
The NASA James Webb Space Telescope (JWST) snapped a striking photograph of an Einstein ring, a bizarre and intriguing optical phenomenon created by gravitational lensing. The unusual sighting was released to the public by the European Space Agency (ESA) and the Canadian Space Agency (CSA) as the image of the month for March, and it includes educational content on the shape of the universe and forces placed upon it.
James Webb Space Telescope uncovers Einstein Ring
The image is a ring system observed when light coming from a distant galaxy is distorted and warped as it passes through an enormous foreground galaxy. The bright center is the foreground, close-by galaxy, and the blue and orange streaking curves around the edge are distorted light from a far-away spiral galaxy. Optical distortion due to gravitational lensing, a powerful effect determined by Einstein’s theory of relativity, produces this photo.
The role of gravitational lensing in forming an Einstein ring
Gravitational lensing happens when a massive object—a galaxy, black hole, or cluster of galaxies—is distorting space-time and deflecting light from a distant source. It is an effect of mass creating a “dent” in space-time and the light following along it. Following the curve, the light gets distorted and enlarged and produces bizarre and captivating optical phenomena. This is a prediction of Einstein’s General Theory of Relativity that has transformed our understanding of gravity and the universe. Ideal Alignment for the Ring to Be Formed
For there to be an Einstein ring, each of the main three must be aligned exactly: the observer, the galaxy that is performing the lensing, and the source of the background light. This won’t be true in the overwhelming majority of cases, so these events are gold dust for science. The lensing causing the ring is only possible when light traversing a background galaxy is maximally amplified by an in-front galaxy or cluster.
Observing the early universe through gravitational lensing
In the galaxy cluster SMACSJ0028.2-7537 in this case here is the ellipsoidal galaxy at the center of this image. So massive a galaxy that it has warped and amplified light from far-off, background spiral galaxies. Such a powerful lens is produced by the enormous energy of such a lens, permitting scientists to look at other galaxies far away in the distance and otherwise too distant or too distant to be observed. Although they are distorted, one can still identify individual star clusters and gas forms of the distant galaxy, and astronomers gain valuable information about the early universe. Window to the Early Universe
Gravitational lensing gives astronomers a unique opportunity to observe distant and remote galaxies, which otherwise remain invisible.
Light from the galaxies, billions of years ago, gives astronomers a glimpse into the early universe. These observations also help astronomers to know how the first galaxies formed shortly after the Big Bang, allowing us to know more about cosmic evolution. The lensing effect, in a way, “magnifies” these galaxies, allowing us to see their shape, size, and other characteristics, which otherwise lie hidden from us.
Gravitational lensing reveals invisible cosmic bodies
One of the most interesting uses of gravitational lensing is in the observation of dark matter and black holes, i.e., dark objects.
The dark bodies themselves cannot be seen, but their existence is inferred from the gravitational effect they exert on surrounding bodies. By observing how light becomes distorted and curved while traveling through dark matter or the gravitational field of black holes in a distant galaxy, astronomers can detect and trace such invisible bodies of the universe.
What is an Einstein Ring?
An Einstein Ring is a rare optical event caused by gravitational lensing, a cosmological phenomenon Albert Einstein explained using his theory of relativity. The effect occurs when light from a distant galaxy is bent and sheared by the gravitational field of a large foreground galaxy and forms a ring-shaped image. The new photo taken by NASA’s James Webb Space Telescope (JWST) captures one of these Einstein rings, a stunning and historic event that has amazed astronomers around the globe.
Einstein Ring historical background
The first Einstein ring was found in 1987. Fewer than a dozen have been observed since, and only with the aid of powerful space telescopes such as Euclid and Hubble can they be observed. Their rarity and precision make them priceless to our knowledge of gravitational lensing, dark matter, and the evolution of the universe.
Why Einstein Rings are important
Einstein rings offer astronomers the unique opportunity to witness a treasure chest of important cosmological phenomena:
- Study of dark matter: Dark matter being lightless, gravitational lensing offers us the facility to study its gravitationally bending power upon light matter.
- Detection of remote galaxies: Gravitational lensing’s magnification of light offers us the ability to observe remote, otherwise invisible, galaxies.
- Measuring the expansion of the universe: Einstein rings can be used to tune our universe expansion models, one of the earliest things in understanding how the universe had grown billions of years ago.