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225088 Gonggong information


225088 Gonggong
Low-resolution Hubble Space Telescope image of Gonggong and its moon Xiangliu, September 2010
Discovery[1][2]
Discovered byMegan Schwamb
Michael E. Brown
David L. Rabinowitz
Discovery sitePalomar Obs.
Discovery date17 July 2007[a]
Designations
MPC designation
(225088) Gonggong
Pronunciation/ˈɡɒŋɡɒŋ/
Named after
共工 Gònggōng
Alternative designations
2007 OR10
Minor planet category
TNO[3] · SDO[4]
3:10 res.[5][6]
 · dwarf planet[7]
Symbol🝽 (mostly astrological)
Orbital characteristics[1]
Epoch 17 December 2020 (JD 2459200.5)
Uncertainty parameter 3
Observation arc37 years and 90 days (13604 days)
Earliest precovery date19 August 1985
Aphelion101.190 AU (15.1378 Tm)
Perihelion33.781 AU (5.0536 Tm)
Semi-major axis
67.485 AU (10.0956 Tm)
Eccentricity0.49943
Orbital period (sidereal)
554.37 yr (202,484 days)[3]
Mean anomaly
106.496°
Mean motion
0° 0m 6.401s / day
Inclination30.6273°
Longitude of ascending node
336.8573°
Time of perihelion
17 February 1857[8]
Argument of perihelion
207.6675°
Known satellites1 (Xiangliu)
Physical characteristics
Mean diameter
1230±50 km[9]
Mean radius
615±25 km
Flattening0.03 (for a rotation period of 22.4 h)[9]
0.007 (for a rotation period of 44.81 h)[9]
Mass(1.75±0.07)×1021 kg[9]
Mean density
1.74±0.16 g/cm3[9]
Equatorial surface gravity
≈ 0.31 m/s2
Equatorial escape velocity
≈ 0.62 km/s
Synodic rotation period
22.40±0.18 h or 44.81±0.37 h
(ambiguous,[10][11] but 22.4 h more likely[9])
Geometric albedo
0.14±0.01[9]
Spectral type
B−V=1.38±0.03[12][13]
V−R=0.86±0.02[12][13]
V−I=1.65±0.028[12][13]
Apparent magnitude
21.4[14]
Absolute magnitude (H)
2.34[10] · 2.0[7]
1.8[3] · 1.6 (assumed)[1]

Gonggong (minor-planet designation: 225088 Gonggong) is a dwarf planet and a member of the scattered disc beyond Neptune. It has a highly eccentric and inclined orbit during which it ranges from 34–101 astronomical units (5.1–15.1 billion kilometers; 3.2–9.4 billion miles) from the Sun. As of 2019, its distance from the Sun is 88 AU (13.2×10^9 km; 8.2×10^9 mi), and it is the sixth-farthest known Solar System object. According to the Deep Ecliptic Survey, Gonggong is in a 3:10 orbital resonance with Neptune, in which it completes three orbits around the Sun for every ten orbits completed by Neptune. Gonggong was discovered in July 2007 by American astronomers Megan Schwamb, Michael Brown, and David Rabinowitz at the Palomar Observatory, and the discovery was announced in January 2009.

At approximately 1,230 km (760 mi) in diameter, Gonggong is similar in size to Pluto's moon Charon, making it the fifth-largest known trans-Neptunian object (apart possibly from Charon). It may be sufficiently massive to be plastic under its own gravity and therefore a dwarf planet. Gonggong's large mass makes retention of a tenuous atmosphere of methane just possible, though such an atmosphere would slowly escape into space. The object is named after Gònggōng, a Chinese water god responsible for chaos, floods and the tilt of the Earth. The name was chosen by its discoverers in 2019, when they hosted an online poll for the general public to help choose a name for the object, and the name Gonggong won.

Gonggong is red, likely due to the presence of organic compounds called tholins on its surface. Water ice is also present on its surface, which hints at a brief period of cryovolcanic activity in the distant past. With a rotation period of around 22 hours, Gonggong rotates slowly compared to other trans-Neptunian objects, which typically have periods of less than 12 hours. The slow rotation of Gonggong may have been caused by tidal forces from its natural satellite, named Xiangliu.

  1. ^ a b c Cite error: The named reference MPC-object was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference MPEC was invoked but never defined (see the help page).
  3. ^ a b c Cite error: The named reference jpldata was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference MPC-CEN-SDO-list was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Buie was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference johnstonsarchive-TNO-list was invoked but never defined (see the help page).
  7. ^ a b Cite error: The named reference Brown-dplist was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference Horizons1857 was invoked but never defined (see the help page).
  9. ^ a b c d e f g Cite error: The named reference massdensity was invoked but never defined (see the help page).
  10. ^ a b Cite error: The named reference Pal-2016 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference scida2015 was invoked but never defined (see the help page).
  12. ^ a b c Cite error: The named reference Boehnhardt-2014 was invoked but never defined (see the help page).
  13. ^ a b c Cite error: The named reference lcdb was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference Grundy-orbits was invoked but never defined (see the help page).


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225088 Gonggong

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Leslie A.; Vinko, Jozsef (2019). "The mass and density of the dwarf planet (225088) 2007 OR10". Icarus. 334: 3–10. arXiv:1903.05439. Bibcode:2018DPS....5031102K...

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Timeline of Solar System astronomy

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24 August 2006. "IAU names dwarf planet Eris". 14 September 2006. "(225088) Gonggong = 2007 OR10". Minor Planet Center. International Astronomical Union...

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Megan Schwamb

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California Institute of Technology (M.S., Ph.D.) Known for Discovery of 225088 Gonggong and other trans-Neptunian objects, Citizen Science projects, Astrotweeps...

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