162173 Ryugu

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162173 Ryugu
162173 Ryugu.jpg
Monochrome view of Ryugu[a]
Discovery [1]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date10 May 1999
(162173) Ryugu
Japanese: [ɾjɯːɡɯː]
Named after
("Dragon palace")
1999 JU3
Apollo · NEO · PHA[1][2]
Orbital characteristics[2]
Epoch 12 December 2011 (JD 2455907.5)
Uncertainty parameter 0
Observation arc30.32 yr (11,075 d)
Aphelion1.4159 AU
Perihelion0.9633 AU
1.1896 AU
1.30 yr (474 d)
0° 45m 34.56s / day
Earth MOID0.0006 AU (0.2337 LD)
Physical characteristics
Mean diameter
0.865±0.015 km[3]
0.87 km[4]
0.90±0.14 km[5]
0.92±0.12 km[6]
0.980±0.029 km[7]
1.13±0.03 km[8]
Volume0.377±0.005 km3[9]
Mass(4.50±0.06)×1011 kg[10][9]
Mean density
1.19±0.03 g cm−3[9]
Equatorial surface gravity
1/80,000 g[10]
7.627±0.007 h[7][11]
SMASS = Cg[2] · C[3] · Cb[12]
18.69±0.07 (R)[4]

162173 Ryugu, provisional designation 1999 JU3, is a near-Earth object and a potentially hazardous asteroid of the Apollo group. It measures approximately 1 kilometre (0.62 mi) in diameter and is a dark object of the rare spectral type Cb,[12] with qualities of both a C-type asteroid and a B-type asteroid. In June 2018, the Japanese spacecraft Hayabusa2 arrived at the asteroid.[13] After making measurements and taking samples, Hayabusa2 left Ryugu for Earth in November 2019[14][15] and returned the sample capsule to Earth on 5 December 2020.[15]


Discovery and name[edit]

Ryugu was discovered on 10 May 1999 by astronomers with the Lincoln Near-Earth Asteroid Research at the Lincoln Lab's ETS near Socorro, New Mexico, in the United States. It was given the provisional designation 1999 JU3.[1] The asteroid was officially named "Ryugu" by the Minor Planet Center on 28 September 2015 (M.P.C. 95804).[16] The name refers to Ryūgū-jō (Dragon Palace), a magical underwater palace in a Japanese folktale. In the story, the fisherman Urashima Tarō travels to the palace on the back of a turtle, and when he returns, he carries with him a mysterious box, much like Hayabusa2 returning with samples.[1][17]

Geological history[edit]

The origin of 162173 Ryugu may be either 495 Eulalia or 142 Polana[18]
   Sun ·    Earth ·    162173 Ryugu ·    142 Polana ·    495 Eulalia

Ryugu formed as part of an asteroid family, belonging either to Eulalia or Polana.[19] Those asteroid families are likely fragments of past asteroid collisions. The large number of boulders on the surface supports a catastrophic disruption of the parent body.[20] The parent body of Ryugu likely experienced dehydration due to internal heating[19] and must have formed in an environment without a strong magnetic field.[21] After this catastrophic disruption, part of the surface was reshaped again by the high speed rotation of the asteroid forming the equatorial ridge (Ryujin Dorsum). Only the western bulge remained as an older structure.[22] It is hoped that surface samples will help to reveal more of the geological history of the asteroid.[19]


Orbit between Earth and Mars


Ryugu orbits the Sun at a distance of 0.96–1.41 AU once every 16 months (474 days; semi-major axis of 1.19 au). Its orbit has an eccentricity of 0.19 and an inclination of 6° with respect to the ecliptic.[2] It has a minimum orbital intersection distance with Earth of 95,400 km (0.000638 au), equivalent to 0.23 lunar distances.[2]


Early analysis in 2012 by Thomas G. Müller et al. used data from a number of observatories, and suggested that the asteroid was "almost spherical", a fact that hinders precise conclusions, with retrograde rotation, an effective diameter of 0.85–0.88 kilometers, (0.528 miles) and a geometric albedo of 0.044 to 0.050. They estimated that the grain sizes of its surface materials are between 1 and 10 mm.[3]

