seconds of arc and encouraged astronomers to test this prediction by observing stars near the Sun during a solar eclipse. [9] It is fortunate for Einstein that the weather precluded results by Perrine in 1912 and Perrine, Freundlich, and Campbell in 1914.

  6. Einstein Cross - Wikipedia

    en.wikipedia.org/wiki/Einstein_Cross

    The Einstein Cross (Q2237+030 or QSO 2237+0305) is a gravitationally lensed quasar that sits directly behind the centre of the galaxy ZW 2237+030, called Huchra's Lens.Four images of the same distant quasar (plus one in the centre, too dim to see) appear in the middle of the foreground galaxy due to strong gravitational lensing.

  7. Gravitational microlensing - Wikipedia

    en.wikipedia.org/wiki/Gravitational_microlensing

    Gravitational lensing's modern theoretical framework was established with works by Yu Klimov (1963), Sidney Liebes (1964), and Sjur Refsdal (1964). [1] Gravitational lensing was first observed in 1979, in the form of a quasar lensed by a foreground galaxy.

  8. ESA’s space telescope Euclid discovers ‘astonishing' Einstein ...

    www.aol.com/news/esa-space-telescope-euclid...

    For me, with a lifelong interest in gravitational lensing, that was amazing." For most of the population out there, an Einstein Ring is an "extremely rare phenomenon," the ESA said.

  9. How astronomers used gravitational lensing to discover 44 new ...

    www.aol.com/news/astronomers-discovered-44-stars...

    The most powerful telescope to be launched into space has made history by detecting a record number of new stars in a distant galaxy. NASA's James Webb Space Telescope, history's largest and most ...