Xiangliu (moon)
.jpg) Gonggong and Xiangliu (pointed at by arrow) imaged by the Hubble Space Telescope in 2010 | |
| Discovery | |
|---|---|
| Discovered by | Gábor Marton Csaba Kiss Thomas Müller[1] |
| Discovery date | 18 September 2010 (first identified)[2] (announced 17 October 2016)[3] |
| Designations | |
| Pronunciation | /ʃæŋ.ljuː/ SHANG-LEW |
Named after | 相柳 Xiāngliǔ |
| Orbital characteristics[4] | |
| Epoch 8 December 2014 (JD 2457000.0) | |
| 24021±202 km (prograde), 24274±193 km (retrograde) | |
| Eccentricity | 0.2908±0.007 (prograde), 0.2828±0.0063 (retrograde) |
| 25.22073±0.000357 d (prograde), 25.22385±0.000362 d (retrograde) | |
| Inclination | 83.08°±0.86° (prograde), 119.14°±0.89° (retrograde) |
| 31.99°±1.07° (prograde), 104.09°±0.82° (retrograde) | |
| Satellite of | 225088 Gonggong |
| Physical characteristics | |
| <200 km[5] 40–100 km[4] | |
| >0.2[4] | |
| V–I=1.22±0.17[4] | |
| 6.93±0.15[4] | |
Xiangliu (formal designation (225088) Gonggong I) is the only known moon of the trans-Neptunian dwarf planet Gonggong. It was discovered by Gábor Marton, Csaba Kiss, and Thomas Müller in archival Hubble Space Telescope images taken on 18 September 2010. Its discovery was announced at the 48th Meeting of the Division for Planetary Sciences on 17 October 2016. The moon is named after Xiangliu, the nine-headed venomous snake monster from Chinese mythology who served the water god Gonggong as his chief minister.
Xiangliu is estimated to be less than 100 km (60 mi) in diameter and orbits Gonggong every 25.22 days at an average distance of 24,021 km (14,926 mi). It is thought to be tidally locked to Gonggong and may contribute to the maintenance of its highly eccentric orbit through tidal interactions or the Kozai mechanism.
Discovery
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After Gonggong was found in March 2016 to have an unusually slow rotation period, astronomers proposed that tidal interactions with an orbiting satellite might have caused the slowdown.[1] This possibility prompted Csaba Kiss and colleagues to examine archival observations of Gonggong taken with the Hubble Space Telescope's Wide Field Camera 3.[2] Their analysis of images taken on 18 September 2010 revealed a faint satellite orbiting at a distance of at least 15,000 km (9,300 mi).[6] The discovery was announced by Gábor Marton, Csaba Kiss, and Thomas Müller at the 48th Meeting of the Division for Planetary Sciences on 17 October 2016,[1][6][7] although the satellite was not immediately assigned a provisional designation.[8] The team later identified the satellite in earlier archival Hubble images taken on 9 November 2009.[2]
Name
[edit]The satellite is named after Xiangliu, the nine-headed venomous snake monster and chief minister of the water god Gonggong in Chinese mythology.[9] In the myth, Xiangliu is associated with flooding and destruction.[10] When the discoverers of Gonggong proposed names for a public vote, they deliberately selected mythological figures with associated characters that could later provide names for any satellites.[11] Xiangliu was named by its discovery team, led by Csaba Kiss, which had the privilege of naming the satellite.[12] The names Gonggong and Xiangliu were approved by the International Astronomical Union's Committee on Small Body Nomenclature and announced simultaneously by the Minor Planet Center on 5 February 2020.[13]
Orbit
[edit]
Based on Hubble Space Telescope images of Gonggong and Xiangliu obtained in 2009 and 2010, the discovery team initially constrained Xiangliu's orbital period to between 20 and 100 days.[2] Additional Hubble observations in 2017 allowed the orbit to be determined more accurately.[14] Xiangliu is thought to be tidally locked to Gonggong.[4]
Because observations of Xiangliu cover only a small portion of Gonggong's orbit around the Sun, it is not yet possible to determine whether Xiangliu's orbit is prograde or retrograde.[4] Under a prograde orbital solution, Xiangliu orbits Gonggong at an average distance of about 24,021 km (14,926 mi) and completes one orbit every 25.22 days. The same model indicates that its orbit is inclined by about 83 degrees to the ecliptic, suggesting that Gonggong is viewed nearly pole-on, assuming Xiangliu's orbit is only slightly inclined to Gonggong's equator.[4]
Xiangliu's orbit is highly eccentric, with an eccentricity of about 0.29.[4] This may reflect an initially eccentric orbit or the effects of slow tidal evolution, in which the timescale for orbital circularization is comparable to the age of the Solar System.[4] Another possible explanation is the Kozai mechanism, driven either by solar tidal perturbations or by higher-order variations in Gonggong's gravitational potential caused by its oblate shape.[4]
Physical characteristics
[edit]To preserve its orbital eccentricity over a timescale comparable to the age of the Solar System, Xiangliu is estimated to be less than 100 km (60 mi) in diameter, corresponding to an albedo greater than 0.2.[4][5] At the time of its discovery, its diameter was estimated to be 237 km (147 mi), based on the assumption that it had the same albedo as Gonggong.[2]
Observations by the Hubble Space Telescope in 2017 showed that Xiangliu is 4.59 magnitudes fainter than Gonggong, corresponding to an estimated absolute magnitude of 6.93±0.15, based on Gonggong's estimated absolute magnitude of 2.34.[14][4] Photometric measurements obtained the same year also showed that Xiangliu is significantly less red than Gonggong.[4] The measured color difference, ΔV–I=0.43±0.17, between Gonggong (V–I=1.65±0.03) and Xiangliu (V–I=1.22±0.17) is among the largest color differences observed for any known trans-Neptunian satellite.[4] This pronounced color difference is unusual, as most trans-Neptunian satellites have colors similar to those of their parent bodies.[4]
References
[edit]- 1 2 3 Lakdawalla, Emily (19 October 2016). "DPS/EPSC update: 2007 OR10 has a moon!". The Planetary Society. Archived from the original on 16 April 2019. Retrieved 19 October 2016.
