Skip to main content

Hubble captures a cosmic sea monster with this image of a jellyfish galaxy

This week’s image from the Hubble Space Telescope shows a special and delightful cosmic object: a jellyfish galaxy. These galaxies are named for their larger main body with tendrils that float along after them, like the sea creatures.

This particular jellyfish galaxy is called JO201, and is located in the constellation of Cetus. Appropriately for the sea theme, Cetus is a constellation named after a Greek mythological sea monster that sometimes had the body of a whale or serpent along with the head of a boar. In the image, you can see the main body of the galaxy in the center, with the trailing tendrils spreading down toward the bottom of the frame.

A jellyfish galaxy with trailing tentacles of stars hangs in inky blackness in this image from the NASA/ESA Hubble Space Telescope. As Jellyfish galaxies move through intergalactic space they are slowly stripped of gas, which trails behind the galaxy in tendrils illuminated by clumps of star formation. These blue tendrils are visible drifting below the core of this galaxy, and give it its jellyfish-like appearance. This particular jellyfish galaxy — known as JO201 — lies in the constellation Cetus, which is named after a sea monster from ancient Greek mythology. This sea-monster-themed constellation adds to the nautical theme of this image.
A jellyfish galaxy with trailing tentacles of stars hangs in inky blackness in this image from the NASA/ESA Hubble Space Telescope. ESA/Hubble & NASA, M. Gullieuszik

Jellyfish galaxies are formed due to an effect called ram-pressure stripping, in which the gravity of other nearby objects like galaxies or galaxy clusters acts like a headwind, moving dust and gas from the galaxy and stripping it in some regions. This process can slow star formation in the galaxy as there is no longer enough dust or gas available to form new stars, and can even cause the eventual death of the galaxy in question.

Recommended Videos

This image was taken using Hubble’s Wide Field Camera 3 instrument looking in both the optical and ultraviolet wavelengths, in order to pick out all the important features of the galaxy, its dust and gas, and its tendrils. It was taken as part of research into jellyfish galaxies and how star formation occurs within them.

Please enable Javascript to view this content

“This particular observation comes from an investigation into the sizes, masses, and ages of the clumps of star formation in the tendrils of jellyfish galaxies,” Hubble scientists write. “Astronomers hope that this will provide a breakthrough in understanding the connection between ram-pressure stripping — the process that creates the tendrils of jellyfish galaxies — and star formation.”

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Feast your eyes on 10 years of Hubble images of Jupiter, Saturn, Uranus, Neptune
This is a montage of NASA/ESA Hubble Space Telescope views of our solar system's four giant outer planets: Jupiter, Saturn, Uranus, and Neptune, each shown in enhanced color. The images were taken over nearly 10 years, from 2014 to 2024.

While the Hubble Space Telescope might be most famous for its images of beautiful and far-off objects like nebulae or distant galaxies, it also takes images of objects closer to home, including the planets right here in our own solar system. For the past 10 years, Hubble has been studying the outer planets in a project called OPAL (Outer Planet Atmospheres Legacy), capturing regular images of each of the four outer planets so scientists can study their changes over time.

The planets Jupiter, Saturn, Uranus, and Neptune are different in many ways from Earth, as they are gas giants and ice giants rather than rocky planets. But they do have some similar phenomena, such as weather that regularly changes, including epic events like storms that are so large they can be seen from space. Jupiter's Great Red Spot, for example, the big orange-red eye shape that is visible on most images of the planet, is an enormous storm larger than the width of the entire Earth and which has been raging for centuries.

Read more
Webb and Hubble snap the same object for two views of one galaxy
Featured in this NASA/ESA/CSA James Webb Space Telescope Picture of the Month is the spiral galaxy NGC 2090, located in the constellation Columba. This combination of data from Webb’s MIRI and NIRCam instruments shows the galaxy’s two winding spiral arms and the swirling gas and dust of its disc in magnificent and unique detail.

With all the excitement over the last few years for the shiny and new James Webb Space Telescope, it's easy to forget about the grand old master of the space telescopes, Hubble. But although Webb is a successor to Hubble in some ways, with newer technology and the ability to see the universe in even greater detail, it isn't a replacement. A pair of new images shows why: with the same galaxy captured by both Webb and Hubble, you can see the different details picked out by each telescope and why having both of them together is such a great boon for scientists.

The galaxy NGC 2090 was imaged by Webb, shown above, using its MIRI and NIRCam instruments. These instruments operate in the mid-infrared and near-infrared portions of the electromagnetic spectrum respectively, which is why the arms of this galaxy appear to be glowing red. These arms are made of swirling gas and dust, and within them are compounds called polycyclic aromatic hydrocarbons that glow brightly in the infrared. The blue color in the center of the galaxy shows a region of young stars burning hot and bright.

Read more
Stunning view of the Sombrero Galaxy captured by James Webb
The NASA/ESA/CSA James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. The mid-infrared light highlights the gas and dust that are part of star formation taking place among the Sombrero galaxy’s outer disk. The rings of the Sombrero galaxy produce less than one solar mass of stars per year, in comparison to the Milky Way’s roughly two solar masses a year. It’s not a particular hotbed of star formation. The Sombrero galaxy is around 30 million light-years from Earth in the constellation Virgo.

A new image from the James Webb Space Telescope shows a stunning and fashionable sight: the Sombrero Galaxy, named for its resemblance to the traditional Mexican hat. With its wide, flat shape reminiscent of the hat's wide brim, the galaxy, also known as Messier 104, has outer rings that are clearly visible for the first time.

The Sombrero Galaxy is located 30 million light-years away, in the constellation of Virgo, and it has been previously imaged by the Hubble Space Telescope. But while in the Hubble image, the galaxy appears as an opaque, pale disk, in the new Webb image you can see an outer blue disk, with a small bright core right at the center.

Read more