James Webb snaps a stunning stellar nursery in a nearby satellite galaxy

By Georgina Torbet Published February 16, 2024

A stunning new image from the James Webb Space Telescope shows a star-forming region in the nearby galaxy of the Large Magellanic Cloud. Our Milky Way galaxy has a number of satellite galaxies, which are smaller galaxies gravitationally bound to our own, the largest of which is the Large Magellanic Cloud or LMC.

The image was taken using Webb’s Mid-Infrared Instrument or MIRI, which looks at slightly longer wavelengths than its other three instruments which operate in the near-infrared. That means MIRI is well suited to study things like the warm dust and gas found in this region in a nebula called N79.

This image from the NASA/ESA/CSA James Webb Space Telescope features an H II region in the Large Magellanic Cloud (LMC), a satellite galaxy of our Milky Way. This nebula, known as N79, is a region of interstellar atomic hydrogen that is ionised, captured here by Webb’s Mid-InfraRed Instrument (MIRI). — This image from the NASA/ESA/CSA James Webb Space Telescope features an H II region in the Large Magellanic Cloud (LMC), a satellite galaxy of our Milky Way. This nebula, known as N79, is a region of interstellar atomic hydrogen that is ionised, captured here by Webb’s Mid-InfraRed Instrument (MIRI). ESA/Webb, NASA & CSA, O. Nayak, M. Meixner

Within this nebula are three giant molecular clouds full of ionized hydrogen. This image focuses on one of these areas, called N79 South. Regions like this are full of star formation, and with its rich environment of dust and gas, the LMC hosts several such areas. One of the most famous is the Tarantula Nebula, which, like N79, is also an area full of ionized hydrogen where new stars are being formed.

Recommended Videos

The LMC also hosts another beautiful phenomenon previously imaged by Webb, the remnant of supernova 1987A. When a massive star exploded, seen in 1987, it threw out layers of material that traveled out into space to create a striking ring structure.

In this image of N79, the light coming from the center of the image has an unusual shape. That’s because of the shape of Webb’s mirror, scientists explain:

“The distinct ‘starburst’ pattern surrounding this bright object is a series of diffraction spikes. All telescopes which use a mirror to collect light, as Webb does, have this form of artifact which arises from the design of the telescope. In Webb’s case, the six largest starburst spikes appear because of the hexagonal symmetry of Webb’s 18 primary mirror segments.

“Patterns like these are only noticeable around very bright, compact objects, where all the light comes from the same place. Most galaxies, even though they appear very small to our eyes, are darker and more spread out than a single star, and therefore do not show this pattern.”

Georgina Torbet

Space Writer

Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…

Topics

Tech News

Space

James Webb captures gorgeous image of a Cosmic Tornado

The NASA/ESA/CSA James Webb Space Telescope observed Herbig-Haro 49/50, an outflow from a nearby still-forming star, in high-resolution near- and mid-infrared light with the NIRCam and MIRI instruments. The intricate features of the outflow, represented in reddish-orange color, provide detailed clues about how young stars form and how their jet activity affects the environment around them. A chance alignment in this direction of the sky provides a beautiful juxtaposition of this nearby Herbig-Haro object (located within our Milky Way) with a more distant, face-on spiral galaxy in the background.

The James Webb Space Telescope has captured another stunning image of space, this time showing the dramatic scenes around a baby star. Very young stars can throw off powerful jets of hot gas as they form, and when these jets collide with nearby dust and gas they form striking structures called Herbig-Haro objects.

This new image shows Herbig-Haro 49/50, located nearby to Earth at just 630 light-years away in the constellation Chamaeleon. Scientists have observed this object before, using the Spitzer Space Telescope, and they named the object the "Cosmic Tornado" because of its cone-like shape. To show the impressive powers of James Webb to capture objects like this one in exquisite detail, you can compare the Spitzer image from 2006 and the new James Webb image.

Space

NASA’s Webb telescope peers straight at Saturn-like planets 130 light-years away

Saturn captured by the James Webb Space Telescope.

The James Webb Space Telescope is NASA's most precise and technically proficient equipment for observing the wonders of the universe. Astronomers rely on it to unravel the deepest secrets by peaking at distant solar systems and capturing planets like those in ours.

Much recently, the Webb Telescope was able to capture its first direct image of exoplanets nearly 130 light-years away from the Earth. The observatory seized images of four "giant" planets in the solar system of a distant star called HR 8799. This is a fairly young system formed roughly 30 million years ago, a timeline that dwarfs in comparison to our solar system's 4.6 billion years of age.

Space

James Webb captures a stunning view of the dreamy Flame Nebula

Webb's image of the Flame Nebula

Our universe is host to many beautiful and fascinating objects, and we're lucky enough to be able to view many of them using high tech instruments like the James Webb Space Telescope. A new Webb image shows a new view of the gorgeous Flame Nebula, an emission nebula located in the constellation of Orion.

This nebula is a busy stellar nursery, with many new stars being formed there. But it isn't stars which researchers were interested in when they looked to the nebula -- in this case, they were studying objects called brown dwarfs. Bigger than most planets but smaller than a star, brown dwarfs are too small to sustain fusion in their cores, so they are often referred to as failed stars.