Gemini South Marks 25 Years: Photographs the Butterfly Nebula

Soumyadeep Mukherjee

Soumyadeep Mukherjee is an award-winning astrophotographer from India. He has a doctorate degree in Linguistics. His work extends to the sub-genres of nightscape, deep sky, solar, lunar and optical phenomenon photography. He is also a photography educator and has conducted numerous workshops. His works have appeared in over 40 books & magazines including Astronomy, BBC Sky at Night, Sky & Telescope among others, and in various websites including National Geographic, NASA, Forbes. He was the first Indian to win “Astronomy Photographer of the Year” award in a major category.

gemini south observatory celebrates 25th anniversary with a new portrait of the butterfly nebula cover

The International Gemini Observatory has released its new image of NGC 6302, better known as the Butterfly Nebula. The new image marked a milestone. Gemini South, one of the world’s leading ground-based telescopes, turned 25 this year. To celebrate the anniversary, the team decided to let students from Chile and Hawai’i, the telescope’s host communities, choose the object that would headline the observatory’s commemorative release. They picked the Butterfly Nebula, and the result is a detailed, sharply defined portrait that shows why the object has fascinated astronomers for decades.

A celebration in the stars

The 25th anniversary celebration could have taken a very traditional route. The observatory could have selected an object itself, released an image, and moved on. Instead, NSF’s NOIRLab, which operates the Gemini Observatory, invited students near its sites in Chile and Hawai‘i to vote for what Gemini South should observe for the commemoration.

The Butterfly Nebula won by a comfortable margin. It is easy to see why. Even a glance at the image reveals a dramatic object with a recognizable shape, something that feels accessible even to people unfamiliar with astronomy. The decision grounded the anniversary in community involvement, a principle the observatory has sought to uphold throughout its history.

A close-up at the heart of the Butterfly Nebula. Credit: International Gemini Observatory/NOIRLab/NSF/AURA Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)
A close-up at the heart of the Butterfly Nebula. Credit: International Gemini Observatory/NOIRLab/NSF/AURA Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)

The Butterfly Nebula

The Butterfly Nebula is a planetary nebula, the remnants of a star that once resembled our Sun. When such a star runs out of fuel, it becomes unstable and sheds its outer layers into space. Those layers drift outward and interact with previously ejected gas. In the case of NGC 6302, the result is a shape with dual poles: two large lobes extending from a central region that is mostly hidden behind dense dust.

The red regions show ionized hydrogen. The blue areas come from ionized oxygen, which often marks hotter, more energetic zones. Sharp filaments run along the edges of the lobes, tracing places where fast-moving material has collided with slower layers that left the star earlier. Some of these ridges help astronomers map the outflow history of the nebula, how fast the material moved, how it expanded, and how the dying star’s winds shaped the surrounding space.

Although this object has been imaged by other telescopes, including Hubble, the Gemini view brings out a slightly different balance of features. Ground-based telescopes like Gemini, especially with adaptive optics and stable atmospheric conditions, can often highlight structures that space telescopes capture differently. Each view contributes a new layer of understanding. This anniversary image sits comfortably within that legacy.

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. Credit: International Gemini Observatory/NOIRLab/NSF/AURA Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF 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. Credit: International Gemini Observatory/NOIRLab/NSF/AURA Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)

Gemini South: A technical masterpiece

Gemini South stands on Cerro Pachón in northern Chile, 2,737 meters above sea level. The site was chosen for its dry air, steady atmosphere, and reliable night-sky clarity, conditions that allow long exposures without major distortions. The telescope’s 8.1-meter mirror gathers huge amounts of light, making it possible to study faint objects at optical and infrared wavelengths.

But the telescope’s strength is not only in its size. It is in its flexibility. Gemini South can respond quickly to sudden events, such as supernovae or alerts from gravitational-wave detectors. Astronomers rely on this responsiveness for time-sensitive observations, and the system’s adaptive optics allow it to deliver sharp images even when atmospheric conditions shift.

The disc of the Milky Way spreads across the eastern horizon of Hawaiʻi as it rises over the International Gemini Observatory. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/T. Slovinský 
The disc of the Milky Way spreads across the eastern horizon of Hawaiʻi as it rises over the International Gemini Observatory. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/T. Slovinský 

The observatory’s instruments, including spectrographs, infrared cameras, and multi-object systems, give scientists a range of tools. In recent years, Gemini South has helped track unusual stellar eruptions, measure chemical signatures in distant galaxies, and follow up on discoveries from satellites such as TESS and Swift.

Even in 2025, long after its “new telescope” phase ended, Gemini South remained scientifically active. Earlier in the year, it helped study a rare extragalactic recurrent nova with temperatures and chemical features not seen before in such objects. The observatory continues to evolve, adopting new instruments and upgrades to keep it at the forefront of ground-based astronomy.

From a dizzying height, the full scale and remoteness of the Gemini South telescope, one half of the International Gemini Observatory, operated by NSF NOIRLab, can be realized. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/T. Matsopoulos
From a dizzying height, the full scale and remoteness of the Gemini South telescope, one half of the International Gemini Observatory, operated by NSF NOIRLab, can be realized. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/T. Matsopoulos

25 years of the Gemini Observatory

The 25th anniversary of Gemini South marks a milestone for the International Gemini Observatory as a whole. Together, Gemini North in Hawai‘i and Gemini South in Chile provide near-complete sky coverage. Very few observatories offer this combination of hemispheric reach, rapid response capability, and advanced optical systems.

Across its 25 years, Gemini has supported research ranging from near-Earth asteroids to some of the earliest galaxies. It has captured detailed images of nebulae, star-forming regions, and distant clusters. It has also served as an essential partner for transient astronomy, a field that has expanded rapidly with the arrival of new detection networks.

The observatory has faced challenges along the way. One of the most serious came in 2023, when a cybersecurity breach temporarily halted operations. NOIRLab resolved the issue and restored full functionality, but the incident was a reminder that astronomical infrastructure faces real-world vulnerabilities, too. The recovery underscored the resilience and adaptability of the teams that run Gemini’s complex systems.

This image captures the use of the laser guide star (LGS) on Gemini South, the southern twin of the international Gemini Observatory, during a night of observations on Cerro Pachón in the Chilean Andes. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/M. Paredes
This image captures the use of the laser guide star (LGS) on Gemini South, the southern twin of the international Gemini Observatory, during a night of observations on Cerro Pachón in the Chilean Andes. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/M. Paredes

Whether in quiet years or eventful ones, Gemini’s output has remained consistent. Its image archives continue to support new research. Its instruments continue to receive upgrades. And its role within international astronomy continues to grow.

Clear skies!


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Soumyadeep Mukherjee

Soumyadeep Mukherjee

Soumyadeep Mukherjee is an award-winning astrophotographer from India. He has a doctorate degree in Linguistics. His work extends to the sub-genres of nightscape, deep sky, solar, lunar and optical phenomenon photography. He is also a photography educator and has conducted numerous workshops. His works have appeared in over 40 books & magazines including Astronomy, BBC Sky at Night, Sky & Telescope among others, and in various websites including National Geographic, NASA, Forbes. He was the first Indian to win “Astronomy Photographer of the Year” award in a major category.

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