Skip to main content

There’s a cosmic jellyfish in this week’s Hubble image

This week’s Hubble image shows an unusual type of galaxy that might seen more at home in the ocean than among the stars: a jellyfish galaxy. These galaxies have a main body of stars, with tentacle-like structures reaching off away from the body in just one direction. This particular jellyfish galaxy, known as JW100, is located more than 800 million light-years away and is found in the constellation of Pegasus.

The jellyfish galaxy is located toward the bottom right of the image, with purple-pink tentacles of stars reaching downward. In the upper middle part of the image, you’ll also see two very bright blobs, which are the core of another galaxy within the same galaxy cluster. This nearby galaxy, called IC 5338, is the brightest one within the cluster and has a large glowing area around it called a halo.

The galaxy JW100 (lower right) features prominently in this image from the NASA/ESA Hubble Space Telescope. The streams of star-forming gas dripping from the disk of the galaxy like streaks of fresh paint are formed by a process called ram pressure stripping. Their resemblance to dangling tentacles led astronomers to refer to JW100 as a ‘jellyfish’ galaxy. JW100 is over 800 million light-years away, in the constellation Pegasus.
The galaxy JW100 (lower right) features prominently in this image from the NASA/ESA Hubble Space Telescope. The streams of star-forming gas dripping from the disk of the galaxy like streaks of fresh paint are formed by a process called ram pressure stripping. Their resemblance to dangling tentacles led astronomers to refer to JW100 as a ‘jellyfish’ galaxy. JW100 is over 800 million light-years away, in the constellation Pegasus. ESA/Hubble & NASA, M. Gullieuszik and the GASP team

As for the jellyfish galaxy, its strange shape is formed through a process called ram pressure stripping. “Ram pressure stripping occurs when galaxies encounter the diffuse gas that pervades galaxy clusters,” Hubble scientists explain. “As galaxies plow through this tenuous gas, it acts like a headwind, stripping gas and dust from the galaxy and creating the trailing streamers that prominently adorn JW100. The bright elliptical patches in the image are other galaxies in the cluster that hosts JW100.”

Scientists are interested in studying jellyfish galaxies to learn more about how stars are formed in their long tendrils. The ram pressure stripping effect feeds dust and gas into the tendrils, which then become hot spots of star formation called starbursts. By studying how stars form in these busy environments, astronomers can learn more about both star formation and about the host clusters in which the jellyfish galaxies reside.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Hubble spots a bright galaxy peering out from behind a dark nebula
The subject of this image taken with the NASA/ESA Hubble Space Telescope is the spiral galaxy IC 4633, located 100 million light-years away from us in the constellation Apus. IC 4633 is a galaxy rich in star-forming activity and also hosts an active galactic nucleus at its core. From our point of view, the galaxy is tilted mostly towards us, giving astronomers a fairly good view of its billions of stars.

A new image from the Hubble Space Telescope shows a galaxy partly hidden by a huge cloud of dust known as a dark nebula. The galaxy IC 4633 still shines brightly and beautifully in the main part of the image, but to the bottom right, you can see dark smudges of dust that are blocking the light from this part of the galaxy.

Taken using Hubble's Advanced Camera for Surveys (ACS) instrument, the image also incorporates data from the DECam instrument on the Víctor M. Blanco 4-meter Telescope, which is located in Chile. By bringing together data from the space-based Hubble and the ground-based DECam, astronomers can get a better look at this galaxy, located 100 million light-years away, and the dark dust partially obscuring it.

Read more
Hubble captures the dramatic jets of a baby star
FS Tau is a multi-star system made up of FS Tau A, the bright star-like object near the middle of the image, and FS Tau B (Haro 6-5B), the bright object to the far right that is partially obscured by a dark, vertical lane of dust. The young objects are surrounded by softly illuminated gas and dust of this stellar nursery. The system is only about 2.8 million years old, very young for a star system. Our Sun, by contrast, is about 4.6 billion years old.

A new image from the Hubble Space Telescope shows the drama that unfolds as a new star is born. Within a swirling cloud of dust and gas, a newly formed star is giving off powerful jets that blast away material and cut through the nearby dust of the surrounding nebula to create this stunning vista.

The image shows a system called FS Tau, located 450 light-years away in a region called Taurus-Auriga. Within this region are many stellar nurseries with new stars forming, making it a favorite target for astronomers studying star formation. But this particular system stands out for the dramatic nature of its newborn star, which has formed an epic structure called a Herbig-Haro object.

Read more
Hubble images the spooky Spider Galaxy
This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829.

This week's image from the Hubble Space Telescope shows an irregular galaxy, the spindly arms and clawed shape of which has led to it being named the Spider Galaxy. Located 30 million light-years away, the galaxy also known as UGC 5829 is an irregular galaxy that lacks the clear, orderly arms seen in spiral galaxies like the Milky Way.

This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829. ESA/Hubble & NASA, R. Tully, M. Messa

Read more