1. October 2018

De­scent in­to the un­known: MAS­COT starts the fi­nal count­down for its as­ter­oid land­ing

Asteroid lander MASCOT on board the Hayabusa2 space probe
As­ter­oid lan­der MAS­COT on board the Hayabusa2 space probe
Image 1/7, Credit: DLR (CC BY-NC-ND 3.0)

Asteroid lander MASCOT on board the Hayabusa2 space probe

The Japanese Hayabusa2 space probe has com­plet­ed a 3200-mil­lion-kilo­me­tre long jour­ney car­ry­ing the Ger­man-French lan­der MAS­COT (Mo­bile As­ter­oid Sur­face Scout).
The MASCOT control centre
A look in­to the MAS­COT con­trol cen­tre
Image 2/7, Credit: DLR (CC BY-NC-ND 3.0)

A look into the MASCOT control centre

The as­ter­oid lan­der MAS­COT is mon­i­tored and op­er­at­ed from the Mi­cro­grav­i­ty Us­er Sup­port Cen­ter (MUSC) in Cologne.
The landing site called 'MA-9'
Land­ing on the south­ern hemi­sphere
Image 3/7, Credit: c

Landing on the southern hemisphere

At this mo­ment, the land­ing site, lo­cat­ed at 315 de­grees east and 30 de­grees south, is still sim­ply called 'MA-9'.
Asteroid lander MASCOT
As­ter­oid lan­der MAS­COT
Image 4/7, Credit: DLR (CC BY-NC-ND 3.0)

Asteroid lander MASCOT

A to­tal of four in­stru­ments are in­stalled with­in the 30 x 30 x 20-cen­time­tre lan­der. A DLR ra­diome­ter and cam­era, to­geth­er with a spec­trom­e­ter from the In­sti­tut d'As­tro­physique Spa­tiale and a mag­ne­tome­ter from the TU Braun­schweig, are set to ex­am­ine the min­er­alog­i­cal and ge­o­log­i­cal com­po­si­tion of the as­ter­oid’s sur­face and gauge its sur­face tem­per­a­ture as well as the as­ter­oid’s mag­net­ic field. A built-in swing arm gives MAS­COT the re­quired propul­sion to make jump­ing ma­noeu­vres over the sur­face.
Landing sites for the Hayabusa2-Mission on the asteroid Ryugu
Land­ing sites for the Hayabusa2-Mis­sion on the as­ter­oid Ryugu
Image 5/7, Credit: JAXA, University of Tokyo & collaborators

Landing sites for the Hayabusa2-Mission on the asteroid Ryugu

The lan­der MAS­COT will land on Ryugu with­in the el­lipse-shaped land­ing site MA-9 marked in blue. The Japanese Hayabusa2 space probe will ap­proach the as­ter­oid’s sur­face and take sam­ples from the ar­eas L07, L08 and M04. The MIN­ER­VA rovers were de­ployed at the land­ing site N6 marked in red.
Image of the Ryugu asteroid from a distance of six kilometres
Close to the Ryugu as­ter­oid
Image 6/7, Credit: JAXA, University of Tokyo, Kochi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, University of Aizu, AIST, Kobe University, Auburn University.

Close to the Ryugu asteroid

On 20 Ju­ly 2018, the Op­ti­cal Nav­i­ga­tion Cam­era – Tele­scop­ic (ONC-T) of the Japanese Hayabusa2 space­craft – took this im­age of as­ter­oid Ryugu from a dis­tance of six kilo­me­tres. Clear­ly vis­i­ble are the nu­mer­ous large rocks on the as­ter­oid’s sur­face as well as the large craters in the mid­dle of the im­age. One pix­el cor­re­sponds to 60 cen­time­tres.
3D model of the asteroid Ryugu
Ryugu – a ‘di­a­mond’ in space
Image 7/7, Credit: University of Aizu, Kobe University, Auburn University, JAXA

Ryugu – a ‘diamond’ in space

Based on the first im­ages of Ryugu, tak­en by the Op­ti­cal Nav­i­ga­tion Cam­era – Tele­scop­ic (ONC-T) of the Japanese Hayabusa2 space probe, the Japanese space agen­cy JAXA and re­searchers from the Uni­ver­si­ty of Aizu de­vel­oped a 3D mod­el of the as­ter­oid. In Oc­to­ber 2018, the lan­der MAS­COT, de­vel­oped and built by the Ger­man Aerospace Cen­ter (Deutsches Zen­trum für Luft- und Raum­fahrt; DLR) in close co­op­er­a­tion with the French space agen­cy CNES (Cen­tre Na­tion­al d’Etudes Spa­tiales), will land on the as­ter­oid. The ce­les­tial body will then be re­searched us­ing four in­stru­ments.
  • Landing will take place autonomously in free fall
  • 16 hours of measurements on Ryugu's surface
  • Hop to second measurement site planned

If everything goes according to plan, the moment will finally come on 3 October 2018. Early in the morning, at 03:58:15 CEST, the asteroid lander MASCOT will separate from the Hayabusa2 space probe and land on the surface of Ryugu a few minutes later. From the first moment of contact with the surface, this will be a journey into the unknown, as MASCOT could come to rest almost anywhere within a radius of about 200 metres from the point of touchdown, after bouncing a few times. During the morning of 3 October, researchers at the lander control centre at the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) in Cologne will be expecting confirmation of the landing. MASCOT will then have come to rest and will start taking comprehensive scientific measurements. The lander will remain there for about 16 hours before the battery runs out. The Twitter account @MASCOT2018 will be posting the very latest information before and during the landing using the hashtag #asteroidlanding.