Initial images taken by the Hayabusa2 spacecraft on approach at a distance of 700 km (430 mi) were released on 14 June 2018. They revealed a diamond shaped body and confirmed its retrograde rotation.[23] Between 17 and 18 June 2018, Hayabusa2 went from 330 to 240 km (210 to 150 mi) from Ryugu and captured a series of additional images from the closer approach.[24] Astronomer Brian May created stereoscopic images from data collected a few days later.[25] After a few months of exploration, JAXA scientists concluded that Ryugu is actually a rubble pile with about 50% of its volume being empty space.[26]

The acceleration due to gravity at the equator has been evaluated at about 0.11 mm/s2, rising to 0.15 mm/s2 at the poles. The mass of Ryugu is estimated at about 450 million tonnes.[27] The asteroid has a volume of 0.377 ± 0.005 km3 and a bulk density of 1.19 ± 0.03 g/cm3 based on the shape-model.[9]


Image sequence showing the rotation of Ryugu
Ryugu imaged in color by the ONC-T camera on board Hayabusa2

Ryugu has a round shape with an equatorial ridge, called Ryujin Dorsum. Ryugu is a spinning top-shape asteroid similar to Bennu. The ridge is shaped by strong centrifugal forces. The western side has a different shape compared to the rest of the asteroid. The western side, also called the western bulge has a smooth surface with a sharp equatorial ridge. The models showed that subsurface material is structurally intact and relaxed in the western bulge, while other regions are more sensitive to structural failure.[22] The eastern and western side of Ryugu are bordered by the Tokoyo and Horai Fossae. The structural differences are due to structural changes in the history of the asteroids. Landslides and internal alternations reshaped the asteroid during a phase of high speed rotation. The western bulge is the region that was not affected by these reshaping forces.[28]


Simulant of the surface of Ryugu produced by the University of Tokyo
Images of the asteroid's surface made with Hayabusa2.

Observations from Hayabusa2 showed that the surface of Ryugu is very young and has an age of 8.9 ± 2.5 million years based on the data collected from the artificial crater that was created with an explosive by Hayabusa2.[12][29]

The surface of Ryugu is porous and contains no or very little dust. The measurements with the radiometer on board of MASCOT, which is called MARA, showed a low thermal conductivity of the boulders. This was an in situ measurement of the high porosity of the boulder material. This result showed that most meteorites originating from C-type asteroids are too fragile to survive the entry into Earth's atmosphere.[30][31] The images from the camera of MASCOT, which is called MASCam, showed that surface of Ryugu contains two different almost black types of rock with little internal cohesion, but no dust was detected. One type of rocky material on the surface is brighter with a smooth surface and sharp edges. The other type of rock is dark with a cauliflower-like, crumbly surface. The dark type of rock has a dark matrix with small, bright, spectrally different inclusions. The inclusions appear similar to CI chondrites.[32][33] An unanticipated side effect from the Hyabusa2 thrusters revealed a coating of dark, fine-grained red material.[34]


Ryugu has 77 craters on the surface. Ryugu shows variations of crater density that cannot be explained by randomness of cratering. There are more craters at lower latitudes and fewer at higher latitudes, and fewer craters in the western bulge (160°E - 290°E) than in the region around the meridian (300°E - 30°E). This variation is seen as evidence of a complicated geologic history of Ryugu.[35] The surface has one artificial crater, which was intentionally formed by the Small Carry-on Impactor (SCI), which was deployed by Hayabusa2. SCI fired a 2 kg copper mass onto the surface of Ryugu on 5 April, 2019.[36] The artificial crater showed a darker sub-surface material. It created an ejecta of 1 cm thickness and excavated material from up to 1 meter in depth.[37]


Ryugu contains 4400 boulders with a size larger than 5 meters. Ryugu has more large boulders per surface area than Itokawa or Bennu, about one boulder larger than 20 meters per 50 km2. The boulders resemble laboratory impact fragments. The high number of boulders is explained with a catastrophic disruption of Ryugu's larger parent body. The largest boulder, called Otohime has a size of ~160 × 120 × 70 m and is too large to be explained with an ejected boulder from a crater.[20]

