The vast universe holds many secrets, and the James Webb Space Telescope is on a mission to uncover some of them. Using this powerful telescope, astronomers have just discovered a brand-new galaxy called JWST-ER1.

This exciting find is part of the big JWST COSMOS-Web survey, and they’ve shared all the details in a recent paper released on September 14th through the arXiv preprint server.

Giant elliptical galaxies

Big round galaxies called “giant elliptical galaxies” have always fascinated space fans and scientists. These galaxies are believed to alter their form over time. At times they are quite massive and quiet, while at other times they are something quite different.

The discovery of JWST-ER1

In a groundbreaking discovery, Pieter van Dokkum and his team from Yale University pinpointed JWST-ER1 using the James Webb Space Telescope’s Near Infrared Camera (NIRCam). This achievement was part of an immense undertaking known as the COSMOS-Web project, which aimed to study an astonishing one million galaxies.

Van Dokkum’s team went on to explain, “Our observations with NIRCam revealed JWST-ER1’s unique make-up: an early-type galaxy paired with a full Einstein ring. The center of this ring spans around 1.54 arcseconds.”

Location of the new galaxy

Positioned at a redshift of 1.94, this galaxy spreads out over a region about 21,500 light-years wide and carries an estimated mass that’s a whopping 650 billion times the size of our Sun.

What’s intriguing is that this galaxy isn’t just massive and tranquil; it’s also impressively compact, resembling other quiet galaxies at a similar redshift.

The Einstein ring

Now, let’s talk about the Einstein ring that comes with JWST-ER1, known as JWST-ER1r. Scientists believe it’s created by a distant galaxy at a photometric redshift of 2.98. Although we’ve seen a few Einstein rings before, only a handful are as complete as this one.

One remarkable thing to note is that JWST-ER1 appears to have an almost perfect circular shape. When we look at it through the NIRCam, but we don’t see any areas where new stars are forming. We also see no other noticeable irregularities.