- 1 2 3 4 5 Kiss, Csaba; Marton, Gábor; Farkas-Takács, Anikó; Stansberry, John; Müller, Thomas; Vinkó, József; Balog, Zoltán; Ortiz, Jose-Luis; Pál, András (16 March 2017). "Discovery of a Satellite of the Large Trans-Neptunian Object (225088) 2007 OR10". The Astrophysical Journal Letters. 838 (1): 5. arXiv:1703.01407. Bibcode:2017ApJ...838L...1K. doi:10.3847/2041-8213/aa6484. S2CID 46766640. L1.
- ↑ Johnston, Wm. Robert (22 March 2020). "(225088) Gonggong and Xiangliu". Johnston's Archive. Archived from the original on 1 April 2023. Retrieved 2 March 2020.
- 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 Kiss, Csaba; Marton, Gabor; Parker, Alex H.; Grundy, Will; Farkas-Takacs, Aniko; Stansberry, John; Pal, Andras; Muller, Thomas; Noll, Keith S.; Schwamb, Megan E.; Barr, Amy C.; Young, Leslie A.; Vinko, Jozsef (October 2018). "The mass and density of the dwarf planet (225088) 2007 OR10". Icarus. 334: 3–10. arXiv:1903.05439. Bibcode:2018DPS....5031102K. doi:10.1016/j.icarus.2019.03.013. S2CID 119370310. 311.02.
- 1 2 Arakawa, Sota; Hyodo, Ryuki; Shoji, Daigo; Genda, Hidenori (December 2021). "Tidal Evolution of the Eccentric Moon around Dwarf Planet (225088) Gonggong". The Astronomical Journal. 162 (6): 29. arXiv:2108.08553. Bibcode:2021AJ....162..226A. doi:10.3847/1538-3881/ac1f91. S2CID 237213381. 226.
- 1 2 The moon of the large Kuiper-belt object 2007 OR10 (PDF). 48th Meeting of the Division for Planetary Sciences. American Astronomical Society. 2016. 120.22. Archived (PDF) from the original on 18 October 2016. Retrieved 24 May 2019.
- ↑ "Moon orbits third largest dwarf planet in our solar system". Science Daily. 18 May 2017. Archived from the original on 8 June 2023. Retrieved 19 May 2017.
- ↑ "Help Name 2007 OR10". Archived from the original on 25 May 2019. Retrieved 9 April 2019.
- ↑ "(225088) = Gonggong". Minor Planet Center. International Astronomical Union. Archived from the original on 14 December 2014. Retrieved 2 November 2019.
- ↑ Yang, Lihui; An, Deming (2005). Handbook of Chinese Mythology. Oxford: Oxford University Press. ISBN 978-0-19-533263-6.
- ↑ "Astronomers Invite the Public to Help Name Kuiper Belt Object". International Astronomical Union. 10 April 2019. Archived from the original on 6 November 2020. Retrieved 12 May 2019.
- ↑ Schwamb, M. (29 May 2019). "The People Have Voted on 2007 OR10's Future Name!". The Planetary Society. Archived from the original on 14 May 2020. Retrieved 29 May 2019.
- ↑ "M.P.C. 121135" (PDF). Minor Planet Circular. Minor Planet Center. 5 February 2020. Archived (PDF) from the original on 25 October 2021. Retrieved 19 February 2020.
- 1 2 Parker, Alex (7 April 2017). "The Moons of Kuiper Belt Dwarf Planets Makemake and 2007 OR10 HST Proposal 15207". Mikulski Archive for Space Telescopes. Space Telescope Science Institute. Archived from the original on 18 March 2023. Retrieved 21 September 2018.