Magnetic field[edit]

No magnetic field was detected near Ryugu on a global or local scale. This measurement is based on the magnetometer on board of MASCOT, which is called MasMag. This shows that Ryugu does not generate a magnetic field, indicating that the larger body from which it was fragmented was not generated in an environment with a strong magnetic field. This result cannot be generalized for C-type asteroids, however, because the surface of Ryugu seems to have been recreated in a catastrophic disruption.[21]

Surface features[edit]

As of August 2019, there are 13 surface features that are named by the IAU.[38][39] The three landing sites are not officially confirmed but are referred to by specific names in media by JAXA. The theme of features on Ryugu is "children's stories." Ryugu was the first object to introduce the feature type known as the Saxum, referring to the large boulders found on Ryugu's surface.


Feature Named after
Brabo Silvius Brabo[40]
Cendrillon Cendrillon
Kibidango Kibi dango featured in Momotaro
Kintaro Kintaro
Kolobok Kolobok
Momotaro Momotaro
Urashima Urashima Taro


A dorsum is a ridge. There is a single dorsum on Ryugu.

Feature Named after
Ryujin Dorsum Ryujin


A fossa is a ditch-like feature.

Feature Named after
Horai Fossa Penglai
Tokoyo Fossa Tokoyo


A saxum is a large boulder. Ryugu is the first astronomical object with them being named. Two boulders have been named "Styx" and "Small Styx" unofficially by the JAXA team, it is unknown if these names will be submitted for IAU approval. Both names refer to the River Styx.[41]

Feature Named after
Catafo Saxum Catafo, from Cajun folktales [39]
Ejima Saxum Ejima, the location where Urashima Taro rescued the turtle [39]
Otohime Saxum Otohime

Landing sites[edit]

JAXA has given informal names to the specific landing and collection sites.

Feature Named after Notes
Alice's Wonderland Alice in Wonderland MASCOT landing site
Tritonis Lake Tritonis MINERVA-II1 landing site, initially referred to as "Trinitas," as of February 2019 this has been rectified.
Tamatebako Tamatebako Site of first sample collection
Uchide-no-Kozuchi Uchide no kozuchi Site of second sample collection

Hayabusa2 mission[edit]

Animation of Hayabusa2's orbit from 3 December 2014
  Hayabusa2   162173 Ryugu   Earth   Sun

The Japan Aerospace Exploration Agency (JAXA) spacecraft Hayabusa2 was launched in December 2014 and successfully arrived at the asteroid on 27 June 2018. It returned material from the asteroid to Earth in December 2020.[42]

The Hayabusa2 mission includes four rovers with various scientific instruments. The rovers are named HIBOU (aka Rover-1A), OWL (aka Rover-1B), MASCOT and Rover-2 (aka MINERVA-II-2). On 21 September 2018, the first two of these rovers, HIBOU and OWL (together the MINERVA-II-1 rovers) which hop around the surface of the asteroid, were released from Hayabusa2.[43] This marks the first time a mission has completed a successful landing on a fast-moving asteroid body.[44]

On 3 October 2018, the German-French Mobile Asteroid Surface Scout (MASCOT) lander successfully arrived on Ryugu, 10 days after the MINERVA rovers landed.[45] Its mission was short-lived, as was planned; the lander had only 16 hours of battery power and no way to recharge.

Hayabusa2 touched down briefly on February 22, 2019 on Ryugu, fired a small tantalum projectile into the surface to collect the cloud of surface debris within the sampling horn, and then moved back to its holding position.[46] The second sampling was from the sub-surface, and it involved firing a large copper projectile from an altitude of 500 meters to expose pristine material. After several weeks, it touched down on 11 July 2019 to sample the sub-surface material, using its sampler horn and tantalum bullet.[47]

The last rover, Rover-2 or MINERVA-II-2, failed before release from the Hayabusa2 orbiter. It was deployed anyway on 2 October 2019 in orbit around Ryugu to perform gravitational measurements. It impacted the asteroid a few days after release.

