Skip to main content

Spiral galaxy caught in the act as it’s about to eat its dwarf galaxy neighbor

A recent image from the Dark Energy Camera shows an act of galactic cannibalism, with a spiral galaxy similar to our Milky Way about to devour a nearby dwarf galaxy that has wandered into its path.

The dramatic interaction is occurring between a large spiral galaxy known as Haley’s Coronet and a smaller dwarf galaxy called NGC 1531. The dwarf galaxy is in the process of merging with the larger galaxy, which is being pulled into an irregular shape by the gravitational forces.

The spiral galaxy NGC 1532, also known as Haley’s Coronet, is caught in a lopsided tug of war with its smaller neighbor, the dwarf galaxy NGC 1531. The image — taken by the US Department of Energy’s (DOE) Dark Energy Camera mounted on the National Science Foundation’s (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF’s NOIRLab — captures the mutual gravitational influences of a massive- and dwarf-galaxy merger.
The spiral galaxy NGC 1532, also known as Haley’s Coronet, is caught in a lopsided tug-of-war with its smaller neighbor, the dwarf galaxy NGC 1531. The image — taken by the US Department of Energy’s (DOE) Dark Energy Camera — captures the mutual gravitational influences of a massive galaxy and dwarf galaxy merger. CTIO/NOIRLab/DOE/NSF/AURA; R. Colombari, M. Zamani & D. de Martin (NSF’s NOIRLab)

“This lopsided cosmic tug-of-war is a snapshot of how large galaxies grow and evolve by devouring smaller galaxies, absorbing their stars and star-forming material,” NOIRLab explains. “A similar process has happened in the Milky Way, possibly six times in the past, leaving vast streams of stars and other signs in the halo of the Milky Way.”

The two galaxies shown in the image will eventually merge into one, as the small dwarf galaxy is absorbed by the larger one. But before that happens, you can see how the larger galaxy’s spiral arms are being distorted by gravity, with one spiral arm twisted up toward the top of the image.

How to predict what will happen when two galaxies meet is a complex issue thought to relate to the galaxies’ supermassive black holes, but we do know that the outcome depends on the size of the galaxies involved. In cases like this, one large galaxy can easily absorb a smaller dwarf galaxy. However, when two similarly sized galaxies collide, they may merge to create an unusual structure, or the meeting may result in one of the galaxies being annihilated.

As dramatic as the process of galaxy merging is, however, it isn’t only destructive. Mergers also often trigger waves of star formation, with material like dust and gas forming bridges between the two galaxies and providing the basis for the birth of new stars.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
This one instrument has surveyed 2 million objects to understand dark energy
The Dark Energy Spectroscopic Instrument (DESI) making observations in the night sky on the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory in Arizona.

The vastness of the universe is hard to comprehend, let alone map, but a cosmological project from the National Science Foundation's NOIRLab aims to do just that. The Dark Energy Spectroscopic Instrument (DESI) is designed to create a 3D map of millions of astronomical objects, and an early release of data from the project combines the thousands of exposures taken by the instrument during its validation phase in 2020 and 2021. It contains nearly 2 million objects.

The video below shows part of the survey validation data, with detailed portions of the sky shown in 20 different directions. Each "beam" of light is one part of the data, showing objects like stars, galaxies, and quasars. There are over 700,000 objects in this 3D map, and as impressive as that is, this represents just 1% of the total volume that will be mapped out in the DESI survey.

Read more
Peer inside the bar of a barred spiral galaxy in new James Webb image
A delicate tracery of dust and bright star clusters threads across this image from the NASA/ESA/CSA James Webb Space Telescope. The bright tendrils of gas and stars belong to the barred spiral galaxy NGC 5068, whose bright central bar is visible in the upper left of this image. NGC 5068 lies around 17 million light-years from Earth in the constellation Virgo.

The newest image from the James Webb Space Telescope shows a stunning display of dust and stars that form the bar of the barred spiral galaxy NCG 5068, located 17 million light-years away. Like our galaxy, the Milky Way, this galaxy has a central bar that is a more concentrated region of stars and dust compared to the arms that reach out from the galaxy's center.

The image was taken using two of Webb's instruments, the Mid-Infrared Instrument (MIRI) and the Near Infrared Camera (NIRCam). By looking in both the mid- and near-infrared wavelengths, Webb is able to pick out features like the swirls of dust and gas, as well as the stars in this region, with the bar of the galaxy glowing in the top left of the image.

Read more
Image of darkness and light shows new stars being born in Lupus 3 nebula
The two young, low-mass proto-stars HR 5999 and HR 6000 illuminate nearby dust, creating the reflection nebula Bernes 149. These stars grew out of the dusty dark cloud of Lupus 3, part of a larger complex of as many as nine dark clouds.

A gorgeous new image of a nebular 500 light-years away gives a peek into the process of star formation.

This image from the Dark Energy Camera shows both the dark cloud of Lupus 3 and the shining bright young stars of the nebula Bernes 149. The dark cloud here is essential to the star formation process, as it is a collection of gas and dust which provides the building blocks for new stars to be born. Known as a dark nebula because of its density, Lupus 3 obscures the light of the stars behind it, giving the impression of a swath of black across the starry sky.

Read more