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New observations of Pa 30 show that its firework-like streaks are not smooth: they resolve into filaments made of tightly spaced, remarkably uniform gas knots. The remnant is associated with the supernova recorded in 1181, and the observations offer a sharper look at a rare survivor of an incomplete stellar explosion.

What the new images reveal

An international team co-led by Ilaria Caiazzo of the Institute of Science and Technology Austria (ISTA) and Tim Cunningham used the Gemini North telescope to obtain what ISTA describes as the most detailed view yet of Pa 30. The work, published in 2026 in The Astrophysical Journal as “Detection of knots in the supernova type Iax remnant Pa 30,” resolves the nebula’s bright, firework-like streaks into filaments containing close chains of gas knots. The published study is by Cunningham, Caiazzo, J. C. Raymond, and S. J. Kenyon.

The knots appear strikingly similar in size. Caiazzo described one knot as large enough that the planetary region of our solar system could fit inside it about ten times, with room to spare. That is a scale comparison, not a claim that the knots are solid objects: astronomers see light emitted by gas in the nebula.

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How astronomers resolved the knot chains

The team analyzed emission from two ionized gases: sulfur (S II), observed in red visible light, and doubly ionized oxygen (O III), represented in blue-green tones. In the S II observations, the researchers resolved roughly ten times as many filamentary features as earlier images could show. The new detail reveals structure in the nebula’s emitted light; it does not by itself explain how that structure formed.

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Gemini North stands on Mauna Kea in Hawai‘i, at an elevation above 4,200 meters. It is one half of the International Gemini Observatory; the other telescope, Gemini South, is in Chile. NSF NOIRLab runs the observatory.

Why Pa 30 is unusual

Pa 30 lies about 7,500 light-years away and is associated with a supernova witnessed in 1181 and recorded independently in Japanese, Chinese, and Arabic historical sources. The nebula itself was first identified in 2013 by a citizen scientist. ISTA describes it as one of only five supernovae recorded before the telescope era whose remnants had long remained unidentified.

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The release calls Pa 30 the only known remnant of its kind in the Milky Way. Its center contains a surviving stellar remnant, sometimes informally called a “zombie star,” left by an incomplete explosion. The event is classified as Type Iax, a rare kind of supernova. A collision between two white dwarfs has been proposed as the origin, but that explanation is not established as settled fact.

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What the centered star can tell astronomers

The surviving star appears almost perfectly centered in the nebula. In many supernova explosions, an uneven blast can give a surviving star a “kick” that sends it moving away from the center. The team measured a surprisingly small upper limit on the star’s sideways, or transverse, kick speed. ISTA’s public account does not give a numerical value for that limit.

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What remains unexplained

The observations establish the knots, their chain-like arrangement, and their remarkably similar sizes, but the ISTA account does not identify the physical process that produced them. Caiazzo said the team is eager to model the features. The imagery therefore adds a new puzzle as well as detail: astronomers can now study the knots more clearly, while their formation mechanism remains an open question.

Pa 30’s proximity also makes its central remnant unusually accessible to study. Similar remnants in other galaxies cannot be resolved in the same way, according to ISTA. Cunningham said the team’s findings could help astronomers sift large datasets for other examples, including possible remnants still hidden in the Milky Way.

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