On 13 November 2019, commands were sent to Hayabusa2 to leave Ryugu and begin its journey back to Earth.[14] On 6 December 2020 (Australian time), a capsule containing the samples landed in Australia and after a brief search was retrieved.[15][48]

The amount of sample was expected to be over 100 mg.[49] Early estimate of the sample after the sample capsule return is about 5400 mg.[50] As of December 2020, description of overall bulk sample is planned to be done by JAXA in the first six months.[51][52][53] 5 wt% of the sample will be allocated for the detailed analysis by JAXA.[51] 15 wt% will be allocated for initial analysis, and 10 wt% for "phase 2" analysis among Japanese research groups.[51] Within a year, NASA (10 wt%) and international "phase 2" research groups (5 wt%) will receive their allotment.[51] 15 wt% will be allocated for research proposals by international Announcement of Opportunity.[51] 40 wt% of the sample will be stored unused for future analysis.[51]

See also[edit]



  1. ^ Photograph of the full disc of 162173 Ryugu by the Optical Navigation Camera – Telescopic (ONC-T) instrument aboard the Hayabusa2 spacecraft. The photograph was taken on 26 June 2018, at a distance of 20 kilometres (12 miles) from the asteroid's surface.


  1. ^ a b c d e f "162173 Ryugu (1999 JU3)". Minor Planet Center. Retrieved 30 October 2018.
  2. ^ a b c d e f "JPL Small-Body Database Browser: 162173 Ryugu (1999 JU3)" (2016-08-09 last obs.). Jet Propulsion Laboratory. Retrieved 30 October 2018.
  3. ^ a b c d e Müller, T. G.; Durech, J.; Ishiguro, M.; Mueller, M.; Krühler, T.; Yang, H.; et al. (March 2017). "Hayabusa-2 mission target asteroid 162173 Ryugu (1999 JU3): Searching for the object's spin-axis orientation". Astronomy and Astrophysics. 599: 25. arXiv:1611.05625. Bibcode:2017A&A...599A.103M. doi:10.1051/0004-6361/201629134. S2CID 73519172.
  4. ^ a b c Kim, Myung-Jin; Choi, Young-Jun; Moon, Hong-Kyu; Ishiguro, Masateru; Mottola, Stefano; Kaplan, Murat; et al. (February 2013). "Optical observations of NEA 162173 (1999 JU3) during the 2011-2012 apparition". Astronomy and Astrophysics. 550: 4. arXiv:1302.4542. Bibcode:2013A&A...550L..11K. doi:10.1051/0004-6361/201220673. S2CID 54684944.
  5. ^ a b Campins, H.; Emery, J. P.; Kelley, M.; Fernández, Y.; Licandro, J.; Delbó, M.; et al. (August 2009). "Spitzer observations of spacecraft target 162173 (1999 JU3)". Astronomy and Astrophysics. 503 (2): L17–L20. arXiv:0908.0796. Bibcode:2009A&A...503L..17C. doi:10.1051/0004-6361/200912374. S2CID 16329091.
  6. ^ a b c Hasegawa, S.; Müller, T. G.; Kawakami, K.; Kasuga, T.; Wada, T.; Ita, Y.; et al. (December 2008). "Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target 162173 1999 JU3 from AKARI and Subaru Observations". Publications of the Astronomical Society of Japan. 60 (SP2): S399––S405. Bibcode:2008PASJ...60S.399H. doi:10.1093/pasj/60.sp2.S399.
  7. ^ a b c d Abe, M.; Kawakami, K.; Hasegawa, S.; Kuroda, D.; Yoshikawa, M.; Kasuga, T.; et al. (March 2008). "Ground-based Observational Campaign for Asteroid 162173 1999 JU3" (PDF). Lunar and Planetary Science (1391): 1594. Bibcode:2008LPI....39.1594A. Retrieved 30 October 2018.
