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  2. Einstein ring - Wikipedia

    en.wikipedia.org/wiki/Einstein_ring

    An Einstein Ring is a special case of gravitational lensing, caused by the exact alignment of the source, lens, and observer. This results in symmetry around the lens, causing a ring-like structure. [2] The geometry of a complete Einstein ring, as caused by a gravitational lens. The size of an Einstein ring is given by the Einstein radius.

  3. Space telescope reveals rare ‘Einstein ring’ phenomenon with ...

    www.aol.com/news/space-telescope-reveals-rare...

    A close-up view of the center of the NGC 6505 galaxy showcases the bright Einstein ring surrounding it. - ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre, G. Anselmi, T. Li

  4. Relativistic images - Wikipedia

    en.wikipedia.org/wiki/Relativistic_images

    Relativistic Einstein rings are ringed shaped images occurring due to light deflection ^ > when the light source, the lens (the deflector), and the observer are perfectly aligned. Obviously, relativistic Einstein rings are relativistic images for the case when the source, lens, and observer are aligned.

  5. Gravitational lens - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lens

    A light source passes behind a gravitational lens (invisible point mass placed in the center of the image). The aqua circle is the light source as it would be seen if there were no lens, while white spots are the multiple images of the source (see Einstein ring).

  6. Strong gravitational lensing - Wikipedia

    en.wikipedia.org/wiki/Strong_gravitational_lensing

    Strong gravitational lensing is a gravitational lensing effect that is strong enough to produce multiple images, arcs, or Einstein rings. Generally, for strong lensing to occur, the projected lens mass density must be greater than the critical density, that is . For point-like background sources, there will be multiple images; for extended ...

  7. Gravitational microlensing - Wikipedia

    en.wikipedia.org/wiki/Gravitational_microlensing

    A(u) always decreases as u increases, so the closer the alignment, the brighter the source becomes. As u approaches infinity, A(u) approaches 1, so that at wide separations, microlensing has no effect. Finally, as u approaches 0, for a point source A(u) approaches infinity as the images approach an Einstein ring.

  8. Einstein radius - Wikipedia

    en.wikipedia.org/wiki/Einstein_radius

    The Einstein radius is the radius of an Einstein ring, and is a characteristic angle for gravitational lensing in general, as typical distances between images in gravitational lensing are of the order of the Einstein radius.

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

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

    The European Space Agency (ESA) said Monday that its Euclid space telescope has detected a rare bright halo of light around a nearby galaxy.. Known as an Einstein ring, the halo was captured in ...