Issue |
A&A
Volume 632, December 2019
|
|
---|---|---|
Article Number | L5 | |
Number of page(s) | 6 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/201936760 | |
Published online | 02 December 2019 |
Letter to the Editor
The Hayabusa2 lander MASCOT on the surface of asteroid (162173) Ryugu – Stereo-photogrammetric analysis of MASCam image data
1
German Aerospace Center (DLR), Institute of Planetary Research, 12489 Berlin, Germany
e-mail: Frank.Scholten@dlr.de
2
German Aerospace Center (DLR), Microgravity User Support Center (MUSC), Cologne, Germany
3
German Aerospace Center (DLR), Institute of Space Systems, Bremen, Germany
4
Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo, Japan
5
University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo, Japan
6
Planetary Exploration Research Center, Chiba Institute of Technology, 2-17-1 Tsudanuma, Narashino, Chiba, Japan
Received:
23
September
2019
Accepted:
7
November
2019
After its release and a descent and bouncing phase, the Hayabusa2 lander MASCOT came to a final rest and MASCOT’s camera MASCam acquired a set of images of the surface of Ryugu. With MASCam’s instantaneous field of view of about 1 mrad, the images provide pixel scales from 0.2 to 0.5 mm pixel−1 in the foreground and up to 1 cm pixel−1 for surface parts in the background. Using a stereo-photogrammetric analysis of the MASCam images taken from slightly different positions due to commanded and unintentional movements of the MASCOT lander, we were able to determine the orientation for the different measurement positions. Furthermore, we derived a 3D surface model of MASCOT’s vicinity. Although the conditions for 3D stereo processing were poor due to very small stereo angles, the derived 3D model has about 0.5 cm accuracy in the foreground at 20 cm distance and about 1.5 cm at a distance of 40–50 cm.
Key words: minor planets / asteroids: general / minor planets / asteroids: individual: (162173) Ryugu / planets and satellites: surfaces
© ESO 2019
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