  8. ^ a b Yu, Liang-Liang; Ji, Jiang-Hui; Wang, Su (July 2014). "Investigation of Thermal Inertia and Surface Properties for Near-earth Asteroid (162173) 1999 JU3". Chinese Astronomy and Astrophysics. 38 (3): 317–329. arXiv:1805.05244. Bibcode:2014ChA&A..38..317L. doi:10.1016/j.chinastron.2014.07.008. S2CID 119186039.
  9. ^ a b c d Watanabe, S.; Hirabayashi, M.; Hirata, N.; Hirata, N.; Shimaki, Y.; Ikeda, H.; Tatsumi, E.; Yoshikawa, M.; Kikuchi, S.; Yabuta, H.; Nakamura, T. (March 2019). "High Porosity Nature of the Top-Shape C-Type Asteroid 162173 Ryugu as Observed by Hayabusa2". LPI (2132): 1265. Bibcode:2019LPI....50.1265W.
  10. ^ a b Clark, Stephen (6 September 2018). "Hayabusa 2 team sets dates for asteroid landings – Spaceflight Now". spaceflightnow.com. Retrieved 7 September 2018.
  11. ^ "LCDB Data for (162173) Ryugu". Asteroid Lightcurve Database (LCDB). Retrieved 30 October 2018.
  12. ^ a b c Sugita, S.; Honda, R.; Morota, T.; Kameda, S.; Sawada, H.; Tatsumi, E.; Honda, C.; Yokota, Y.; Yamada, M.; Kouyama, T.; Sakatani, N. (July 2019). "Ryugu's Parent-Body Processes Estimated from Hayabusa2 Multi-Band Optical Observations". LPICo. 82 (2157): 6366. Bibcode:2019LPICo2157.6366S. ISSN 0161-5297.
  13. ^ Chang, Kenneth; Stirone, Shannon (19 March 2019). "The Asteroid Was Shooting Rocks Into Space. 'Were We Safe in Orbit?'". The New York Times. Retrieved 21 March 2019. NASA's Osiris-Rex and Japan's Hayabusa2 spacecraft reached the space rocks they are surveying last year, and scientists from both teams announced early findings on Tuesday.
  14. ^ a b Stephen Clark (13 November 2019). "Japanese sample return craft departs asteroid, heads for Earth"./
  15. ^ a b c Chang, Kenneth (5 December 2020). "Japan's Journey to an Asteroid Ends With a Hunt in Australia's Outback - The Hayabusa2 mission cements Japan's role in exploring the solar system, but finding its asteroid cargo presents one last challenge". The New York Times. Retrieved 5 December 2020.
  16. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 30 October 2018.
  17. ^ "Name Selection of Asteroid 1999 JU3 Target of the Asteroid Explorer "Hayabusa2"" (Press release). JAXA. 5 October 2015. Retrieved 30 October 2018.
  18. ^ S. Sugita; et al. (19 March 2019). "The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes". Science. 364 (6437): eaaw0422. doi:10.1126/science.aaw0422. hdl:1893/29363. PMC 7370239. PMID 30890587.
  19. ^ a b c Sugita, S.; Honda, R.; Morota, T.; Kameda, S.; Honda, C.; Yokota, Y.; Yamada, M.; Kouyama, T.; Sakatani, N.; Suzuki, H.; Yoshioka, K. (March 2019). "The Evolution of Ryugu's Parent Body Constrained by Hayabusa2 Imaging Observations". LPI (2132): 2622. Bibcode:2019LPI....50.2622S.
  20. ^ a b Michikami, Tatsuhiro; Honda, Chikatoshi; Miyamoto, Hideaki; Hirabayashi, Masatoshi; Hagermann, Axel; Irie, Terunori; Nomura, Keita; Ernst, Carolyn M.; Kawamura, Masaki; Sugimoto, Kiichi; Tatsumi, Eri (October 2019). "Boulder size and shape distributions on asteroid Ryugu". Icar. 331: 179–191. Bibcode:2019Icar..331..179M. doi:10.1016/j.icarus.2019.05.019. ISSN 0019-1035.
