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— CH. 1 · INTRODUCTION —

Xiangliu (moon)

6 min listen · Ch. 1 of 5
5 sections
  • Xiangliu, formally designated 225088 Gonggong I, was not discovered through a pointed telescope aimed at a promising region of sky. It was found inside data that had been sitting in an archive for six years. Gábor Marton, Csaba Kiss, and Thomas Müller announced the find on the 17th of October 2016. The venue was the 48th Meeting of the Division for Planetary Sciences. Behind that announcement lay a detective story that began with a spinning dwarf planet and a nagging question about gravity.

    The dwarf planet is Gonggong, a scattered-disc object far beyond Neptune. In March 2016, researchers established that Gonggong rotates unusually slowly for a body of its type. Tidal drag from a hidden companion was the most plausible explanation they could test. If such a satellite existed, it might have been captured in earlier Hubble images and simply overlooked. That possibility sent Csaba Kiss's team into the archive.

    What emerged from that search was not only a confirmed moon but a set of puzzles still waiting for answers. Why does this satellite look so strikingly different from its host world? And how did a nine-headed serpent from ancient Chinese legend come to name a frozen body at the solar system's outer edge?

  • Wide Field Camera 3 collected the crucial image on the 18th of September 2010, recording a faint object at least 15,000 km from Gonggong. That image remained unexamined for its satellite-hunting potential until the question of Gonggong's slow rotation made it relevant.

    A second set of archival Hubble images, captured on the 9th of November 2009, also contained Xiangliu. The two sets were collected nearly a year apart, and neither had been flagged as notable at the time.

    At the time of announcement, no provisional designation had been assigned to the satellite. Follow-up Hubble observations conducted in 2017 produced a more precise brightness measurement. Xiangliu's absolute magnitude is estimated at 6.93. That figure derives from Gonggong's estimated absolute magnitude of 2.34 and a measured brightness gap of at least 4.59 magnitudes. Those 2017 observations also placed firmer constraints on the moon's orbital path.

  • An orbital period somewhere between 20 and 100 days was the best the initial discovery observations could establish. Subsequent follow-up tightened that considerably. Under a prograde orbit model, Xiangliu completes one full revolution every 25.22 days, traveling at roughly 24,021 km from Gonggong.

    Xiangliu's observed arc covers only a small fraction of Gonggong's full path around the Sun. That limited coverage makes it impossible to determine whether the satellite travels prograde or retrograde.

    An inclination of about 83 degrees to the ecliptic is what the prograde model predicts. That steep tilt implies that observers on Earth are currently looking at the Gonggong system almost directly down onto its pole.

    Three separate mechanisms may explain an orbital eccentricity of 0.29. The orbit may simply have formed elongated. Tidal forces may alternatively be circularizing it so slowly that the process takes as long as the Solar System's entire age to complete. A third possibility is the Kozai mechanism. Under that scenario, perturbations from the Sun's gravity, or from the non-spherical shape of Gonggong itself, periodically reshape the orbit.

    Xiangliu is thought to be tidally locked to Gonggong, always turning the same face toward its host. The 2017 photometric measurements that refined the orbital model also captured the satellite's color. That color measurement would reveal one of the largest color contrasts recorded between the two components of a trans-Neptunian binary.

  • Xiangliu's color index V-I sits at 1.22, while Gonggong's is 1.65. The difference of 0.43 places this pair among the most color-disparate binary trans-Neptunian objects known. Most pairs in the trans-Neptunian region show similar surface colors between their two components. Gonggong and Xiangliu stand apart from that pattern.

    The size of Xiangliu remains uncertain. When the discovery team assumed identical albedos for both bodies, they estimated the satellite's diameter at 237 km. Two boundary constraints now define the plausible range. A theoretical maximum albedo of 1 sets a lower bound of 36 km. For the eccentric orbit to survive over the Solar System's age, Xiangliu must be smaller than 100 km, implying an albedo above 0.2.

    Xiangliu's official name did not arrive until years after the satellite itself had been confirmed. It was the conclusion of a deliberate mythological plan set in motion before the moon was ever found.

