{"id":9529,"date":"2025-02-11T11:04:02","date_gmt":"2025-02-11T16:04:02","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=9529"},"modified":"2025-02-11T11:04:02","modified_gmt":"2025-02-11T16:04:02","slug":"euclid-discovers-a-stunning-einstein-ring","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=9529","title":{"rendered":"Euclid Discovers a Stunning Einstein Ring"},"content":{"rendered":"
The ring of light surrounding the center of the galaxy NGC 6505, captured by ESA\u2019s Euclid telescope, is an example of an Einstein ring. NGC 6505 is acting as a gravitational lens, bending light from a galaxy far behind it. Credit: ESA\/Euclid\/Euclid Consortium\/NASA, image processing by J.-C. Cuillandre, G. Anselmi, T. Li; CC BY-SA 3.0 IGO or ESA Standard Licence<\/figcaption><\/figure>\n

Euclid<\/a> blasted off on its six-year mission to explore the dark Universe on 1 July 2023. Before the spacecraft could begin its survey, the team of scientists and engineers on Earth had to make sure everything was working properly. During this early testing phase, in September 2023, Euclid sent some images back to Earth. They were deliberately out of focus, but in one fuzzy image Euclid Archive Scientist Bruno Altieri saw a hint of a very special phenomenon and decided to take a closer look.<\/p>\n

\u201cI look at the data from Euclid as it comes in,\u201d explains Bruno. \u201cEven from that first observation, I could see it, but after Euclid made more observations of the area, we could see a perfect Einstein ring. For me, with a lifelong interest in gravitational lensing, that was amazing.\u201d<\/p>\n

The Einstein Ring, an extremely rare phenomenon, turned out to be hiding in plain sight in a galaxy not far away. The galaxy, called NGC 6505, is around 590 million light-years from Earth, a stone\u2019s throw away in cosmic terms. But this is the first time that the ring of light surrounding its centre is detected, thanks to Euclid\u2019s high-resolution instruments.<\/p>\n

The ring around the foreground galaxy is made up of light from a farther out bright galaxy. This background galaxy is 4.42 billion light-years away, and its light has been distorted by gravity on its way to us. The far-away galaxy hasn\u2019t been observed before and doesn\u2019t yet have a name.<\/p>\n

A close-up view of the center of the NGC 6505 galaxy, with the bright Einstein ring aligned with it, captured by ESA\u2019s Euclid space telescope. Credit: ESA\/Euclid\/Euclid Consortium\/NASA, image processing by J.-C. Cuillandre, G. Anselmi, T. Li; CC BY-SA 3.0 IGO or ESA Standard Licence<\/figcaption><\/figure>\n

\u201cAn Einstein ring is an example of strong gravitational lensing<\/a>,\u201d explains Conor O\u2019Riordan, of the Max Planck Institute for Astrophysics, Germany, and lead author of the first scientific paper analysing the ring. \u201cAll strong lenses are special, because they’re so rare, and they’re incredibly useful scientifically. This one is particularly special, because it\u2019s so close to Earth and the alignment makes it very beautiful.\u201d<\/p>\n

Albert Einstein\u2019s general theory of relativity predicts that light will bend around objects in space, so that they focus the light like a giant lens. This gravitational lensing effect is bigger for more massive objects \u2013 galaxies and clusters of galaxies. It means we can sometimes see the light from distant galaxies that would otherwise be hidden.<\/p>\n

If the alignment is just right, the light from the distant source galaxy bends to form a spectacular ring around the foreground object. These Einstein rings are a rich laboratory for scientists. Studying their gravitational effects can help us learn about the expansion of the Universe, detect the effects of invisible dark matter and dark energy<\/a>, and investigate the background source whose light is bent by dark matter in between us and the source.<\/p>\n

\u201cI find it very intriguing that this ring was observed within a well-known galaxy, which was first discovered in 1884,\u201d says Valeria Pettorino, ESA Euclid Project Scientist. \u201cThe galaxy has been known to astronomers for a very long time. And yet this ring was never observed before. This demonstrates how powerful Euclid is, finding new things even in places we thought we knew well. This discovery is very encouraging for the future of the Euclid mission and demonstrates its fantastic capabilities.\u201d<\/p>\n

By exploring how the Universe has expanded and formed over its cosmic history, Euclid will reveal more about the role of gravity and the nature of dark energy and dark matter. The space telescope will map more than a third of the sky, observing billions of galaxies out to 10 billion light-years. It is expected to find around 100 000 strong lenses, but to find one that\u2019s so spectacular \u2013 and so close to home \u2013 is astonishing. Until now, less than 1000 strong lenses were known, and even fewer were imaged at high resolution.<\/p>\n

\u201cEuclid is going to revolutionise the field, with all this data we’ve never had before,\u201d adds Conor.<\/p>\n

Although this Einstein ring is stunning, Euclid\u2019s main job is searching for the more subtle effects of weak gravitational lensing, where background galaxies appear only mildly stretched or displaced. To detect this effect, scientists will need to analyse billions of galaxies. Euclid began its detailed survey of the sky on 14 February 2024 and is gradually creating the most extensive 3D map of the Universe yet. Such an amazing find, so early in its mission, means Euclid is on course to uncover many more hidden secrets.<\/p>\n","protected":false},"excerpt":{"rendered":"

Euclid blasted off on its six-year mission to explore the dark Universe on 1 July 2023. Before the spacecraft could begin its survey, the team of scientists and engineers on Earth had to make sure everything was working properly. During this early testing phase, in September 2023, Euclid sent some images back to Earth. They were…<\/p>\n","protected":false},"author":71,"featured_media":9531,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/d2pn8kiwq2w21t.cloudfront.net\/images\/Euclid-EWS-NGC6505-EinsteinRing_embargoed.width-1320.jpg","fifu_image_alt":"","footnotes":""},"categories":[216],"tags":[],"class_list":["post-9529","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-discovery"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9529","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/users\/71"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=9529"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9529\/revisions"}],"predecessor-version":[{"id":9532,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9529\/revisions\/9532"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/9531"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=9529"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=9529"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=9529"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}