  21. ^ a b Hercik, David; Auster, Hans-Ulrich; Constantinescu, Dragos; Blum, Jürgen; Fornaçon, Karl-Heinz; Fujimoto, Masaki; Gebauer, Kathrin; Grundmann, Jan-Thimo; Güttler, Carsten; Hillenmaier, Olaf; Ho, Tra-Mi (2020). "Magnetic Properties of Asteroid (162173) Ryugu". Journal of Geophysical Research: Planets. 125 (1): e2019JE006035. doi:10.1029/2019JE006035. ISSN 2169-9100.
  22. ^ a b Hirabayashi, Masatoshi; Tatsumi, Eri; Miyamoto, Hideaki; Komatsu, Goro; Sugita, Seiji; Watanabe, Sei-ichiro; Scheeres, Daniel J.; Barnouin, Olivier S.; Michel, Patrick; Honda, Chikatoshi; Michikami, Tatsuhiro (March 2019). "The Western Bulge of 162173 Ryugu Formed as a Result of a Rotationally Driven Deformation Process". Astrophysical Journal Letters. 874 (1): L10. arXiv:1904.03480. Bibcode:2019ApJ...874L..10H. doi:10.3847/2041-8213/ab0e8b. ISSN 0004-637X. S2CID 102350610.
  23. ^ "From a distance of about 700km, Ryugu's rotation was observed". JAXA. 16 June 2016. Retrieved 30 October 2018.
  24. ^ Plait, Phil (20 June 2018). "Asteroid Ryugu Starts to Come Into Focus". SyFy Wire. Retrieved 30 October 2018.
  25. ^ Bartels, Meghan (10 July 2018). "Queen's Brian May Will Rock You with This Stereo Image of Asteroid Ryugu". Space.com. Retrieved 24 December 2018.
  26. ^ Hayabusa-2: Asteroid mission exploring a 'rubble pile'. Paul Rincon, BBC News. 19 March 2019.
  27. ^ Operation status for the asteroid explorer, Hayabusa2, in the vicinity of Ryugu (PDF), JAXA, 5 September 2018, retrieved 30 October 2018
  28. ^ "May 13, 2019. What's new". JAXA Hayabusa2 project (in Japanese). Retrieved 9 March 2020.
  29. ^ Arakawa, M.; Saiki, T.; Wada, K.; Ogawa, K.; Kadono, T.; Shirai, K.; Sawada, H.; Ishibashi, K.; Honda, R.; Sakatani, N.; Iijima, Y. (19 March 2020). "An artificial impact on the asteroid 162173 Ryugu formed a crater in the gravity-dominated regime". Science. 368 (6486): 67–71. doi:10.1126/science.aaz1701. ISSN 0036-8075. PMID 32193363. S2CID 214591738.
  30. ^ "DLR - MASCOT confirms what scientists have long suspected". DLRARTICLE DLR Portal. Retrieved 7 March 2020.
  31. ^ Grott, M.; Knollenberg, J.; Hamm, M.; Ogawa, K.; Jaumann, R.; Otto, K. A.; Delbo, M.; Michel, P.; Biele, J.; Neumann, W.; Knapmeyer, M. (15 July 2019). "Low thermal conductivity boulder with high porosity identified on C-type asteroid (162173) Ryugu". Nature Astronomy. 3 (11): 971–976. doi:10.1038/s41550-019-0832-x. ISSN 2397-3366. S2CID 197402876.
  32. ^ Jaumann, R.; Schmitz, N.; Ho, T.-M.; Schröder, S. E.; Otto, K. A.; Stephan, K.; Elgner, S.; Krohn, K.; Preusker, F.; Scholten, F.; Biele, J. (23 August 2019). "Images from the surface of asteroid Ryugu show rocks similar to carbonaceous chondrite meteorites". Science. 365 (6455): 817–820. doi:10.1126/science.aaw8627. ISSN 0036-8075. PMID 31439797. S2CID 201616571.
  33. ^ "The near-Earth asteroid Ryugu – a fragile cosmic rubble pile". DLRARTICLE DLR Portal. Retrieved 7 March 2020.
