Scientists Spot Potential New Dwarf Planet Using Rubin Data

“My first reaction was excited disbelief,” Matthew Holman said after spotting an unusual speck of light in astronomical data.

That initial signal from the night of Oct. 13, 2026, points to 2026 ED138, a potential new dwarf planet orbiting in the distant fringes of our solar system. If confirmed by further observation, the icy world beyond Neptune could rank among the largest objects ever discovered in that region, measuring roughly 370 to 930 miles across.

How Astronomers Tracked 2026 ED138 Across a Decade

Matthew Holman, a Harvard & Smithsonian astrophysicist, made the discovery while running Rubin data through a custom computer program designed to spot moving objects. When the object emerged in the automated search, Holman noted its high brightness and extreme distance.

YouTube embedded video player

To verify the finding, Mario Jurić, the solar system lead scientist for the Rubin project at the University of Washington, searched through additional telescope files. Jurić located 20 previous sightings captured by the Rubin Observatory between March 4 and July 11, 2026. In total, the Simonyi Survey Telescope logged the object 30 times across 20 distinct nights.

Researchers pushed the timeline back even further by searching archival images through the Asteroid Institute’s ADAM Precovery service. They found the object in digital files dating back to 2016, captured by the Dark Energy Camera on the U.S. Armed with a decade of tracking data, the research team announced the find on Oct. 27, 2026.

Why Surface Reflectivity Remains Unmeasured

While the telescope data establishes an orbit sitting roughly 46 times farther from the sun than Earth does—farther out than Pluto’s average distance of about 40 times—scientists still lack a precise measurement for the object’s physical dimensions. The estimated diameter range of 600 to 1,500 kilometers relies on three primary variables: distance, brightness, and an assumed albedo, or surface reflectivity.

Because the actual reflectivity has not yet been measured, researchers cannot confirm whether the candidate sits closer to the smaller or larger end of that estimated scale. The object traces an orbital path close to the plane of the Milky Way, where millions of background stars create visual crowding that makes faint, slow-moving bodies difficult to isolate from ordinary light sources.

YouTube embedded video player

What Qualifies a Body as a Dwarf Planet

If subsequent studies confirm its physical characteristics, 2026 ED138 will join Ceres, Eris, Haumea, Makemake, and Pluto as the sixth recognized dwarf planet in the solar system. The dwarf planet category was established during a major astronomical debate sparked by the 2005 discovery of Eris, an icy world comparable in size to Pluto.

In 2006, the International Astronomical Union formally defined a planet as an object that orbits the sun, possesses enough mass to pull itself into a rounded spherical shape, and has cleared its immediate orbital neighborhood of other debris. A dwarf planet meets the first two criteria but fails the third, sharing its orbital zone with numerous other bodies in the Kuiper Belt—a doughnut-shaped region of icy remnants beyond Neptune.

ED138 graphic
Photo: New Atlas

Frequently Asked Questions About 2026 ED138

Where is the Vera C. Rubin Observatory located?

The observatory sits on Cerro Pachón in Chile.

What instrument captured the initial images?

The Simonyi Survey Telescope at the Rubin Observatory tracked the candidate dwarf planet 30 times across 20 nights using the world’s largest digital camera, the 3,200-megapixel LSST Camera.

How far is the object from Earth?

The candidate orbits at a distance of approximately 46 times farther from the sun than Earth does, which translates to about 4.3 billion miles away.

What makes finding objects in this region difficult?

Because the object travels along a trajectory near the crowded plane of the Milky Way, millions of background stars obscure faint moving specks, requiring specialized software to connect scattered data points across multiple nights.

2026 ED138 3D orbit