162173 Ryugu

Discovery and name

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 . The asteroid was officially named "Ryugu" by the Minor Planet Center on 28 September 2015 (M.P.C. 95804). 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.

Geological history

Ryugu formed as part of an asteroid family, belonging either to Eulalia or Polana. Those asteroid families are most likely fragments of past asteroid collisions. The large number of boulders on the surface supports a catastrophic disruption of the parent body. The parent body of Ryugu probably experienced dehydration due to internal heating and must have formed in an environment without a strong magnetic field. 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), through internal failure and/or mass wasting. The geologically distinct western area ('Western bulge') is probably the result of asymmetrical internal failure. It is hoped that surface samples will help to reveal more of the geological history of the asteroid.

Ryugu is hypothesized to be an extinct comet.

Characteristics

Orbit

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. It has a minimum orbital intersection distance with Earth of 0.000638 AU, equivalent to 0.23 lunar distances.

Physical

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 km (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.

Initial images taken by the Hayabusa2 spacecraft on approach at a distance of 700 km were released on 14 June 2018. They revealed a diamond-shaped body in diameter and confirmed its retrograde motion. Between 17 and 18 June 2018, Hayabusa2 went from 330 to from Ryugu and captured a series of additional images from the closer approach. Astronomer Brian May created stereoscopic images from data collected a few days later. 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.

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 450 million tonnes. 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.

Shape

Ryugu has a round shape with an equatorial ridge, called Ryujin Dorsum. Ryugu is a spinning top-shape asteroid similar to Bennu. The ridge was shaped by strong centrifugal forces during a phase of high-speed rotation, through landslides and/or internal failure. The western side, also called the western bulge, has a distinct shape. It has a smooth surface with a sharp equatorial ridge. When modeling a high-speed rotation of present-day Ryugu, subsurface material appears structurally intact and relaxed in the western bulge, while other regions are more sensitive to structural failure. This indicates past structural failure in the western bulge (only the elements that did not experience structural failure previously are now sensitive to failure). The western bulge is bordered by the Tokoyo and Horai Fossae.

Surface

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.

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. 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. An unanticipated side effect from the Hayabusa2 thrusters revealed a coating of dark, fine-grained red material.

Craters

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. 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. The artificial crater showed a darker subsurface material. It created an Ejecta of 1 cm thickness and excavated material from up to 1 metre in depth.

Boulders

Ryugu contains 4,400 boulders with a size larger than 5 metres. Ryugu has more large boulders per surface area than Itokawa or Bennu, about one boulder larger than 20 metres 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 as an ejected boulder from a crater.

Sample analysis results

After the initial description (phase-1), part of the sample was distributed to the Hayabusa2 Initial Analysis Team, consisting of six sub-teams, and two Phase-2 curation institutes at Okayama University and JAMSTEC Kochi Institute for Core Sample Research.

In September 2022 the Hayabusa 2 initial Analysis Stone Team announced the results of their study, which includes:

• Ryugu samples contain grains that were formed at high temperatures above 1000 °C, which formed close to the Sun and were later transported towards the outer Solar System.
• The samples are soft enough to be cut with a knife and the samples preserve the magnetic field like a hard disk.
• A simulation of the formation was performed, which showed that the parent body of Ryugu accumulated 2 million years after the formation of the Solar System. It heated up to 50 °C over the next 3 million years, resulting in reactions of rocky material with water. In these reactions anhydrous silicates became hydrous silicates and iron became magnetite. The 100 km large parent body was then destroyed by a

Origin from the outer Solar System

The deuterium-rich and nitrogen-15-rich isotopic compositions of fine-grained minerals and organics suggests that the parent body of Ryugu formed in the outer Solar System. Titanium, chromium and molybdenum isotopic anomalies provide more evidence that ties Ryugu's origin to the outer Solar System.

Based on preserved magnetism in the samples researchers concluded that the parent body of Ryugu was probably formed in the darkness of nebular gas.

Volatiles

Water

The Hayabusa2 sample capsule was significantly upgraded from Hayabusa, to preserve water, light organics, gases, and other volatiles. This water was successfully sampled and preserved. Via a bulk sample (~95 milligrams), its water content was reported as 6.84 ±0.34 wt%.

