Bibcode
                                    
                            Scholten, F.; Preusker, F.; Elgner, S.; Matz, K. -D.; Jaumann, R.; Biele, J.; Hercik, D.; Auster, H. -U.; Hamm, M.; Grott, M.; Grimm, C.; Ho, T. -M.; Koncz, A.; Schmitz, N.; Trauthan, F.; Kameda, S.; Sugita, S.; Honda, R.; Morota, T.; Tatsumi, E.; Cho, Y.; Yoshioka, K.; Sawada, H.; Yokota, Y.; Sakatani, N.; Hayakawa, M.; Matsuoka, M.; Yamada, M.; Kouyama, T.; Suzuki, H.; Honda, C.; Ogawa, K.
    Bibliographical reference
                                    Astronomy and Astrophysics
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                        12
            
                        2019
            
  Journal
                                    
                            Citations
                                    18
                            Refereed citations
                                    18
                            Description
                                    Images from the Optical Navigation Camera system (ONC) onboard the Hayabusa2 spacecraft show the MASCOT lander during its descent to the surface of asteroid (162173) Ryugu. We used results from a previous stereo-photogrammetric analysis that provided precise ONC image orientation data (camera position and pointing), ONC orthoimages, and an ONC-based 3D surface model to combine them with the visibilities of MASCOT itself and its shadow on-ground within the ONC images. We integrated additional information from instruments onboard MASCOT (MASMag, MARA, MASCam) and derived MASCOT's release position and modeled its free-fall descent path and its velocity over 350 s from its release at ̃41 m altitude above ground until its first contact with the surface of Ryugu. After first contact, MASCOT bounced over the surface of Ryugu for 663 s and came to rest at its first settlement point after four intermediate surface contacts. We again used ONC images that show MASCOT and partly its shadow and reconstructed the bouncing path and the respective velocities of MASCOT. The achieved accuracy for the entire descent and bouncing path is ̃0.1 m (1σ).
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Small Bodies of the Solar System
            
    This project studies the physical and compositional properties of the so-called minor bodies of the Solar System, that includes asteroids, icy objects, and comets. Of special interest are the trans-neptunian objects (TNOs), including those considered the most distant objects detected so far (Extreme-TNOs or ETNOs); the comets and the comet-asteroid
            
            Julia de
            
                        León Cruz