  34. ^ "Hayabusa-2 Reveals Surface of Near-Earth Asteroid Ryugu in Stunning Detail". Sci News. 11 May 2020. Retrieved 12 May 2020.
  35. ^ Hirata, Naoyuki; Morota, Tomokatsu; Cho, Yuichiro; Kanamaru, Masanori; Watanabe, Sei-ichiro; Sugita, Seiji; Hirata, Naru; Yamamoto, Yukio; Noguchi, Rina; Shimaki, Yuri; Tatsumi, Eri (March 2020). "The spatial distribution of impact craters on Ryugu". Icar. 338: 113527. Bibcode:2020Icar..33813527H. doi:10.1016/j.icarus.2019.113527. ISSN 0019-1035.
  36. ^ "Apr. 24, 2019. What's new". JAXA Hayabusa2 project (in Japanese). Retrieved 9 March 2020.
  37. ^ "Asteroid explorer, Hayabusa2, reporter briefing" (PDF). JAXA Hayabusa2 Project. 25 June 2019. Retrieved 9 March 2020.
  38. ^ Jason Davis Hayabusa2 team sets date for sample collection, considers two touchdown sites Planetary.org January 16, 2019
  39. ^ a b c http://www.hayabusa2.jaxa.jp/en/topics/20190121e_Nomenclature/
  40. ^ "Jan. 21, 2019. What's new". JAXA Hayabusa2 project (in Japanese). Retrieved 7 September 2019. The brave young man who defeated a giant
  41. ^ "July 8, 2019. What's new". JAXA Hayabusa2 project (in Japanese). Retrieved 7 September 2019.
  42. ^ "Current status of the asteroid explorer, Hayabusa2, leading up to arrival at asteroid Ryugu in 2018" (PDF). JAXA. 14 June 2016. Retrieved 30 October 2018.
  43. ^ Wall, Mike (21 September 2018). "Japanese Probe Deploys Tiny Hopping Robots Toward Big Asteroid Ryugu". space.com. Retrieved 30 October 2018.
  44. ^ Yoshimitsu, Tetsuo; Kubota, Takashi; Tsuda, Yuichi; Yoshikawa, Makoto (23 September 2015). "MINERVA-II1: Successful image capture, landing on Ryugu and hop!". JAXA Hayabusa2 Project. JAXA. Retrieved 30 October 2018.
  45. ^ "Touchdown! Japan space probe lands new robot on asteroid". phys.org. 3 October 2018. Retrieved 30 October 2018.
  46. ^ Touchdown: Japan probe Hayabusa2 lands on distant asteroid. Kyoko Hasegawa, PhysOrg. February 22, 2019.
  47. ^ "Hayabusa2 successfully collects 1st-ever subsurface samples: JAXA". Kyodo News. 11 July 2019. Retrieved 15 July 2019.
  48. ^ Rincon, Paul (6 December 2020). "Hayabusa-2: Capsule with asteroid samples in 'perfect' shape". BBC News. Retrieved 6 December 2020.
  49. ^ "Hayabusa2 Project". Astromaterials Science Research Group, Extraterrestrial Sample Curation Center, JAXA. Archived from the original on 25 September 2018. Retrieved 10 December 2020.
  50. ^ 小惑星探査機「はやぶさ2」が採取した小惑星Ryugu(リュウグウ)サンプルは約5.4グラム (in Japanese). JAXA. 18 December 2020. Retrieved 7 January 2021.
  51. ^ a b c d e f 安部 正真; 橘 省吾; 小林 桂; 伊藤 元雄; 渡邊 誠一郎 (2020). 火の鳥「はやぶさ」未来編 その20 ~小惑星リュウグウからの リターンサンプル分析の全体像~. 日本惑星科学会誌遊星人 (in Japanese). 29 (1): 28–37. doi:10.14909/yuseijin.29.1_28.
  52. ^ JAXA Astromaterials Science Research Group. はやぶさ2試料の初期記載・分析 (PDF) (in Japanese). JAXA. Retrieved 10 December 2020.
  53. ^ JAXA Hayabusa2 Project (16 November 2020). "Asteroid explorer, Hayabusa2, reporter briefing" (PDF). JAXA. Retrieved 10 December 2020.


External links[edit]

162173 Ryugu at the JPL Small-Body Database Edit this at Wikidata