Astrophysicists from Harvard University have identified a potential new dwarf planet, designated as 2026 ED138, located beyond the orbit of Neptune in the Kuiper Belt. The object was detected using the Vera C. Rubin Observatory in Chile, which utilized a wide field of view to find the object despite its alignment with the brightness of the Milky Way.
The object is estimated to have a diameter between 600 and 1,500 kilometers, suggesting a spherical shape consistent with a dwarf planet. The discovery was announced at the 59th Annual Division Meeting.