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469219 Kamoʻoalewa

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469219 Kamoʻoalewa
Orbit of Kamoʻoalewa in the inner Solar System
Discovery [1]
Discovered byPan-STARRS
Discovery siteHaleakala Observatory
Discovery date27 April 2016
Designations
(469219) 2016 HO3
Pronunciation/kəˌmoʊʔoʊəˈlɛvə/
Hawaiian: [kəˈmoʔowəˈlɛvə]
Named after
Ka moʻo a lewa
("the oscillating fragment")
2016 HO3
Orbital characteristics [2]
Epoch 2024-Mar-31 (JD 2460400.5)
Uncertainty parameter 0
Observation arc20.00 yr (7,306 d)
Aphelion1.10373 AU
Perihelion0.89816 AU
1.00094 AU
Eccentricity0.10269
(964 wrt Earth)[a]
1.0014 yr (365.77 d)
175.153°
0° 59m 3.192s / day
Inclination7.79605°
65.7907°
305.0478°
Earth MOID0.0311 AU (12.1 LD)
Physical characteristics
  • 0.041 km (calculated)[5]
  • 0.04–0.10 km[4]
0.467±0.008 h[b]
0.20 (assumed)[5]
S (assumed)[5]

469219 Kamoʻoalewa (/kəˌmoʊʔoʊəˈlɛvə/),[6] provisionally designated 2016 HO3, is a very small elongated asteroid, fast rotator and near-Earth object of the Apollo group, approximately 40–100 meters (130–330 feet) in diameter. At present it is a quasi-satellite of Earth, and currently the second-smallest, closest, and most stable known such quasi-satellite (after 2023 FW13).

The asteroid was discovered by Pan-STARRS at Haleakala Observatory on 27 April 2016. Numerous proposed missions have since targeted the object, including a NASA solar-sail mission,[7] a University of Colorado flyby and impact experiment,[8] and was selected as a target for the Chinese ZhengHe[9] which has turned into the Tianwen-2 mission.[10] The chondritic simulants QLS-1, 2, and 3 have been developed by the Qian Xuesen Laboratory of Space Technology to better prepare for these missions.[11] In an ambitious proposal, 469219 Kamo’oalewa is even considered for use as a space station for Earth-to-Mars travel.[12]

The object's Earth-like orbit, proximity to the Earth-Moon system, higher spectral reddening to other asteroids, and similarity to space weathered lunar materials indicate that it is likely lunar ejecta.[13][14][15][16] However, it might also be an S-type or L-type asteroid.[17][13][18] Despite being most similar to weathered Apollo 14 and Luna 24 Lunar Mare soils, it is suggested to be from the lunar far-side highland crust crater, Giordano Bruno.[16]

Orbital similarities suggest it is likely a co-orbital pair with 2000 WN10[19] or a broken up set including the other NEOs 2020 KZ2, 2020 PN1, and 2020 PP1.[13]

Discovery and naming

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Kamoʻoalewa was first spotted on 27 April 2016, by the Pan-STARRS 1 asteroid survey telescope on Haleakalā, Hawaii, that is operated by the University of Hawaii's Institute for Astronomy and funded by NASA's Planetary Defense Coordination Office.[1][4] It was named in 2019 Ka moʻo a lewa, from the Hawaiian chant Kumulipo for an oscillating celestial object by A Hua He Ino at the ‘Imiloa Astronomy Center of Hawai’i.[20][21]

The name Kamoʻoalewa is derived from the Hawaiian words ka 'the', moʻo 'fragment', referring to it being a piece broken off a larger object, a 'of', and lewa 'to oscillate', referring to its motion in the sky as viewed from Earth.[22][23] The official naming citation was published by the Minor Planet Center on 6 April 2019 (M.P.C. 112435).[24]

Orbit and classification

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Kamoʻoalewa orbits the Sun at a distance of 0.90–1.10 AU. Although the period as of 2022 is about 366 days, its longer-term average period is closer to 365 days. 469219 Kamoʻoalewa is a quasi-moon and not gravitationally bound to earth like a true satellite. It's orbit transfers between a Quasi satellite orbit type which resides in the L1 and L2 Lagrange points, and Horseshoe orbit between the L4 and L5 Lagrange points.[15][25]

Its orbit has an eccentricity of 0.10 and an inclination of 8° with respect to the ecliptic.[2] It presently has an Earth minimum orbital intersection distance of 0.031 AU (4.6 million km) or 12 lunar distances,[2] well outside of Earth's Hill sphere of 1.5 million km (3.9 LD).

