Dynamic precise orbit determination of Hayabusa2 using laser altimeter (LIDAR) and image tracking data sets
Creators
- Yamamoto, Keiko1
- Otsubo, Toshimichi2
- Matsumoto, Koji3, 1
- Noda, Hirotomo3, 1
- Namiki, Noriyuki3, 1
- Takeuchi, Hiroshi4, 3
- Ikeda, Hitoshi5
- Yoshikawa, Makoto4, 3
- Yamamoto, Yukio4, 3
- Senshu, Hiroki6
- Mizuno, Takahide4
- Hirata, Naru7
- Yamada, Ryuhei7
- Ishihara, Yoshiaki8, 9
- Araki, Hiroshi3, 1
- Abe, Shinsuke10
- Yoshida, Fumi6
- Higuchi, Arika1
- Sasaki, Sho11
- Oshigami, Shoko4
- and others
- 1. National Astronomical Observatory of Japan (Japan)
- 2. Hitotsubashi University (Japan)
- 3. The Graduate University for Advanced Studies, SOKENDAI (Japan)
- 4. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (Japan)
- 5. Research and Development Directorate, JAXA, Japan Aerospace Exploration Agency (Japan)
- 6. Planetary Exploration Research Center, Chiba Institute of Technology (Japan)
- 7. The University of Aizu (Japan)
- 8. JAXA Space Exploration Center,Japan Aerospace Exploration Agency (Japan)
- 9. National Institute for Environmental Studies (Japan)
- 10. Nihon University (Japan)
- 11. Osaka University (Japan)
Description
The precise orbit of the Hayabusa2 spacecraft with respect to asteroid Ryugu is dynamically determined using the data sets collected by the spacecraft's onboard laser altimeter (LIght Detection And Ranging, LIDAR) and automated image tracking (AIT). The LIDAR range data and the AIT angular data play complementary roles because LIDAR is sensitive to the line-of-sight direction from Hayabusa2 to Ryugu, while the AIT is sensitive to the directions perpendicular to it. Using LIDAR and AIT, all six components of the initial state vector can be derived stably, which is difficult to achieve using only LIDAR or AIT. The coefficient of solar radiation pressure (SRP) of the Hayabusa2 spacecraft and standard gravitational parameter (GM) of Ryugu can also be estimated in the orbit determination process, by combining multiple orbit arcs at various altitudes. In the process of orbit determination, the Ryugu-fixed coordinate of the center of the LIDAR spot is determined by fitting the range data geometrically to the topography of Ryugu using the Markov Chain Monte Carlo method. Such an approach is effective for realizing the rapid convergence of the solution. The root mean squares of the residuals of the observed minus computed values of the range and brightness-centroid direction of the image are 1.36 m and 0.0270°, respectively. The estimated values of the GM of Ryugu and a correction factor to our initial SRP model are 29.8 ± 0.3 m3/s2 and 1.13 ± 0.16, respectively.
Additional details
Identifiers
Publishing Information
- Journal Title
- Earth, Planets and Space (Online)
- Journal Volume
- 72
- Journal Issue
- 1
- Journal Page Range
- vp.
- ISSN
- 1880-5981
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 55062324
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ALTITUDE; BRIGHTNESS; CONVERGENCE; COORDINATES; CORRECTIONS; IMAGES; LASERS; MONTE CARLO METHOD; ORBITS; RADIATION PRESSURE; SATELLITES; SOLAR RADIATION; SPACE VEHICLES; SUN; TOPOGRAPHY; VISIBLE RADIATION
- Descriptors DEC
- CALCULATION METHODS; ELECTROMAGNETIC RADIATION; MAIN SEQUENCE STARS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS; STELLAR RADIATION; VEHICLES
Optional Information
- Copyright
- Copyright (c) 2020 © The Author(s) 2020