Stunning new image of Butterfly Nebula captured by Gemini South telescope in Chile

Located 2,500 to 3,800 light-years away in the Scorpius constellation, this nebula's unusual shape is a result of its central star shedding material.
PUBLISHED 2 HOURS AGO
NGC 6302 lies between 2,500 and 3,800 light-years away in the constellation Scorpius (Cover Image Source: NASA, ESA, Joel Kastner)
NGC 6302 lies between 2,500 and 3,800 light-years away in the constellation Scorpius (Cover Image Source: NASA, ESA, Joel Kastner)

A dramatic new image of an interstellar 'butterfly' was taken by the Gemini South telescope high atop Cerro Pachón in Chile. The image reveals with striking detail the glowing, wing-like shape of the Butterfly Nebula (NGC 6302) as if it is exploding into space, according to NOIRLab.

To celebrate 25 years since the completion of the International Gemini Observatory, students in Chile voted for the Gemini South telescope to image the NGC 6302 — a billowing planetary nebula that resembles a cosmic butterfly (Image Source: International Gemini Observatory/NOIRLab/NSF/AURA)
To celebrate 25 years since the completion of the International Gemini Observatory, students in Chile voted for the Gemini South telescope to image the NGC 6302 — a billowing planetary nebula that resembles a cosmic butterfly (Image Source: International Gemini Observatory/NOIRLab/NSF/AURA)

This spectacular target was chosen by students in Chile as part of a recent competition celebrating the legacy of the International Gemini Observatory that started operating in 2000. The Butterfly Nebula is a planetary nebula. While typically they do have a planet-like shape, this nebula is distinctly bipolar, shaped like a bug or butterfly. Located between 2,500 and 3,800 light-years away in the constellation Scorpius, the nebula’s unusual shape results from the star at its heart that is emitting layers of gas and dust as it nears the end of its life.

The Butterfly Nebula, NGC 6302, is observed by the instruments on the Hubble, Webb, and ALMA telescopes. (Image Source: ESA | Photo by Hubble, Webb, ALMA)
The Butterfly Nebula, NGC 6302, is observed by the instruments on the Hubble, Webb, and ALMA telescopes. (Image Source: ESA | Photo by Hubble, Webb, ALMA)

The central star is now a white dwarf, a tiny, dense remnant of what was once a massive and one of the hottest stars known, with a surface temperature over 250,000 degrees Celsius. In its prior life, the star was a red giant about 1,000 times the size of our Sun. The star first cast off a slow-moving, donut-shaped band of gas. It later ejected material perpendicular to this band, which channeled the outflows to form the two distinct wings. A subsequent burst of stellar wind, blowing at over 1.8 miles per hour, then carved and sculpted the 'wings' into their intricate, cloud-like structures

This animation shows a burned-out star, called a white dwarf, accreting rocky debris left behind by the star's surviving planetary system (Image Source: NASA, ESA | G. Bacon)
This  shows a burned-out star, called a white dwarf, accreting rocky debris left behind by the star's surviving planetary system (Representative Image Source: NASA, ESA | G. Bacon)

The intense radiation now coming from the hot white dwarf heats the surrounding gas to a temperature of well over 20,000 degrees Celsius so that it glows brightly. While the red areas in the image highlight energized hydrogen gas, the blue regions trace energized oxygen gas. Ultimately, it will disperse into space, along with elements such as nitrogen, sulfur, and iron that it contains, and contribute to the formation of future stars and planets. 

While the recent picture was taken by a ground-based Gemini telescope, the Butterfly Nebula was also imaged by the Hubble Space Telescope (HST) back in 2009, as mentioned on NASA Science. This detailed picture was photographed with Hubble's Wide Field Camera 3, installed during the final Space Shuttle servicing mission. The close-up shows several intricate structures within the dying star's expelled gas cloud. 

A planetary nebula named NGC 6302, also known as, Butterfly Nebula and Bug Nebula, in the Scorpius constellation is pictured in Space. (Cover Image Source: Getty Images | Photo by NASA, ESA, and the Hubble SM4 ERO Team)
A planetary nebula named NGC 6302, also known as, Butterfly Nebula and Bug Nebula, in the Scorpius constellation is pictured in Space. (Image Source: Getty Images | Photo by NASA, ESA, and the Hubble SM4 ERO Team)

The instrument in charge of the latest breathtaking photo, the Gemini South telescope, is one half of the International Gemini Observatory. Its twin is Gemini North, which, according to Space.com, is located on Mauna Kea in Hawaii. Taken together, the two observatories allow for near-continuous coverage of the entire night sky from both the Northern and Southern hemispheres. They are operated by NOIRLab of the National Science Foundation with financial support from Brazil, Canada, Chile, and the United Kingdom. The conception of these identical, high-tech telescopes, which employ advanced optics to gather wide-field images, was the brainchild of astronomer Fred Gillett.

More on Starlust

NASA's James Webb Telescope captures stunning image of warped 'Butterfly Star' 525 light-years away

Heart of Butterfly Nebula in the constellation Scorpius reveals clues to Earth's creation

MORE STORIES

New data from a NASA space telescope hints that scientists may have finally captured the first direct glimpse of the mysterious substance.
1 day ago
Comet 3I/ATLAS might have stolen all the headlines, but it's far from the only comet that has been discovered this year.
4 days ago
The discovery throws light on how giant or dying stars behave with their surroundings and other objects around them. 
Nov 18, 2025
Scientists have spotted a red dwarf star about 130 light-years away ejecting an enormous amount of material into space.
Nov 13, 2025
A black hole has a huge mass packed into an infinitely tiny space.
Nov 13, 2025
The huge collision was detected around 7 billion light-years away with huge masses and extreme black hole spins
Nov 11, 2025
Data from the NSF-funded Zwicky Transient Facility pinpointed the energy source: J2245+3743, an active galactic nucleus 500 million times more massive than our Sun.
Nov 11, 2025
Astronomers pinpointed BiRD near the extensively studied quasar J1030+0524, which resides at a distance of about 12.5 billion light-years from Earth.
Nov 5, 2025