Quasi-satellite of Earth

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The oscillating path of asteroid Kamoʻoalewa as it orbits around the Sun. The traced path of Kamoʻoalewa makes it appear as a constant companion of the Earth.

In a rotating frame of reference Kamoʻoalewa appears to circle elliptically around the Earth every ~45 years.[26] Although it is too distant to be considered a true natural satellite of Earth, it is the best and most stable example to date of a near-Earth companion, or quasi-satellite.[3] Orbital and Yarkovsky effect modeling suggest it will be stable for 0.3-0.5 million years.[19][18][25]

Paul Chodas, manager of NASA's Center for Near-Earth Object Studies (CNEOS) at the Jet Propulsion Laboratory (JPL) in Pasadena, California described the orbit of 2016 HO3 as a quasi-satellite of Earth. Unlike asteroid 2003 YN107, which previously followed a similar orbit, 2016 HO3 is more stable and has been Earth's companion for more than a century and will remain so for much longer. This asteroid spends half of its orbit closer to the Sun than Earth and the other half farther away, causing it to oscillate above and below Earth's orbit annually. Its orbit experiences slight drifts that Earth's gravity corrects, keeping it between 38 and 100 times the distance of the Moon. Thus, 2016 HO3 continually dances around the Earth.[4]

The closest Earth approach was on 27 December 1923 (100 years ago) (1923-12-27) at 12.44 million km (0.0832 AU; 32.4 LD).[2] By late May 2369, the asteroid will be 2.0 AU (780 LD; 300 million km) from Earth.[27] The Earth-like orbit may be a result of it being lunar ejecta.[13] Most objects in this kind of orbit are eventually perturbed out of being in an Earth-co-orbital state and hit the Earth, Venus, or the Sun or are ejected from the solar system, and Kamoʻoalewa will probably hit the Earth in the next 100 million years.[16]

Physical characteristics

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The size of Kamoʻoalewa has not yet been firmly established, but it is approximately 40–100 m (130–330 ft).[4] Based on an assumed standard albedo for stony S-type asteroids of 0.20, its absolute magnitude of 24.3 corresponds to a 41 meters (135 ft) diameter.[5]

Photometric observations in April 2017 revealed that Kamoʻoalewa is a fast rotator. Lightcurve analysis gave a rotation period of 0.467 ± 0.008 hours (28.02 ± 0.48 minutes) and a brightness variation of 0.80±0.05 magnitude (U=2).[5][b]. 2024 inversion modeling was used to create a 100m x 81m x 46m (~72m diameter) 3D model from light curve data.[28]

In 2021, a spectroscopic characterization of Kamoʻoalewa was conducted using the Large Binocular Telescope and the Lowell Discovery Telescope, which found that the asteroid is likely silicate in origin. The object's Earth-like orbit, proximity to the Earth-Moon system, higher spectral reddening to other asteroids, and similarity to space weathered lunar materials indicate that it is likely lunar ejecta.[13][14][15][16] However, it might also be an S-type or L-type asteroid.[17][13][18] Despite being most similar to weathered Apollo 14 and Luna 24 Lunar Mare soils, it is suggested to be from the lunar far-side highland crust crater, Giordano Bruno for its required size and Copernican age.[16]

Lunar ejecta modeling shows some avenues that can achieve a stable QS 469219 Kamo’oalewa-style orbit.[29][15][16]

Exploration

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Proposed missions

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De la Fuente Marcos & de la Fuente Marcos first suggested in situ study of 2016 HO3 because of its ideal orbital characteristics in their August 2016 paper.[30]