Independently, a research group with a far smaller allocation (particles) reported 4-7 percent water.

The lower-than-expected water signature seen by Hayabusa2 instruments was the result of space weathering, producing a dehydrated rind.

Liquid water and aqueous alteration

Carbonated liquid water was discovered in one crystal. The water contained salts and organic matter. The liquid water was found inside a hexagonal iron sulfide crystal. The carbon dioxide was most likely CO2-ice (dry ice) inside the parent body. The water ice melted soon after the parent body formed and the CO2 dissolved into the water.

Crystals "shaped like coral reefs" were found. These crystals probably formed in liquid water, which was once present in the interior of the parent body. The parent body had a dryer surface and a wetter interior. After the collision of the parent body with a smaller asteroid, the interior and surface material were mixed. Today Ryugu has both interior and parent body surface material on its surface.

An international team found particles in the samples that contained small amounts of material unaltered by water. The team found about 0.5 vol% of anhydrous silicates. The isotopic analysis of the magnesium-rich olivine and pyroxene in the sample suggests that two types of high-temperature objects accreted onto the surface of Ryugu: amoeboid olivine aggregates and magnesium-rich chondrules.

Gas

Hayabusa2 recovered helium and other noble gases. Some terrestrial contamination entered the system, but the Ryugu components are still measurable.

Organic molecules

Aliphatic carbon-rich organics associated with coarse-grained phyllosilicates were found. Such an association has not been observed in any meteorite study and could be unique to the asteroid Ryugu.

In samples retrieved on Ryugu from the Japanese Hayabusa2 spacecraft, scientists discovered 20 different amino acids.

In March 2023, scientists announced that uracil and vitamin B3 were detected in samples retrieved from Ryugu. Unlike previous instances when nucleobases and vitamins were found in certain carbon-rich meteorites, the samples were collected directly from the asteroid and delivered to Earth in sealed capsules, which meant Earthside contamination was not possible.

Similarities to CI chondrites

NanoSIMS-based analysis at the Carnegie Institution found that the Ryugu samples contained grains older than the solar system. The abundance and composition of these presolar grains were similar when compared to presolar grains in CI chondrites. Researchers using the particle accelerator in J-PARC, used Muon beams to analyse the chemical composition of the samples. The researchers found a similar composition when compared to CI chondrites, but a 25% lower oxygen abundance relative to silicon for the Ryugu samples. The oxygen excess in meteorites might come from contamination after they entered earth's atmosphere.

Magnetic field

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.

Extreme speculation, not confirmed by Hyabusa2:

Composition and potential value

, according to the Asterank website, operated by Planetary Resources, the current value of Ryugu for mining purposes is speculated to be US$82.76 billion, and the chemical composition of the asteroid was estimated based on its class before Hayabusa2 to be of nickel, iron, cobalt, water, nitrogen, hydrogen and ammonia.

Surface features

As of August 2019, there are 13 surface features that are named by the IAU. 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 saxa, referring to the large boulders found on Ryugu's surface.

Craters

Dorsa

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

Fossae

A fossa is a ditch-like feature.

Saxa

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.

Landing sites

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

Exploration

''Hayabusa2'' mission

Main article: Hayabusa2

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.

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. This marks the first time a mission has completed a successful landing on a fast-moving asteroid body.

On 3 October 2018, the German-French Mobile Asteroid Surface Scout (MASCOT) lander successfully arrived on Ryugu, ten days after the MINERVA rovers landed. 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. The second sampling was from the subsurface, and it involved firing a large copper projectile from an altitude of 500 metres to expose pristine material. After several weeks, it touched down on 11 July 2019 to sample the subsurface material, using its sampler horn and tantalum bullet.

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. On 6 December 2020 (Australian time), a capsule containing the samples landed in Australia and after a brief search was retrieved.

Prior to the sample capsule return, the amount of sample was expected to be at least 0.1 g. The description of overall bulk sample was planned to be done by JAXA in the first six months. 5 wt% of the sample will be allocated for the detailed analysis by JAXA. 15 wt% will be allocated for initial analysis, and 10 wt% for "phase 2" analysis among Japanese research groups. Within a year, NASA (10 wt%) and international "phase 2" research groups (5 wt%) will receive their allotment. 15 wt% will be allocated for research proposals by international Announcement of Opportunity. 40 wt% of the sample will be stored unused for future analysis.

