Skip to main content

Hubble captures the delicate edge of the enormous Cygnus Loop nebula

The latest image captured by the Hubble Space Telescope shows a glimpse of an elegant, delicate portion of a huge round nebula which was formed when a star 20 times the mass of our sun exploded between 10,000 and 20,000 years ago.

The supernova explosion was so fierce that the dust and gas at the edge of the shock wave is still moving at a speed of over 200 miles per second, and since the event the remnant has expanded out 60 light-years from its original position.

a small section of the Cygnus supernova blast wave
While appearing as a delicate and light veil draped across the sky, this image from the NASA/ESA Hubble Space Telescope actually depicts a small section of the Cygnus supernova blast wave, located around 2,400 light-years away. The name of the supernova remnant comes from its position in the northern constellation of Cygnus (The Swan), where it covers an area 36 times larger than the full moon. ESA/Hubble & NASA, W. Blair

This image shows just one section of the Cygnus Loop, the remnants of a supernova blast located 1,500 light-years away, and despite this distance the loop is so large that it covers an area 36 times larger than the full moon. It is given its name because it is located near the Cygnus constellation, where is sits near one of the swan’s “wings.”

Recommended Videos

If you recognize the name Cygnus Loop, it may well be from another image taken by Hubble which we picked as one of the 10 best images the telescope captured since its launch. This is the Veil Nebula, another part of the same supernova remnant as the new image above, which was named for its delicate, draping appearance. Hubble had to take six different images and scientists arranged them into this mosaic to capture the nebula portion in all its glory:

The remnants of a 8,000 year old supernova
The Veil Nebula, the remnants of the supernova in another section of the Cygnus Loop NASA/ESA/Hubble Heritage Team

This particular part of the loop is considered to be its own nebula, and this portion measures 110 light-years across in total. The line shape was formed by the shock wave of the supernova explosion, and it is wispy due to filaments of gas where the blast wave meets a region of cooler gas.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
See Hubble’s take on the famous and beautiful Carina Nebula
This sparkling new image depicts a small section of the Carina Nebula, one of the NASA Hubble Space Telescope’s most-imaged objects. The Carina Nebula, NGC 3372, is an enormous cloud of gas and dust home to several massive and bright stars, including at least a dozen that are 50 to 100 times the mass of our Sun.

The Hubble Space Telescope recently captured a scene made famous by its sibling, the James Webb Space Telescope. One of the first images released from Webb showed the Carina Nebula, a particularly striking structure of dust and gas located in an area of the Milky Way called the Carina-Sagittarius arm. Recently, Hubble has imaged Carina as well, snapping an image of a small section of this famous nebula.

Compared to Webb's image of Carina, which was taken in the infrared wavelength, Hubble's image is more pastel. Although Hubble operates primarily in the visible light wavelength and Webb operates in the infrared, in this case, Hubble used its infrared capabilities to peer through the dust of the nebula and see its structure.

Read more
Hubble captures an open star cluster in a nearby satellite galaxy
Against a backdrop littered with tiny pinpricks of light glint a few, brighter stars. This whole collection is NGC 1858, an open star cluster in the northwest region of the Large Magellanic Cloud, a satellite galaxy of our Milky Way that boasts an abundance of star-forming regions. NGC 1858 is estimated to be around 10 million years old.clock

The Hubble Space Telescope recently captured an image of a beautiful star cluster called NGC 1858, located in an area full of star-forming regions. This area is part of the Large Magellanic Cloud, one of the Milky Way's satellite galaxies, and is located 160,000 light-years away and is thought to be around 10 million years old.

The Large Magellanic Cloud is one of several satellite galaxies to the Milky Way, which are smaller galaxies that are gravitationally bound to our galaxy. Along with its companion, the Small Magellanic Cloud, it orbits around the Milky Way and will eventually collide with our galaxy in billions of years' time.

Read more
Hubble captures a pair of galaxies merging into an unusual ring shape
The galaxy merger Arp-Madore 417-391 steals the spotlight in this image from the NASA/ESA Hubble Space Telescope. The Arp-Madore catalog is a collection of particularly peculiar galaxies spread throughout the southern sky, and includes a collection of subtly interacting galaxies as well as more spectacular colliding galaxies. Arp-Madore 417-391, which lies around 670 million light-years away in the constellation Eridanus in the southern celestial hemisphere, is one such galactic collision. The two galaxies were distorted by gravity and twisted into a colossal ring, leaving their cores nestled side by side.

This week's image from the Hubble Space Telescope shows a collection of galaxies, with an unusual merging pair as the star of the show. The merging galaxy pair Arp-Madore 417-391 is located 670 million light-years from Earth in the constellation of Eridanus, which is in the southern celestial hemisphere.

The pair are classified as a "peculiar galaxy" because of the way their shapes have been distorted by their interaction. "The Arp-Madore catalog is a collection of particularly peculiar galaxies spread throughout the southern sky, and includes a collection of subtly interacting galaxie,s as well as more spectacular colliding galaxies," Hubble scientists write.

Read more