During the 2017 Astrodynamics Specialist Conference held in Stevenson in the U.S. state of Washington, a team composed of graduate research assistants from the University of Colorado Boulder and the São Paulo State University (UNESP) was awarded for presenting a project denominated "Near-Earth Asteroid Characterization and Observation (NEACO) Mission to Asteroid (469219) 2016 HO3", providing the first baselines for the investigation of this celestial object using a spacecraft.[31][32][33] Recently, another version of this work was presented adopting different constraints in the dynamics.[34]

A 2019 NASA solar sail mission proposal selected it as a target.[7]

The China National Space Administration (CNSA) is planning a robotic mission that would return samples from Kamoʻoalewa.[35][36] This mission, Tianwen-2, is planned to launch in 2025.[37]

469219 Kamo’oalewa has been considered for use as a space station for Earth-to-Mars travel.[12]

[edit]
Animation of the orbit of Kamoʻoalewa from 2000 to 2300, showing quasi-satellite phase
Relative to Sun and Earth (rotating frame of reference)
Around Earth (non-rotating frame)
Around Sun (non-rotating frame)
   Sun ·    Earth ·    469219 Kamo'oalewa
Animation of the orbit of Kamoʻoalewa from 1600 to 2500, going from horseshoe orbit to quasi-satellite and back
Relative to Sun and Earth (rotating frame of reference)
Around Earth (non-rotating frame)
Around Sun (non-rotating frame)
   Sun ·    Earth ·    469219 Kamo'oalewa

See also

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Notes

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  1. ^ Computed with JPL Horizons using a geocentric solution. Ephemeris Type: Orbital Elements / Center: 500 / Time Span: 2022-Jan-21 (to match infobox epoch)
  2. ^ a b Exceptional rotation period of 0.467 ± 0.008 hours (28.02 ± 0.48 minutes) with a brightness amplitude of 0.80±0.05 mag, quality code = 2, based on summary figures at the LCDB, which references (Reddy 2018).[5] Relevant abstract in ADS is (Reddy 2017).[38]

