23. August 2018
Next stop for MASCOT: A southern location, pleasant temperatures and a beautiful view

Land­ing site on the as­ter­oid Ryugu de­ter­mined

Landing of the Hayabusa2 mission on the asteroid Ryugu
Land­ing of the Hayabusa2 mis­sion on the as­ter­oid Ryugu
Image 1/3, Credit: ©JAXA, University of Tokyo & collaborators.

Landing of the Hayabusa2 mission on the asteroid Ryugu

The MAS­COT lan­der is set to land on the blue-marked land­ing el­lipse MA-9 on Ryugu. The Japanese Hayabusa2 probe will ap­proach the as­ter­oid sur­face at lo­ca­tion L07 (L08 and M04 are sub­sti­tute land­ing sites), where it will take sam­ples. The MIN­ER­VA rovers will be dropped off at the red marked land­ing N6.
Landing at the equator
Land­ing at the equa­tor
Image 2/3, Credit: ©JAXA, University of Tokyo & collaborators.

Landing at the equator

The Hayabusa2 probe will de­scend to the as­ter­oid Ryugu for sam­pling in the L08 area near the equa­tor. L07 and M04 are the re­place­ment sites.
Land­ing in the south­ern hemi­sphere
Image 3/3, Credit: ©JAXA, University of Tokyo & collaborators.

Landing in the southern hemisphere

The lo­ca­tion on the as­ter­oid, at about 315 de­grees east and 30 de­grees south, where MAS­COT will land and con­duct mea­sure­ments with four in­stru­ments, is cur­rent­ly still sim­ply called 'MA-9'.

  • Selection of the final landing site from 10 candidate sites completed
  • Temperature fluctuations between 47 and minus 63 degrees Celsius at the landing site
  • More fresh material and boulders up to 30 metres tall await MASCOT
  • Landing scheduled for 3 October 2018.
  • Focus: Space, exploration, mission

Not too hot and not too cold. Not too many boulders, nor too few. Easily accessible and scientifically exciting. Meeting the requirements that the Mobile Asteroid Surface Scout (MASCOT) team had for the landing site on the asteroid Ryugu was no easy task. "However, we have now decided on an almost perfect landing site," says Ralf Jaumann from the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) Institute of Planetary Research, who is Principal Investigator of the MASCOT landing probe and responsible for the lander's MasCam camera experiment. DLR Project Manager Tra-Mi Ho is also satisfied with the selection of the landing site: "For the operation of our lander, the chosen landing site was among the favourites from the very start." In consultation with more than 100 international and national partners, the MASCOT landing site was selected from 10 potential candidates, and announced on 23 August 2018. MASCOT's landing is scheduled for 3 October 2018. The locations at which the Hayabusa2 probe is expected to take soil samples have also been designated, as have the sites where the three MINVERVA-II rovers will be placed on the asteroid's surface.

Located at approximately 315 degrees east and 30 degrees south, the place at which MASCOT is supposed to land on the primordial celestial body and carry out measurements on the asteroid's surface using four instruments is, at the moment, still simply called 'MA-9'. The landing site area has several advantages. Firstly, it is far enough from the regions in which Hayabusa2 will descend to the surface and take soil samples – in this way, MASCOT and Hayabusa2 will not get in each other's way as they perform their activities. Secondly, the landing site lies in Ryugu's southern hemisphere, so with the data collected by Hayabusa2 at the equator and MINERVA in the northern hemisphere, scientists will be able to gain good coverage of and investigate the 950-metre-diameter asteroid.

Numerous boulders and fresh material

Temperatures are expected to reach up to 47 degrees Celsius during the asteroid day and drop to minus 63 degrees Celsius at night. This is in line with the desired framework conditions for the operation of the instruments and for the lander's battery. In the vicinity of the landing site, there are numerous boulders up to 30 metres tall, but the really big rocks are not located in the MA-9 region. Images acquired by the optical navigation camera on the Hayabusa2 probe indicate that the landing site area probably holds fresher material that had little exposure to cosmic radiation, the particle flow of solar winds, as well as interplanetary dust – and is therefore still very primordial and in an unchanged state.

Spoilt for choice

Making a final selection from 10 potential landing sites was not easy for the scientists and engineers. After all, every team of instrument experts should be able to get the working conditions and data that it expects. For example, the MicrOmega infrared hyperspectral microscope of the Institut d'Astrophysique Spatiale (IAS) would have preferred slightly cooler temperatures during the asteroid day. The MAG magnetometer of the Technical University Braunschweig would have favoured very large boulders for its measurements. By contrast, the MasCam camera and the MARA radiometer – both instruments developed by the DLR Institute of Planetary Research – enjoy almost ideal conditions for their scientific work because they have a view of boulders on the horizon and can examine fresh asteroid material. Ultimately, the conditions that the landing site offers are very favourable for the lander and all instruments on board. "From our perspective, the selected landing site means that we engineers can guide MASCOT to the asteroid's surface in the safest way possible, while the scientists can use their various instruments in the best possible way," says Tra-Mi Ho, Project Manager at the DLR Institute of Space Systems. "But we are also aware: there seem to be large boulders across most of Ryugu's surface, and barely surfaces with flat regolith. Although scientifically very interesting, this is also a challenge for a small lander and for sampling."

About the Hayabusa2 mission and MASCOT

Hayabusa2 is a JAXA - GLOB­AL (Japan Aerospace Exploration Agency; JAXA) mission to the near-Earth asteroid Ryugu. The German-French lander MASCOT on board Hayabusa2 was developed by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) and built in close cooperation with the CoRoT Spe­cial (Centre National d'Etudes Spatiales). DLR, the Institut d'Astrophysique Spatiale and the Technical University of Braunschweig have contributed the scientific experiments on board MASCOT. The MASCOT lander and its experiments are operated and controlled by DLR with support from CNES and in constant interaction with the Hayabusa2 team.

The DLR Institute of Space Systems in Bremen was responsible for developing and testing the lander together with CNES. The DLR Institute of Composite Structures and Adaptive Systems in Braunschweig was responsible for the stable structure of the lander. The DLR Robotics and Mechatronics Center in Oberpfaffenhofen developed the swing arm that allows MASCOT to hop on the asteroid. Das DLR Institute of Planetary Research in Berlin contributed the MasCam camera and the MARA radiometer. The asteroid lander is monitored and operated from the MASCOT Control Center in the Mi­cro­grav­i­ty Us­er Sup­port Cen­ter (MUSC)at the DLR site in Cologne.

  • Falk Dambowsky
    Ger­man Aerospace Cen­ter (DLR)
    Me­dia Re­la­tions
    Telephone: +49 2203 601-3959
    Fax: +49 2203 601-3249
    Linder Höhe
    51147 Cologne
  • Manuela Braun
    Ger­man Aerospace Cen­ter (DLR)
    Strat­e­gy Space R&D
    Telephone: +49 2203 601-3882
    Fax: +49 2203 601-3249
    Hansestraße 115
    51149 Köln
  • Tra-Mi Ho
    Ger­man Aerospace Cen­ter (DLR)
    In­sti­tute of Space Sys­tems
    Telephone: +49 421 24420-1171
    Robert-Hooke-Straße 7
    28359 Bremen
  • Prof.Dr. Ralf Jaumann
    Freie Uni­ver­sität Berlin
    In­sti­tute of Ge­o­log­i­cal Sci­ences
    Plan­e­tary Sci­ences and Re­mote Sens­ing
    Telephone: +49-172-2355864
    Malteserstr. 74-100
    12249 Berlin

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