On 3 December 2014 at 05:22 CEST, an H IIA launch vehicle lifted off from the Tanegashima Space Center and the Japanese Hayabusa 2 spacecraft and its MASCOT lander, developed by DLR, began their journey to Asteroid 1999 JU3.
The Japanese Hayabusa2 spacecraft with the German-French Mobile Asteroid Surface Scout (MASCOT) lander on board has completed its 3200-million-kilometre journey to asteroid Ryugu.
DLR (CC-BY 3.0).
On 26 June 2018, the Japanese Optical Navigation Camera – Telescopic (ONC-T) on board Hayabusa2 imaged the asteroid Ryugu from a distance of approximately 22 kilometres, shortly before it arrived.The ONC was developed and built under the leadership of JAXA in collaboration with the University of Tokyo, Kochi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, Aizu University and the National Institute of Advanced Industrial Science and Technology (AIST) with contracted contributions from the company NEC.
JAXA, University of Tokyo, Kochi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, Aizu University, AIST.
A total of four instruments are installed within the 30 × 30 × 20-centimetre lander. A DLR radiometer and camera, together with a spectrometer from the Institut d’Astrophysique Spatiale and a magnetometer from Technical University Braunschweig are set to examine the mineralogical composition and geological properties of the asteroid’s surface and measure its surface temperature and magnetic field. MASCOT’s swing arm will provide it with the kinetic energy required to perform its manoeuvres on the surface.
The Hayabusa2 space probe is currently en route to C-type asteroid 162173 Ryugu (1999 JU3). It is operated by the Japan Aerospace Exploration Agency (JAXA) and carries the MASCOT (Mobile Asteroid Surface Scout) lander built by the German Aerospace Center (DLR) in collaboration with the French Space Agency (CNES). Its target Ryugu is what is known as a near-Earth asteroid. 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.
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 will:
Hayabusa2 and MASCOT will work together as a team: Hayabusa2 will transmit data so that a suitable landing place can be found for MASCOT, whereas MASCOT will carry out experiments on the asteroid's surface, and provide 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. The measurements taken by MASCOT will also serve as an important reference for the samples brought back to Earth, because there is a possibility that the material gathered could have changed during the extraction process.
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, presents a challenge for the mission. This force is insufficient to 'pull' the lander out of the Hayabusa probe. As such, MASCOT will be pushed out of its holder by a spring mechanism and fall to Ryugu from a height of approximately 60 metres. If this happens too quickly, then there is a risk that MASCOT will bounce off the asteroid's surface. It is also important that the lander's 'hopping' on the asteroid from site to site is programmed from start to finish so that it does 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 surface and its surface temperature and magnetic field will be 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 will reach Ryugu in the summer of 2018, with Hayabusa2 returning 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.
Last modified:10/01/2018 15:18:01