After the sample capsule returned, the amount of retrieved sample turned out to be about 5.4 g. Since it was 50 times more than anticipated, the allotment plan was adjusted to: 2 wt% to the detailed analysis by JAXA; 6 wt% for the initial analysis; 4 wt% for the "phase 2" analysis by Japanese research groups; 10 wt% for NASA; 2 wt% for the international "phase 2" research groups; 1 wt% for the public outreach; 15 wt% for the international Announcement of Opportunity; and the remaining 60 wt% will be preserved for future analysis.

In popular culture

162173 Ryugu is the setting of Daniel Suarez's novel Delta-V, describing the adventures of eight space miners who explore near-Earth asteroid Ryugu.

References

Citations

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General references

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References

1. (July 2019). "82nd Annual Meeting of The Meteoritical Society, held 7-12 July, 2019 in Sapporo, Japan".
2. (19 March 2019). "The Asteroid Was Shooting Rocks Into Space. 'Were We Safe in Orbit?'". [[The New York Times]].
3. Stephen Clark. (November 13, 2019). "Japanese sample return craft departs asteroid, heads for Earth".
4. (March 2019). "The Evolution of Ryugu's Parent Body Constrained by Hayabusa2 Imaging Observations". LPI.
5. (2022). "The Asteroid 162173 Ryugu: a Cometary Origin". The Astrophysical Journal Letters.
6. S. Sugita. (19 Mar 2019). "The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes". Science.
7. Bartels, Meghan. (10 July 2018). "Queen's Brian May Will Rock You with This Stereo Image of Asteroid Ryugu". [[Space.com]].
8. [https://www.bbc.com/news/science-environment-47633649 Hayabusa-2: Asteroid mission exploring a 'rubble pile'.] Paul Rincon, ''BBC News''. 19 March 2019.
9. (April 2019). "Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pile". Science.
10. (March 2019). "The Western Bulge of 162173 Ryugu Formed as a Result of a Rotationally Driven Deformation Process". Astrophysical Journal Letters.
11. (2020-03-19). "An artificial impact on the asteroid 162173 Ryugu formed a crater in the gravity-dominated regime". Science.
12. "DLR – MASCOT confirms what scientists have long suspected".
13. (2019-07-15). "Low thermal conductivity boulder with high porosity identified on C-type asteroid (162173) Ryugu". Nature Astronomy.
14. (2019-08-23). "Images from the surface of asteroid Ryugu show rocks similar to carbonaceous chondrite meteorites". Science.
15. "The near-Earth asteroid Ryugu – a fragile cosmic rubble pile".
16. (May 11, 2020). "Hayabusa-2 Reveals Surface of Near-Earth Asteroid Ryugu in Stunning Detail".
17. (March 2020). "The spatial distribution of impact craters on Ryugu". Icar.
18. "Apr. 24, 2019. What's new".
19. (June 25, 2019). "Asteroid explorer, Hayabusa2, reporter briefing".
20. (October 2019). "Boulder size and shape distributions on asteroid Ryugu". Icar.
21. "JAXA {{!}} Asteroid Explorer Hayabusa2 Initial Analysis Chemical Analysis Team reveals aqueous alteration and primitive composition of asteroid Ryugu".
22. "JAXA {{!}} Asteroid Explorer Hayabusa2 Initial Analysis Stone Team reveals the formation and evolution of carbonaceous asteroid Ryugu.".
23. "JAXA {{!}} Asteroid Ryugu is a drifter from the outer Solar System: Results from the Hayabusa2 Phase-2 Curation Kochi Team published in Nature Astronomy".
24. (2022). "Ryugu's nucleosynthetic heritage from the outskirts of the Solar System Science Advances (2022): eadd8141.". Science Advances.
25. (2014). "Hayabusa-returned sample curation in the Planetary Material Sample Curation Facility of JAXA". Met. & Planet. Sci..
26. (2017). "Readiness of Receiving and Curation facility for Hayabusa2 Asteroid Sample Return Mission".
