The Vera C. Rubin Observatory may have just discovered our solar system’s sixth dwarf planet

October 27, 2026

2 min read

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Located farther away from Earth than Pluto, the object was hidden in the light of the Milky Way's stars

By Adam Kovac edited by Claire Cameron

Congratulations to Pluto, Ceres, Eris, Haumea and Makemake—there may be a new sibling to welcome into the dwarf planet family.

On Tuesday, astronomers at the Vera C. Rubin Observatory announced the discovery of a new dwarf planet candidate in a distant part of the solar system beyond Neptune’s orbit. The new object doesn’t have an official name yet, and is instead going by its provisional designation—2026 ED138.

The discovery was made by running billions of pieces of data collected by the Rubin Observatory through a search code developed by Harvard-Smithsonian Center for Astrophysics astronomer Kevin Napier.

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“My first reaction was one of excited disbelief,” said Holman in a statement. “Objects like this are very rare, so I immediately started checking whether I or the code had done something wrong.”

When Holman and his colleague Mario Jurić of the University of Washington went to double check, they found more 30 observations by Rubin of the object dating between March and July of this year. Looking at other observation tools, the pair found even more sightings going back to 2016. Together, these data allowed the astronomers to begin mapping out 2026 ED138’s orbit.

The suspected dwarf planet is about 46 times farther away from the sun than Earth, making it even more remote than Pluto, which is just 40 times farther away. The object is also tilted off the solar system’s plane by around 25 degrees, which could be due to disruptions caused by Neptune’s gravitational pull.

Initial measurements indicate a diameter between 600 and 1,500 kilometers (373 to 932 miles), which makes it one of the largest dwarf planet candidates yet detected. But size isn’t all that matters: further observations are required to determine if the object has enough mass to be pulled into a round shape, which is a key requirement to be a dwarf planet.

Despite its size, 2026 Ed138 was able to avoid detection for all these years because it’s located in a part of the night sky that’s crowded with stars whose light drowned it out. The Vera C. Rubin observatory, which is loaded with state-of-the-art, powerful instruments and only recently came online, made the discovery possible. Now that the object has been identified, astronomers can get to work on learning more about it to see if it can join Pluto and the others in the dwarf planet family.

“If confirmed as a dwarf planet, ED138 would join a very small family of worlds,” said Holman. “Rubin will image the whole southern sky again and again for ten years, so any others hiding in the places earlier surveys skipped are now within reach.”

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