The Hayabusa2 mis­sion

In­ves­ti­gat­ing a near-Earth as­ter­oid

On 3 December 2014, the Japanese space probe Hayabusa2 embarked on a sample return mission to the C-type asteroid (162173) Ryugu (formerly designated 1999 JU3). It is operated by the Japan Aerospace Exploration Agency (JAXA) and carried the MASCOT (Mobile Asteroid Surface Scout) lander built by the German Aerospace Center (DLR) in collaboration with the French Space Agency (CNES) and the Japanese space agency (JAXA). Hayabusa2 is the immediate follow-on mission of the Hayabusa mission, which saw the first probe return to Earth with samples taken from asteroid Itokawa in June 2010. At that time, the DLR Institute of Planetary Research also investigated the rare particles.

The aim of the Hayabusa2 mission is to learn more about the origin and evolution of the Solar System. Like comets, asteroids are some of the most primordial celestial bodies. Researching asteroids gives us a glimpse into our cosmic past. Near-Earth Objects (NEOs), such as Ryugu, also pose a potential threat to Earth and therefore need to be investigated to learn about and reduce their threat.

This unique mission involves:

  • observation and mapping the asteroid from a distance,
  • providing measurements of the asteroid,
  • depositing the first measurement laboratory (MASCOT) capable of moving on an asteroid,
  • conducting on-site experiments and reference measurements at multiple locations, and
  • returning samples of the asteroid to Earth.

Hayabusa2 and MASCOT worked together as a team: Hayabusa2 provided the necessary data so that a suitable landing place could be found for MASCOT, whereas MASCOT carried out experiments on the asteroid's surface and provided data on materials and the surrounding area to find a location to gather soil samples. For this, Hayabusa2 will lightly touch the asteroid's surface in order to gather material, which it will then bring back to Earth.

Big challenges for a small lander

The low gravitational force of the asteroid, which amounts to just one 60,000th of the gravitational force on Earth, presented a challenge for the mission. This force is insufficient to 'pull' the lander out of the Hayabusa probe. As such, MASCOT was pushed out of its holder by a spring mechanism and fell to Ryugu from a height of approximately 60 metres. Had this happened too quickly, then MASCOT could have bounced off the asteroid's surface. The lander's 'hopping' on the asteroid from site to site was programmed from start to finish so that it did not reach escape velocity. The escape velocity from Ryugu is calculated to be 38 centimetres per second. By way of comparison, the escape velocity from Earth is 11.2 kilometres per second, and that from the Moon is 2.3 kilometres per second.

The mineralogical and geological composition of the asteroid’s surface and its surface temperature and magnetic field were investigated with a radiometer and a camera developed by DLR, as well as a spectrometer of the Institut d'Astrophysique Spatiale and a magnetometer by TU Braunschweig.

The duo reached Ryugu on 27 June 2018. On 3 October 2018 at 03:58 (CEST) MASCOT separated from the Japanese Hayabusa2 spacecraft, and landed and made contact wit Ryugu approximately 20 minutes later. MASCOT was operational for over 17 hours, during which it collected data from the asteroid's surface. Hayabusa2 will return samples to Earth in 2020.

DLR participation in the Hayabusa2 mission

The DLR Institute of Space Systems, based in Bremen, together with CNES (Centre national d'études spatiales), designed, manufactured and tested the lander in the Institute's laboratories under space conditions, for example on a shaker, in the thermal vacuum chamber and during parabolic flights in the drop tower at the Centre of Applied Space Technology and Microgravity (ZARM). The DLR Institute of Composite Structures and Adaptive Systems in Braunschweig was responsible for the lander's stable structure. The DLR Robotics and Mechatronics Center in Oberpfaffenhofen developed the arm that allows MASCOT to ‘hop’ on the asteroid. The DLR Institute of Planetary Research in Berlin contributed to the MASCAM camera and the MARA radiometer. The MASCOT lander will be monitored and operated from the DLR control centre at the Microgravity User Support Center (MUSC) in Cologne.

CNES contributed the power subsystem to MASCOT, as well as a part of the telecommunications system, which included the development of antennas, and the agency will assume responsibility for the descent and landing mission analyses.

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Falk Dambowsky

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Dr. Tra-Mi Ho

German Aerospace Center (DLR)
Institute of Space Systems
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