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Ryugu

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Parent: Space Age Hop 4
Expansion Funnel Raw 31 → Dedup 0 → NER 0 → Enqueued 0
1. Extracted31
2. After dedup0 (None)
3. After NER0 ()
4. Enqueued0 ()
Ryugu
Name162173 Ryugu
CaptionImage of Ryugu taken by the Hayabusa2 spacecraft in 2018
DiscovererLINEAR
Discovery date10 May 1999
Mp categoryApollo · NEO · PHA
Epoch31 May 2020
Semimajor1.1896 AU
Eccentricity0.1902
Inclination5.8839°
Perihelion0.9633 AU
Aphelion1.4159 AU
Orbital period1.30 yr
Dimensions~0.9 km (diameter)
Rotation period7.63 hours
Spectral typeCb
Abs magnitude19.2

Ryugu is a near-Earth asteroid and a potentially hazardous object of the Apollo group, classified as a dark C-type asteroid. It became a primary target for the JAXA Hayabusa2 mission, which successfully collected and returned pristine samples to Earth in 2020. The asteroid's composition and structure provide crucial insights into the early Solar System and the origins of water and organic compounds on terrestrial planets.

Discovery and naming

The asteroid was discovered on 10 May 1999 by astronomers with the LINEAR survey at the White Sands Test Facility in New Mexico. It received the provisional designation **1999 JU3** before being officially numbered 162173. In 2015, JAXA named it **Ryugu**, after the magical underwater palace, **Ryūgū-jō**, in the Japanese folktale **Urashima Tarō**. This name was chosen by the mission team because the spacecraft's goal was to "bring back a treasure" from a distant celestial object, mirroring the tale where a fisherman returns from the palace with a mysterious box.

Physical characteristics

Ryugu is a relatively small, roughly spherical body with an effective diameter of approximately 900 meters. Observations from Hayabusa2 revealed it has a distinct top-like or spinning-top shape, a common morphology for small, rapidly rotating asteroids influenced by the YORP effect. It completes one rotation every 7.63 hours. The asteroid's surface is very dark, with an albedo of only about 0.045, indicating a surface rich in carbonaceous material. Its bulk density is surprisingly low, suggesting a highly porous rubble-pile interior structure held together by weak gravity.

Composition and surface features

Spectroscopic data from ground-based telescopes and the Hayabusa2 spacecraft confirm Ryugu as a C-type asteroid, chemically primitive and similar to carbonaceous chondrite meteorites. The surface is uniformly dark and covered with numerous large boulders, with a notable scarcity of fine regolith. A prominent equatorial ridge and a large crater, later named **Urashima**, are key surface features. The lack of significant spectral variation suggests the body experienced extensive aqueous alteration in its early history, with minerals like phyllosilicates detected, pointing to past interactions with water ice.

Sample return mission

The JAXA Hayabusa2 mission, launched in December 2014, rendezvoused with Ryugu in June 2018. The spacecraft conducted extensive remote sensing, deployed the rovers **MINERVA-II** and **MASCOT**, and performed two precise touchdown maneuvers to collect surface and subsurface material. The second sample was acquired after the spacecraft fired a copper projectile from its **Small Carry-on Impactor** to excavate fresh material from beneath the surface. The sample capsule successfully landed in the Woomera Prohibited Area in South Australia in December 2020, delivering over 5.4 grams of asteroidal material to laboratories worldwide.

Scientific significance

The pristine samples from Ryugu represent some of the most primordial material ever studied, offering an unprecedented window into the conditions of the early Solar System. Initial analyses, led by teams in Japan and at NASA, confirmed the material is rich in organic compounds and water-bearing minerals, strengthening the hypothesis that carbonaceous asteroids delivered these essential ingredients to the early Earth. Studies of its composition help calibrate observations of other dark asteroids, such as Bennu, visited by NASA's OSIRIS-REx. The mission's success has profound implications for understanding planetary formation, the source of Earth's volatiles, and future planetary defense strategies against near-Earth objects.

Category:Asteroids Category:Near-Earth asteroids Category:C-type asteroids Category:Discoveries by LINEAR