Gonggong
A dwarf-planet candidate about 1,230 km across on a tilted, elongated orbit far beyond Pluto, with a small moon, Xiangliu, found in Hubble images.
At a glance
- Status
- Candidate: likely large enough to be round, not formally classified[2]Not among the five dwarf planets the International Astronomical Union recognizes, although NASA's Hubble team describes it as one
- Size
- About 1,230 km across[1]1,230 km, give or take 50, from Hubble, Kepler and Herschel data combined; an earlier estimate had been 1,535 km
- Orbit
- 33.1 to 101 au from the Sun, once every 550 years or so[4]Semi-major axis 66.9 au, tilted 30.9° to the plane of the planets; a trans-Neptunian object in JPL's catalogue
- Moons
- One, Xiangliu[3]Found in Hubble images from 2009 and 2010 and announced in 2017
- Density
- About 1.75 g/cm³[1]From a system mass of 1.75 × 10²¹ kg, which makes it the fifth most massive known dwarf planet
Timeline
- July 17, 2007Discovered[4]Meg Schwamb, Mike Brown and David Rabinowitz at the Palomar Observatory, California
- November 6, 2009First Hubble images of the moon[3]Four images; a second set followed on 18 September 2010
- May 18, 2017Moon announced[3]Found in the archived Hubble images after Kepler data showed an unusually slow rotation
- February 5, 2020Named Gonggong[4]For a Chinese water god; the moon is named Xiangliu, for his nine-headed minister
Gonggong, long known by its provisional designation 2007 OR10, is one of the largest bodies found beyond Neptune and a dwarf-planet candidate: at about 1,230 km across it is almost certainly round, but the International Astronomical Union has not formally classified it, and the five it recognizes remain Ceres, Pluto, Haumea, Makemake and Eris.[1][2] NASA's Hubble team is less cautious, calling it a member of an exclusive club of nine dwarf planets, of which only Pluto and Eris are larger.[3]
How it was found
It was discovered on 17 July 2007 by Meg Schwamb, Mike Brown and David Rabinowitz with the Samuel Oschin Telescope at the Palomar Observatory in California, in a survey for distant bodies.[4][3] It went unnamed for more than twelve years; the name Gonggong, for a Chinese water god with red hair and a serpent's tail, known for causing chaos and floods, was announced in February 2020.[4]
Orbit
Like Pluto, Gonggong follows an eccentric orbit, and it is currently about three times farther from the Sun than Pluto.[3] JPL's catalogue gives a path from 33.1 to 101 astronomical units, with a semi-major axis of 66.9 astronomical units, tilted 30.9 degrees to the plane of the planets; one orbit takes about 550 years.[4] Its rotation is unusually slow for a Kuiper belt object: NASA's Kepler telescope measured a period of 45 hours, where typical periods are under 24, although JPL's catalogue lists 22.4 hours.[3][4]
Size and interior
Its size has been revised more than once. NASA's 2017 release put it at about 950 miles, roughly 1,530 km, which would have made it the third-largest dwarf planet.[3] A 2019 study that combined Hubble, Kepler and Herschel data with the moon's orbit found a diameter of 1,230 km, give or take 50, and a density of about 1.75 grams per cubic centimeter; the earlier, larger figure would have implied a density of 0.92, unexpectedly low for a body of its size.[1] With a system mass of 1.75 × 10²¹ kg it is the fifth most massive known dwarf planet, after Eris, Pluto, Haumea and Makemake.[1]
The moon
The moon was found in two Hubble observations a year apart, from 6 November 2009 and 18 September 2010, after Kepler's measurement of the slow rotation prompted astronomers to look for a companion that might have slowed the spin.[3] NASA's release estimated it at 150 to 250 miles across, roughly 240 to 400 km, while the 2019 orbit study argues from the orbit's dynamics that it is small, under 100 km.[3][1] Its orbit is noticeably eccentric, which may reflect an intrinsically eccentric orbit with slow tidal evolution, or the Sun's gravitational influence through what is called the Kozai mechanism.[1] The moon is named Xiangliu, the nine-headed poisonous snake who served Gonggong in Chinese mythology.[4]
What is not yet known
Gonggong has never been visited by a spacecraft. Its exact size, the size of Xiangliu and the reason for its slow rotation are all open, and its formal status waits on the International Astronomical Union.[1][2]
Sources
- [1]arXiv (Icarus, 2019), The mass and density of the dwarf planet (225088) 2007 OR10 — doi.org, retrieved November 5, 2026
- [2]NASA, Pluto & Dwarf Planets — science.nasa.gov, retrieved November 5, 2026
- [3]NASA, Hubble Spots Moon Around Third Largest Dwarf Planet — science.nasa.gov, retrieved November 5, 2026
- [4]NASA/JPL Small-Body Database, 225088 Gonggong (2007 OR10) — ssd.jpl.nasa.gov, retrieved November 5, 2026
Related
- What is a dwarf planet?The definition that made Pluto a dwarf planet in 2006, the five the IAU recognises, why the list grows so slowly, and the candidates waiting to join it.
- The Kuiper belt and beyondThe ring of icy worlds past Neptune, the scattered disk and the Oort cloud beyond it, how many objects are known, and how new ones are found.
- ErisThe dwarf planet about the size of Pluto whose discovery in 2005 led to Pluto's reclassification; it orbits about 68 au from the Sun once every 557 years.
- QuaoarA dwarf-planet candidate about 1,110 km across on a nearly circular orbit beyond Pluto, with a moon, Weywot, and two rings where none were expected.
- SednaA dwarf-planet candidate about 995 km across on one of the most distant orbits known, never closer to the Sun than 76 au and about 12,700 years around.
- OrcusA dwarf-planet candidate about 917 km across on an orbit much like Pluto's, in the same resonance with Neptune, with a large moon, Vanth, about half its size.
- 2026 ED138A dwarf-planet candidate found by the Rubin Observatory beyond Neptune and announced on 27 October 2026, an icy world that may be 600 to 1,500 km across.