"In the hours leading to the separation, the Japanese Hayabusa2 space probe will be operating at a relative height of only 60 metres above the asteroid’s surface," explains Tra-Mi Ho, Project Manager of the German-French lander MASCOT at the DLR Institute of Space Systems in Bremen. "Just before the landing, Hayabusa2 will go into a freefall phase, at the end of which – after just 2 minutes and 20 seconds – MASCOT will be separated." Once the separation is complete, MASCOT will fall, completely unpowered, tumbling down onto the asteroid. The low gravitational pull will gently accelerate the lander to a speed of up to 20 centimetres per second. By comparison, normal walking speed is seven times faster. Five to 10 minutes after separation, MASCOT will already touch down on the selected landing zone on Ryugu for the first time, and then bounce several times before coming to rest.

"We are anxious to see whether MASCOT will slide out of its supporting frame smoothly", as we have planned and tested so extensively,” Ho says. “A smooth descent is crucial, otherwise MASCOT will bounce back up from the asteroid like a rubber ball due to the low gravitational pull, and be lost in space.” In addition, the researchers will be watching with excitement in the minutes and hours after touchdown, as it is impossible to predict how MASCOT will move on the surface according to the laws of physics alone. "We do not know in which direction and for how long MASCOT will bounce around after the initial touchdown, and we are of course hoping that it will not end up on terrain that is too soft or get stuck in a crevice, where it could not straighten itself," explains DLR's MASCOT Operations Manager Christian Krause. "However, we are optimistic because we ran through numerous scenarios on the ground and have sent the corresponding command sequences to MASCOT."

The lander will operate autonomously while on the asteroid and must operate robustly using the prepared command sequences, so that all of the measurements can be carried out according to plan. During the mission, MASCOT will decide how and when to initiate these sequences. An in-built autonomy manager will then determine when MASCOT has come to rest and can start to conduct measurements.

Landing and jumping between 30 metre-high boulders

It is planned that MASCOT will land in the southern hemisphere of the 950-metre-diameter Ryugu asteroid, at 315 degrees east and 30 degrees south. This location has a favourable day and night cycle, and a temperature range of around +47 to –63 degrees Celsius, which is neither too hot nor too cold for the lander. The rocks around the landing site are not too big, but there are numerous boulders measuring up to 30 metres in height, which present an additional challenge.

After MASCOT has uprighted itself autonomously, if necessary, and carried out the initial measurements autonomously for a few hours, the scientists in the MASCOT control centre in Cologne will decide whether the lander should hop to another measuring point using its built-in swing arm. "In the final tests before the landing, we estimated that we would probably only let MASCOT perform one jump of less than 10 metres, in order to preserve the battery life and ensure the optimal execution of the measurements and data transfer," Ho explains. "What is more, recent images suggest that the surface of Ryugu has a rather uniform composition everywhere, so we do not need to perform big jumps."

First images after a few days

A total of four instruments are installed within the 30 x 30 x 20 centimetre lander, which weighs only 10 kilograms. A DLR radiometer and camera, together with a spectrometer from the Institut d'Astrophysique Spatiale and a magnetometer from TU Braunschweig, are set to examine the mineralogical and geological composition of the asteroid’s surface and gauge its surface temperature, as well as the asteroid's magnetic field. Upon landing on Ryugu, MASCOT will only be reachable during a few time windows, whereby sending a command to the lander and receiving a response back on Earth will take more than 30 minutes. Therefore, MASCOT will be left largely to its own devices during the 16-hour-long measurement operation planned on the surface. As the orbiter will also be generating huge quantities of data during this period and the bandwidth of the link to Earth is relatively low, only a few status updates from MASCOT will be transmitted to the control centre in Cologne. The scientific data and images are expected to arrive a few days after the landing, at which point they will be analysed.

About the Hayabusa2 mission and MASCOT

Hayabusa2 is a Japanese space agency (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 French space agency CNES (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.

Follow the landing via our Livestream channel.

  • Falk Dambowsky
    Ger­man Aerospace Cen­ter (DLR)
    Me­dia Re­la­tions
    Com­mu­ni­ca­tions and Me­dia Re­la­tions
    Telephone: +49 2203 601-3959
    Fax: +49 2203 601-3249
    Linder Höhe
    51147 Cologne
  • Tra-Mi Ho
    Ger­man Aerospace Cen­ter (DLR)
    In­sti­tute of Space Sys­tems
    Telephone: +49 421 24420-1171
    Robert-Hooke-Straße 7
    28359 Bremen
  • Christian Krause
    Ger­man Aerospace Cen­ter (DLR)

    Mi­cro­grav­i­ty Us­er Sup­port Cen­ter (MUSC), Space Op­er­a­tions and As­tro­naut Train­ing
    Telephone: +49 2203 601-3048
    Linder Höhe
    51147 Köln
  • Manuela Braun
    Ger­man Aerospace Cen­ter (DLR)
    Pro­gramme and Strat­e­gy, Space Re­search and Tech­nol­o­gy
    Telephone: +49 2203 601-3882
    Fax: +49 2203 601-3249
    Hansestraße 115
    51149 Cologne
  • 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

Main menu