Skip to main content

See the stunning Vela supernova remnant in exquisite detail in expansive image

A new image of the ghostly Vela supernova remnant shows off the fascinating and elaborate structure of this striking cosmic object. Taken using the Dark Energy Camera (DECam), this enormous image is 1.3 gigapixels, making it DECam’s largest image to date.

This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago. This image was taken with the Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the US National Science Foundation's Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF’s NOIRLab. The striking reds, yellows, and blues in this image were achieved through the use of three DECam filters that each collect a specific color of light. Separate images were taken in each filter and then stacked on top of each other to produce this high-resolution image that contains 1.3 gigapixels and showcases the intricate web-like filaments snaking throughout the expanding cloud of gas.
This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago. This image was taken with the Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the U.S. National Science Foundation’s Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile. CTIO/NOIRLab/DOE/NSF/AURA Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab)

A supernova remnant like this is formed when a massive star runs out of fuel and comes to the end of its life. With its hydrogen depleted, the star burns through some its other elements, but the end is now in sight: soon, the heat generated from the fusion won’t be enough to balance out the force of gravity pushing in on the star, and it will collapse in on itself. The energy of this collapse is so great that matter bounces outward in a tremendous explosion, throwing off layers of gas.

Recommended Videos

The supernova that created the Vela remnant, which is located 800 light-years away, happened around 11,000 years ago. Over the thousands of years since then, the shockwave caused by the supernova explosion has traveled out and away from the dead star to create a huge remnant almost 100 light-years across, It has sculpted the dust and gas of the interstellar medium into the delicate structures illuminated in this image, which you can compare to a previous image of the same structure taken by the VLT Survey Telescope.

Please enable Javascript to view this content

The core of the dead star that created this epic structure wasn’t completely destroyed in the explosion, however. It lives on as the Vela pulsar, a type of ultra-dense core called a neutron star that has a powerful magnetic field that causes it to pulse with radio, optical, X-ray, and gamma wavelengths like a lighthouse. It is located in the bottom left of the image.

The DECam data was taken using three filters on the instrument, each of which is sensitive to a different wavelength of light. The reds, yellows, and blues each represent a different filter, and were layered together to create this extremely detailed image that has a total of 35,786 x 35,881 pixels.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
This famous supernova remnant is hiding a secret
Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A). At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W).

When massive stars reach the end of their lives and explode in a supernova, they can leave behind huge structures in space called supernova remnants. These are often favorite targets of astronomers because of their beautiful and distinctive shapes. They include the famous SN 1987A remnant that was imaged by the James Webb Space Telescope last year. Now, astronomers using Webb have peered closer at this remnant and found something special inside.

The SN 1987A supernova was first observed in 1987 (hence its name) and was bright enough to be seen with the naked eye, making it extremely recent by astronomical standards. Stars live for millions or even billions of years, so observing one coming to the end of its life in real time is a real scientific treat. When this star died, it created a kind of supernova called a core collapse, or Type II, in which the heart of the star runs out of fuel, causing it to collapse suddenly and violently. This collapse it so severe that the material rebounds and is thrown out in an explosion traveling up to a quarter of the speed of light.

Read more
Four telescopes work together to create a gorgeous image of a supernova remnant
This deep dataset from Chandra of the remains of a supernova known as 30 Doradus B (30 Dor B) reveals evidence for more than one supernova explosion in the history of this remnant. Unusual structures in the Chandra data cannot be explained by a single explosion. These images of 30 Dor B also show optical data from the Blanco telescope in Chile, and infrared data from Spitzer. Additional data from Hubble highlights sharp features in the image.

A stunning new image of a supernova remnant combines data from four different telescopes to show a colorful, detailed picture of a busy region of space. The remnant 30 Doradus B (or 30 Dor B) was created when a massive star came to the end of its life and exploded, and while the explosion was only brief, it sculpted the dust and gas around the star in a way that remains visible even now, thousands of years later.

This deep dataset from Chandra of the remains of a supernova known as 30 Doradus B (30 Dor B) reveals evidence of more than one supernova explosion in the history of this remnant. Unusual structures in the Chandra data cannot be explained by a single explosion. These images of 30 Dor B also show optical data from the Blanco telescope in Chile, and infrared data from Spitzer. Additional data from Hubble highlights sharp features in the image. Credit: X-ray: NASA/CXC/Penn State Univ./L. Townsley et al.; Optical: NASA/STScI/HST; Infrared: NASA/JPL/CalTech/SST; Image Processing: NASA/CXC/SAO/J. Schmidt, N. Wolk, K. Arcand

Read more
SpaceX shares stunning images of Saturday’s Starship launch
SpaceX's Starship rocket leaving the launchpad on Saturday.

SpaceX has released some stunning images of its Starship rocket heading skyward during its second integrated test flight on Saturday.

The images (below) show the 33 Raptor engines of the first-stage Super Heavy booster as the world’s most powerful space vehicle blasted off the launchpad at SpaceX's Starbase facility in Texas, creating around 17 million pounds of thrust in the process.

Read more