LLMpediaThe first transparent, open encyclopedia generated by LLMs

Hayabusa2

Generated by DeepSeek V3.2
Note: This article was automatically generated by a large language model (LLM) from purely parametric knowledge (no retrieval). It may contain inaccuracies or hallucinations. This encyclopedia is part of a research project currently under review.
Article Genealogy
Parent: Space Age Hop 4
Expansion Funnel Raw 41 → Dedup 0 → NER 0 → Enqueued 0
1. Extracted41
2. After dedup0 (None)
3. After NER0 ()
4. Enqueued0 ()
Hayabusa2
NameHayabusa2
Mission typeAsteroid sample-return
OperatorJapan Aerospace Exploration Agency
COSPAR ID2014-076A
SATCAT40319
Mission durationPlanned: 6 years, Elapsed: 7 years, 10 months, 24 days
SpacecraftHayabusa2
ManufacturerNEC, JAXA
Launch mass609 kg
Dry mass490 kg
Power2.6 kW (at 1 AU)
Launch date3 December 2014, 04:22:04 UTC
Launch rocketH-IIA 202
Launch siteTanegashima Space Center
Deployed fromH-IIA
Deployment date3 December 2014
Landing date5 December 2020
Recovered byJAXA
Recovery date6 December 2020
Landing siteWoomera Test Range
Orbit reference162173 Ryugu
Orbit regimeHeliocentric orbit
Apsishelion
Insignia captionMission logo

Hayabusa2 is an ambitious asteroid sample-return mission developed by the Japan Aerospace Exploration Agency. Building upon the legacy of the original Hayabusa mission, it targeted the carbonaceous near-Earth object 162173 Ryugu. The spacecraft successfully collected subsurface material and returned these pristine samples to Earth in December 2020, providing unprecedented insights into the early Solar System.

Overview

Launched aboard an H-IIA rocket from the Tanegashima Space Center, the mission was a cornerstone of Japan's planetary exploration program. The project involved extensive international collaboration, with instruments contributed by teams from Germany, France, and the United States. Operations were managed by JAXA's Institute of Space and Astronautical Science, with project scientist Makoto Yoshikawa playing a key leadership role.

Mission objectives

The primary goal was to obtain detailed data on 162173 Ryugu and return surface and subsurface samples to Earth for laboratory analysis. Scientific objectives included characterizing the asteroid's physical properties, composition, and geological history to understand the role of such bodies in delivering water and organic materials to the early Earth. The mission also aimed to demonstrate advanced technologies, such as precise navigation and a novel impactor system, for future deep-space exploration.

Spacecraft design

The spacecraft inherited and improved upon the design of its predecessor, Hayabusa. It was equipped with four primary ion thruster engines for efficient deep-space propulsion and a sophisticated guidance system featuring optical navigation cameras. Key payloads included the Small Carry-on Impactor (SCI) to excavate subsurface material, the Mobile Asteroid Surface Scout (MASCOT) lander provided by DLR and CNES, and three miniature MINERVA-II rovers. The sample collection system utilized a projectile and horn mechanism to capture ejecta during brief touchdowns.

Mission timeline and events

Following its launch in late 2014, the spacecraft performed an Earth swing-by in 2015 to gain momentum. It arrived at 162173 Ryugu in June 2018, commencing a detailed remote sensing survey. In 2019, it executed two successful sample collection touchdowns and deployed the SCI to create an artificial crater. The Mobile Asteroid Surface Scout and rovers conducted in-situ surface studies. After departure in November 2019, the return capsule re-entered Earth's atmosphere and landed at the Woomera Test Range in South Australia in December 2020.

Sample analysis and scientific results

Initial analysis at the Extraterrestrial Sample Curation Center in Sagamihara confirmed the presence of abundant hydrated minerals and organic matter. Studies published in journals like Science (journal) and Nature Astronomy revealed that 162173 Ryugu's material is among the most primitive ever studied, closely resembling CI chondrite meteorites. Findings indicated the asteroid formed from rubble-pile remnants of a larger parent body that experienced aqueous alteration, providing crucial evidence for the distribution of prebiotic materials in the inner Solar System.

Legacy and future missions

The mission's success cemented JAXA's leadership in sample-return technology and asteroid science. Its methods directly inform the upcoming Martian Moons eXploration (MMX) mission to Phobos (moon) and Deimos (moon). The returned samples continue to be analyzed by global teams, with portions allocated to NASA and other international partners. The mission also demonstrated operational techniques critical for future planetary defense initiatives, such as the Double Asteroid Redirection Test (DART).

Category:Japan Aerospace Exploration Agency Category:Asteroid spacecraft Category:Sample-return missions Category:Spacecraft launched in 2014