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Rubin Spots Its First Possible Dwarf Planet

Rubin Observatory has found a faint moving dot that could be a sixth recognized dwarf planet. Older images from 2016, taken by another telescope's camera, helped pin down its orbit.

Well, That Changed2 min read ·
Simulated top-down view of the orbit of dwarf planet candidate 2026 ED138 around the Sun, from NSF–DOE Vera C. Rubin Observatory/NOIRLab.

A new telescope in Chile has spotted a possible dwarf planet, a faint dot that was almost lost among millions of stars. Rubin Observatory calls 2026 ED138 its first dwarf planet candidate.

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What happened

On 27 October 2026, Rubin Observatory announced 2026 ED138 as its first dwarf planet candidate. The object showed up as a faint dot moving against the crowded stars of the Milky Way, lost among the many background sources.[1][4]

The detections came from Rubin data collected earlier in 2026. On the evening of 13 October, the astronomer Holman, of the CfA, ran a search on that data using code written by K. Napier. The search linked the separate detections into one path across the sky.[1]

The Minor Planet Center published the object's details the same day in circular MPEC 2026-U85.[2]

Mosaic of Rubin Observatory images in which a faint dot, marked 2026 ED138, shifts position against dense background stars from March to June 2026.
Rubin's discovery images: the same faint dot, 2026 ED138, moving against the crowded stars of the Milky Way between March and June 2026. NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA · CC BY 4.0

It was already in older pictures

The same object had already been recorded years earlier. According to the Minor Planet Center, its earliest known detection dates to 25 February 2016. Those images came from the DECam camera on the Blanco telescope at Cerro Tololo (observatory code W84), not from Rubin.[2][4]

Our read

In other words, the evidence was sitting in existing images. Nobody had connected those older sightings to a single object until Rubin's detections gave astronomers a path to match them against.[1][2]

Star field with a marked arc showing the path of 2026 ED138 across the sky, with dates of the detections.
The object's path across the sky, traced from its detections. Older sightings, back to 2016, were taken by another telescope's camera. NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA · CC BY 4.0

How the orbit and size were worked out

The older detections trace more than 10 years of the object's orbit. That long record is what lets astronomers pin the orbit down. One trip around the Sun takes about 281 years.[1][2][4]

Right now it is about 46 times Earth's distance from the Sun, out past Pluto. It does not stay that far out. At its closest, it comes within 36.86 au of the Sun, closer than Pluto's average distance.[2]

Its size is estimated at 600 to 1,500 kilometres across. The estimate comes from how bright it looks and an assumed reflectivity, so the true size is not yet measured.[1][4]

Chart of the pathway of 2026 ED138 during May 2026, with circles marking each detection along a line.
Its pathway during May 2026: linking separate detections like these is how the search tied the dots into one orbit. NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA · CC BY 4.0 · cropped

Why it matters

NASA lists five recognized dwarf planets: Ceres, Pluto, Haumea, Makemake and Eris. If 2026 ED138 is confirmed, it would be the sixth.[3]

Our read

The find also shows a working method: new survey data, a search program to link faint moving dots, and older archives to extend the record back in time.[1][2]

Simulation seen from above the Solar System: circular orbits of Jupiter, Saturn, Uranus and Neptune, with the larger, tilted orbit of the dwarf planet candidate 2026 ED138.
Simulation, not a photo: the orbit of 2026 ED138 compared with the outer planets. One trip around the Sun takes about 281 years. NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA/R. Proctor · CC BY 4.0

What's confirmed and what isn't

Confirmed: Rubin found the object in its 2026 data, the 13 October search linked the detections, and older DECam detections reach back to 2016. The orbit period of about 281 years and its current distance come from the Minor Planet Center.[1][2]

Not yet known: its exact size, and whether it truly is a dwarf planet. Rubin says observations in the infrared are needed to constrain its size and confirm its nature.[1]

Nobody has seen what the object looks like. It remains a candidate, and the size range is an estimate rather than a measurement.

  • Not claimedThat 2026 ED138 is a confirmed dwarf planet.
  • Not claimedThat it always orbits beyond Pluto.
  • Not claimedWhat the object looks like.
  • Not claimedThat the 2016 images were taken by Rubin.
  • Not claimedThat its size has been measured rather than estimated.

Sources

  1. Rubin Observatory — Rubin Observatory news release: first dwarf planet candidate, 2026-10-27Primary
  2. Minor Planet Center — Minor Planet Electronic Circular MPEC 2026-U85, 2026-10-27Primary
  3. NASA — Dwarf PlanetsIndependent
  4. Universe Today — The Rubin Observatory finds its first dwarf planet candidateIndependent

7 claims checked against these sources; 6 confirmed.

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Production note: Visuals are unaltered CC BY 4.0 discovery images and labelled orbit simulations from NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA, resized and reframed. No artist's impression or generated imagery was used, and the narration voice is a synthetic preset voice.