References

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  1. ^ a b c d "(469219) Kamoʻoalewa = 2016 HO3". Minor Planet Center. Retrieved 29 April 2024.
  2. ^ a b c d e f "JPL Small-Body Database Browser: 469219 Kamo'oalewa (2016 HO3)" (2024-03-18 last obs.). Jet Propulsion Laboratory. Retrieved 29 April 2024.
  3. ^ a b de la Fuente Marcos, C.; de la Fuente Marcos, R. (November 2016). "Asteroid (469219) 2016 HO3, the smallest and closest Earth quasi-satellite". Monthly Notices of the Royal Astronomical Society. 462 (4): 3441–3456. arXiv:1608.01518. Bibcode:2016MNRAS.462.3441D. doi:10.1093/mnras/stw1972.
  4. ^ a b c d e Agle, DC; Brown, Dwayne; Cantillo, Laurie (15 June 2016). "Small Asteroid Is Earth's Constant Companion". Jet Propulsion Laboratory. Retrieved 29 April 2024.
  5. ^ a b c d e f g "LCDB Data for (469219)". MinorPlanet.Info — ALCDEF Query. Asteroid Lightcurve Database (LCDB). Retrieved 29 April 2024.
  6. ^ "He Noiʻi Nowelo i ka ʻIke Kuʻuna Hawaiʻi o ka ʻŌnaeao". ʻImiloa Astronomy Center. 30 December 2018. Retrieved 29 April 2024.
  7. ^ a b Heiligers, J., Fernandez, J. M., Stohlman, O. R., & Wilkie, W. K. (2019). Trajectory design for a solar-sail mission to asteroid 2016 HO3. Astrodynamics, 3(3), 231-246. https://doi.org/10.1007/s42064-019-0061-1
  8. ^ Venigalla, C., Baresi, N., Aziz, J. D., Bercovici, B., Brack, D. N., Dahir, A., De Smet, S., Fulton, J., Pellegrino, M. M., & Van wal, S. (2019). Near-Earth Asteroid Characterization and Observation (NEACO) Mission to Asteroid (469219) 2016 HO3. Journal of Spacecraft and Rockets, 56(4), 1121-1136. https://doi.org/10.2514/1.A34268
  9. ^ Jin, W., Li, F., Yan, J., Yang, X., Ye, M., Andert, T., & Peytavi, G. (2019). Simulation of global GM estimate of Asteroid (469219) 2016 HO3 for China’s future asteroid mission EPSC-DPS, Geneva, CH
  10. ^ Yan, J., Liu, L., Ye, M., Jin, W., Qiu, D., & Barriot, J.-P. (2022). A simulation of the joint estimation of the GM value and the ephemeris of the asteroid 2016 HO3. Icarus, 385. https://doi.org/10.1016/j.icarus.2022.115120
  11. ^ Zhang, X., Luo, Y., Xiao, Y., Liu, D., Guo, F., & Guo, Q. (2021). Developing Prototype Simulants for Surface Materials and Morphology of Near Earth Asteroid 2016 HO3. Space: Science & Technology, 2021. https://doi.org/10.34133/2021/9874929
  12. ^ a b Fargion, D. (2022). Mini-moon, Kamo’oalewa: The Future Space Station 44th COSPAR Scientific Assemly, https://ui.adsabs.harvard.edu/abs/2022cosp...44..215F/abstract
  13. ^ a b c d e f Sharkey, Ben; Reddy, Vishnu; Malhotra, Renu; et al. (11 November 2021). "Lunar-like silicate material forms the Earth quasi-satellite (469219) 2016 HO3 Kamoʻoalewa". Communications Earth & Environment. 2 (231). Nature: 231. arXiv:2111.06372. Bibcode:2021ComEE...2..231S. doi:10.1038/s43247-021-00303-7. S2CID 243985893.
  14. ^ a b Lea, Robert (23 April 2024). "Earth's weird 'quasi-moon' Kamo'oalewa is a fragment blasted out of big moon crater". Space.com. Retrieved 24 April 2024.
  15. ^ a b c d Castro-Cisneros, J. D., Malhotra, R., & Rosengren, A. J. (2023). Lunar ejecta origin of near-Earth asteroid Kamo'oalewa is compatible with rare orbital pathways. Commun Earth Environ, 4(1), 372. https://doi.org/10.1038/s43247-023-01031-w
  16. ^ a b c d e f Jiao, Yifei; Cheng, Bin; et al. (19 April 2024). "Asteroid Kamo'oalewa's journey from the lunar Giordano Bruno crater to Earth 1:1 resonance". Nature Astronomy. 8 (7): 819–826. arXiv:2405.20411. Bibcode:2024NatAs...8..819J. doi:10.1038/s41550-024-02258-z.
  17. ^ a b Reddy, V., Kuhn, O., Thirouin, A., Conrad, A., Malhotra, R., Sanchez, J., & Veillet, C. (2017). Ground-based Characterization of Earth Quasi Satellite (469219) 2016 HO3 49th AAS-DPS Meeting, https://ui.adsabs.harvard.edu/abs/2017DPS....4920407R/abstract