27. Nittler, L. R.. (2022). "Can SIMS measurements constrain the D/H ratio of water on Ryugu?".
28. (2022). "H isotopic composition of water in Ryugu samples returned by the Hayabusa2 mission".
29. (2023). "Water in Asteroid Ryugu is Deuterium-Rich Compared to Earth and CI Chondrites".
30. (2023). "Nano-Scale Infrared and Raman Spectroscopy of Ryugu Particles".
31. (2023). "Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites". Science.
32. (2023). "Ryugu's volatiles investigated using stepped combustion and EGA methods".
33. (19 Dec 2022). "A dehydrated space-weathered skin cloaking the hydrated interior of Ryugu". Nature.
34. (Jul 12, 2023). "Hayabusa2 and Sample Science – JAXA".
35. (Aug 11, 2023). "CRISPY On The OUTSIDE, RAW On The INSIDE: IMPACT-INDUCED MELTING And FRAGMENTATION Of C-Type ASTEROID Regolith DocumentedIn A Ryugu Sample".
36. (2022). "Direct Measurement of the Composition of Aqueous Fluids from the Parent Body of Asteroid 162173 Ryugu".
37. (2022). "Early History of Ryugu's Parent Asteroid: Evidence from Return Sample".
38. "Team identifies parent body materials in Ryugu asteroid".
39. (20 Oct 2022). "First asteroid gas sample delivered by the Hayabusa2 mission: a treasure box from Ryugu". Science Advances.
40. (2023). "Noble gases and nitrogen in samples of asteroid Ryugu record its volatile sources and recent surface evolution". Science.
41. (Aug 11, 2023). "Recently Recovered Pristine Extraterrestrial Materials As Carriers of Primordially Trapped Noble Gases".
42. (2023). "Extremely High Xe Concentration in The Hayabusa2 C0209 Sample".
43. [https://www.livescience.com/20-amino-acid-types-found-on-ryugu 'Rubber-ducky' asteroid 200 million miles away holds building blocks of life] Ben Turner, LiveScience. June 9, 2022
44. Ashley Strickland. (22 March 2023). "RNA compound and vitamin B3 found in samples from near-Earth asteroid". CNN.
45. (2023-03-21). "Uracil in the carbonaceous asteroid (162173) Ryugu". Nature Communications.
46. (2022-08-01). "Presolar Stardust in Asteroid Ryugu". The Astrophysical Journal.
47. (2022-09-23). "Researchers have used beams of muons to analyze the elemental composition of Asteroid Ryugu samples".
48. (2020). "Magnetic Properties of Asteroid (162173) Ryugu". Journal of Geophysical Research: Planets.
49. http://www.asterank.com/, Value: 82.76 billion. Estimated profit: 30.07 billion
50. Jason Davis [http://www.planetary.org/blogs/jason-davis/hayabusa2-updates-sample-collection.html Hayabusa2 team sets date for sample collection, considers two touchdown sites] Planetary.org January 16, 2019
51. (January 21, 2019). "Locations on the surface of Ryugu have been named!". JAXA.
52. "RYUGU – Ryujin Dorsum".
53. "July 8, 2019. What's new".
54. (February 2, 2019). "Correction to the name of the MINERVA-II1 landing site.". JAXA.
55. [https://phys.org/news/2019-02-touchdown-japan-probe-hayabusa2-distant.html Touchdown: Japan probe Hayabusa2 lands on distant asteroid.] Kyoko Hasegawa, ''PhysOrg''. February 22, 2019.
56. (11 July 2019). "Hayabusa2 successfully collects 1st-ever subsurface samples: JAXA".
57. (2022). "Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu". Nature Astronomy.
58. 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]].
59. Rincon, Paul. (6 December 2020). "Hayabusa-2: Capsule with asteroid samples in 'perfect' shape". [[BBC News]].
60. "Hayabusa2 Project". Astromaterials Science Research Group, Extraterrestrial Sample Curation Center, JAXA.
61. 日本惑星科学会誌遊星人. (2020)
62. link. JAXA Astromaterials Science Research Group. JAXA
63. ((JAXA Hayabusa2 Project)). (16 November 2020). "Asteroid explorer, Hayabusa2, reporter briefing". JAXA.
64. link. (19 June 2021). TECH+. Minoru. Ōtsuka
65. link. JAXA. (17 June 2021)