grobi<p>Gravitational Lensing Today</p><p>Excerpts from "Hubble Gravitational Lenses" by Andrea Gianopoulos and "For the First Time Hubble Directly Measures Mass of a Lone White Dwarf" by NASA Hubble Mission Teamon</p><p>Today, Hubble astronomers continue to use the century-old General Relativity/Eddington Experiment to measure distant objects in the universe. For the first time, they measured the mass of a lone white dwarf — the dense, burned-out remnant of a Sun-like star — by seeing how much its gravity deflected the light from a background star. The researchers found that the white dwarf, called LAWD 37, is 56 percent the mass of our Sun, which agrees with earlier theoretical predictions of the white dwarf's mass and corroborated current theories of how white dwarfs evolve as the end product of a typical star's evolution.</p><p>When the mass of the lensing object is much larger, like a large galaxy or cluster of galaxies, the effects of gravitational lensing can resemble a house of mirrors. The gravitational lens not only bends and magnifies the light of distant objects, but distorts it in both space and time.</p><p>One example of this spacetime distortion lies in the galaxy cluster 0024+1654, seen above. The gravitational lens forms as a result of the cluster's tremendous gravitational field that bends light to magnify, brighten, and stretches the image of a more distant object. How distorted the image becomes and how many copies are made depends on the alignment between the foreground cluster and the more distant galaxy, which is behind the cluster. In this photograph, light from the distant galaxy bends as it passes through the cluster, dividing the galaxy into five separate images. The light also distorted the galaxy's image from a normal spiral shape into a more arc-shaped object. </p><p><a href="https://science.nasa.gov/mission/hubble/science/science-behind-the-discoveries/hubble-gravitational-lenses/" rel="nofollow noopener noreferrer" translate="no" target="_blank"><span class="invisible">https://</span><span class="ellipsis">science.nasa.gov/mission/hubbl</span><span class="invisible">e/science/science-behind-the-discoveries/hubble-gravitational-lenses/</span></a><br><a href="https://science.nasa.gov/missions/hubble/for-the-first-time-hubble-directly-measures-mass-of-a-lone-white-dwarf/" rel="nofollow noopener noreferrer" translate="no" target="_blank"><span class="invisible">https://</span><span class="ellipsis">science.nasa.gov/missions/hubb</span><span class="invisible">le/for-the-first-time-hubble-directly-measures-mass-of-a-lone-white-dwarf/</span></a></p><p><a href="https://defcon.social/tags/space" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>space</span></a> <a href="https://defcon.social/tags/galaxy" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>galaxy</span></a> <a href="https://defcon.social/tags/astrophotography" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>astrophotography</span></a> <a href="https://defcon.social/tags/photography" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>photography</span></a> <a href="https://defcon.social/tags/science" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>science</span></a> <a href="https://defcon.social/tags/physics" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>physics</span></a> <a href="https://defcon.social/tags/nature" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>nature</span></a> <a href="https://defcon.social/tags/NASA" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>NASA</span></a> <a href="https://defcon.social/tags/ESA" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>ESA</span></a></p>