  18. ^ a b c Fenucci, M., & Novaković, B. (2021). The Role of the Yarkovsky Effect in the Long-term Dynamics of Asteroid (469219) Kamo’oalewa. The Astronomical Journal, 162(6). https://doi.org/10.3847/1538-3881/ac2902
  19. ^ a b Dermawan, B. (2019). Temporal Earth Coorbital Types of Asteroid 2016 HO3. Paper No. 012038 6th International Conference on Mathematics & Natural Sciences 2019. IOP Publishing. DOI: 10.1088/1742-6596/1127/1/012038
  20. ^ M.P.C. (2019). The MINOR PLANET CIRCULARS/MINOR PLANETS AND COMETS. In (Vol. 112435): International Astronomical Union. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/2019/MPC_20190406.pdf
  21. ^ ʻImiloa. A Hua He Inoa Calling forth a name. https://imiloahawaii.org/a-hua-he-inoa
  22. ^ "A Hua He Inoa". ʻImiloa Astronomy Center. 30 December 2018.
  23. ^ ulukau HAWAIIAN ELECTRONIC LIBRARY
  24. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 29 April 2024.
  25. ^ a b Qi, Y., & Qiao, D. (2022). Co-orbital transition of 2016 HO3. Astrodynamics, 7(1), 3-14. https://doi.org/10.1007/s42064-021-0122-0
  26. ^ Chodas, P. (2016). The Orbit and Future Motion of Earth Quasi-Satellite 2016 HO3 AAS-DPS 48th Meeting, https://ui.adsabs.harvard.edu/abs/2016DPS....4831104C/abstract
  27. ^ "Horizons Batch for May 2369 Geocentric distance". JPL Horizons. Retrieved 29 April 2024.
  28. ^ Ren, J., Wu, B., Hesse, M. A., Li, H., Liu, Y., & Wang, X. (2024). Surface dynamics of small fast-rotating asteroids: Analysis of possible regolith on asteroid 2016 HO3. Astronomy & Astrophysics, 692. https://doi.org/10.1051/0004-6361/202451407
  29. ^ Winter, O., Moraes, R., Gomes, L., Sfair, R., & Borderes-Motta, G. (2022). On the possibility that 2016 HO3 Kamo'oalewa was a piece of the Moon 44th COSPAR Scientific Assembly, https://ui.adsabs.harvard.edu/abs/2022cosp...44..274W/abstract
  30. ^ C. de la Fuente Marcos & R. de la Fuente Marcos. (2016).Asteroid (469219) 2016 HO3, the smallest and closest Earth quasi-satellite. Monthly Notices of the Royal Astronomical Society 2016 Vol. 462 Issue 4 Pages 1-16 DOI: 10.1093/mnras/stw1972
  31. ^ Venigalla, C; Baresi, N; Aziz, J; Bercovici, B; Borderes Motta, G; Brack, D; Cardoso dos Santos, J; Dahir, A; Davis, A B; Smet, S D; et al. (2019). "Near-Earth Asteroid Characterization and Observation (NEACO) Mission to Asteroid (469219) 2016 HO3" (PDF). Journal of Spacecraft and Rockets. 56 (4): 1121–1136. Bibcode:2019JSpRo..56.1121V. doi:10.2514/1.A34268. S2CID 126452156. Retrieved 29 April 2024.
  32. ^ Venigala, C; et al. (September–October 2017). "STUDENT DESIGN COMPETITION" (PDF). Space Times Magazine. Retrieved 29 April 2024.
  33. ^ Cardoso dos Santos, J; Borderes Motta, G (March 2018). "Alunos da Unesp vencem competição internacional". UNESP Notícias (Portuguese). Retrieved 29 April 2024.
  34. ^ Venigalla, C; Baresi, N; Aziz, J; Bercovici, B; Brack, D; Dahir, A; Davis, A B; Smet, S D; et al. (February 2019). "Near-Earth Asteroid Characterization and Observation (NEACO) Mission to Asteroid (469219) 2016 HO3". Journal of Spacecraft and Rockets. 56 (4): 1121–1136. Bibcode:2019JSpRo..56.1121V. doi:10.2514/1.A34268. S2CID 126452156.
  35. ^ Gibney, Elizabeth (30 April 2019). "China plans mission to Earth's pet asteroid". Nature. doi:10.1038/d41586-019-01390-5. PMID 32346150. S2CID 155198626. Retrieved 29 April 2024.
  36. ^ Zhang, Xiaojing; Huang, Jiangchuan; Wang, Tong; Huo, Zhuoxi (18–22 March 2019). ZhengHe – A Mission to a Near-Earth Asteroid and a Main Belt Comet (PDF). 50th Lunar and Planetary Science Conference. Retrieved 29 April 2024.
  37. ^ Jones, Andrew (30 June 2021). "China outlines space plans to 2025". SpaceNews. Retrieved 29 April 2024.
  38. ^ Reddy, Vishnu; Kuhn, Olga; Thirouin, Audrey; et al. (October 2017). "Ground-based Characterization of Earth Quasi Satellite (469219) 2016 HO3". AAS DPS Meeting. 49. American Astronomical Society. id.204.07. Bibcode:2017DPS....4920407R.
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