  • Chinese mythology describes Xiangliu as a nine-headed venomous snake monster known for bringing floods and destruction. It served as chief minister to the water god Gonggong. That mythological relationship made the satellite's name a natural counterpart to Gonggong's.

    The privilege of naming the satellite rested with the discovery team led by Csaba Kiss. The groundwork for that choice, however, had been laid by an earlier group. When the discoverers of Gonggong selected candidates for a public vote, they deliberately chose mythological figures whose associates could later provide satellite names.

    The International Astronomical Union's Committee on Small Body Nomenclature approved both names. The Minor Planet Center published them simultaneously on the 5th of February 2020. With that, both mythological figures received permanent designations in the outer solar system's catalog. Xiangliu remains the only satellite Gonggong is currently known to have.

Common questions

Who discovered Xiangliu, the moon of Gonggong?

Xiangliu was discovered by a team led by Csaba Kiss. The find was formally announced by Gábor Marton, Csaba Kiss, and Thomas Müller on the 17th of October 2016 at the 48th Meeting of the Division for Planetary Sciences.

How was Xiangliu found in archival Hubble images?

Xiangliu was identified in Hubble Space Telescope images taken with the Wide Field Camera 3 on the 18th of September 2010. The search was prompted by Gonggong's unusually slow rotation, which suggested a gravitational companion had been braking its spin. An earlier set of Hubble images from the 9th of November 2009 was also found to contain the satellite.

What is Xiangliu's orbital period around Gonggong?

Under a prograde orbit model, Xiangliu completes one full orbit around Gonggong every 25.22 days at a distance of roughly 24,021 km. The initial estimate, based only on the discovery images, placed the period anywhere between 20 and 100 days.

How big is Xiangliu, the moon of Gonggong?

Xiangliu's diameter is uncertain. The initial discovery estimate was 237 km, assuming equal reflectivity with Gonggong. Current constraints put its diameter above 36 km at minimum and most likely below 100 km, with an albedo above 0.2 required for the eccentric orbit to have persisted over the Solar System's age.

Why does Xiangliu look different in color from Gonggong?

Xiangliu's color index V-I is 1.22, compared to 1.65 for Gonggong, a difference of 0.43. This gap is among the largest recorded for any binary trans-Neptunian pair; most such pairs show very little color variation between their two components. The cause of the difference has not been established.

What is the mythological origin of the name Xiangliu?

Xiangliu is named after a nine-headed venomous snake monster in Chinese mythology known for causing flooding and destruction, who served as chief minister to the water god Gonggong. Both names were approved by the International Astronomical Union's Committee on Small Body Nomenclature and announced simultaneously by the Minor Planet Center on the 5th of February 2020.

All sources

14 references cited across the entry

  1. 1(225088) = GonggongInternational Astronomical Union
  2. 2DPS/EPSC update: 2007 OR10 has a moon!Emily Lakdawalla — The Planetary Society — 19 October 2016
  3. 3The moon of the large Kuiper-belt object 2007 OR10American Astronomical Society — 2016
  4. 5JournalDiscovery of a Satellite of the Large Trans-Neptunian Object (225088) 2007 OR10Csaba Kiss et al. — 16 March 2017
  5. 6The Moons of Kuiper Belt Dwarf Planets Makemake and 2007 OR10 HST Proposal 15207Alex Parker — Space Telescope Science Institute — 7 April 2017
  6. 7JournalThe mass and density of the dwarf planet (225088) 2007 OR10Csaba Kiss et al. — October 2018
  7. 8JournalTidal Evolution of the Eccentric Moon around Dwarf Planet (225088) GonggongSota Arakawa et al. — December 2021
  8. 10Astronomers Invite the Public to Help Name Kuiper Belt ObjectInternational Astronomical Union — 10 April 2019
  9. 11The People Have Voted on 2007 OR10's Future Name!M. Schwamb — The Planetary Society — 29 May 2019
  10. 12M.P.C. 121135Minor Planet Center — 5 February 2020
  11. 13BookHandbook of Chinese MythologyLihui Yang et al. — Oxford University Press — 2005
  12. 14(225088) Gonggong and XiangliuWm. Robert Johnston — 22 March 2020