TY - JOUR
T1 - Orbit insertion strategy of Hayabusa2’s rover with large release uncertainty around the asteroid Ryugu
AU - Oki, Yusuke
AU - Yoshikawa, Kent
AU - Takeuchi, Hiroshi
AU - Kikuchi, Shota
AU - Ikeda, Hitosi
AU - Scheeres, Daniel J.
AU - McMahon, Jay W.
AU - Kawaguchi, Junichiro
AU - Takei, Yuto
AU - Mimasu, Yuya
AU - Ogawa, Naoko
AU - Ono, Go
AU - Terui, Fuyuto
AU - Yamada, Manabu
AU - Kouyama, Toru
AU - Kameda, Shingo
AU - Yoshida, Kazuya
AU - Nagaoka, Kenji
AU - Yoshimitsu, Tetsuo
AU - Saiki, Takanao
AU - Tsuda, Yuichi
N1 - Funding Information:
This work was partially supported by JSPS KAKENHI Grant (No. 18H01628).
Publisher Copyright:
© 2020, Tsinghua University Press.
PY - 2020/12
Y1 - 2020/12
N2 - This paper describes the orbit design of the deployable payload Rover 2 of MINERVA-II, installed on the Hayabusa2 spacecraft. Because Rover 2 did not have surface exploration capabilities, the operation team decided to experiment with a new strategy for its deployment to the surface. The rover was ejected at a high altitude and made a semi-hard landing on the surface of the asteroid Ryugu after several orbits. Based on the orbital analysis around Ryugu, the expected collision speed was tolerable for the rover to function post-impact. Because the rover could not control its position, its motion was entirely governed by the initial conditions. Thus, the largest challenge was to insert the rover into a stable orbit (despite its large release uncertainty), and avoid its escape from Ryugu due to an environment strongly perturbed by solar radiation pressure and gravitational irregularities. This study investigates the solution space of the orbit around Ryugu and evaluates the orbit’s robustness by utilizing Monte Carlo simulations to determine the orbit insertion policy. Upon analyzing the flight data of the rover operation, we verified that the rover orbited Ryugu for more than one period and established the possibility of a novel method for estimating the gravity of an asteroid.
AB - This paper describes the orbit design of the deployable payload Rover 2 of MINERVA-II, installed on the Hayabusa2 spacecraft. Because Rover 2 did not have surface exploration capabilities, the operation team decided to experiment with a new strategy for its deployment to the surface. The rover was ejected at a high altitude and made a semi-hard landing on the surface of the asteroid Ryugu after several orbits. Based on the orbital analysis around Ryugu, the expected collision speed was tolerable for the rover to function post-impact. Because the rover could not control its position, its motion was entirely governed by the initial conditions. Thus, the largest challenge was to insert the rover into a stable orbit (despite its large release uncertainty), and avoid its escape from Ryugu due to an environment strongly perturbed by solar radiation pressure and gravitational irregularities. This study investigates the solution space of the orbit around Ryugu and evaluates the orbit’s robustness by utilizing Monte Carlo simulations to determine the orbit insertion policy. Upon analyzing the flight data of the rover operation, we verified that the rover orbited Ryugu for more than one period and established the possibility of a novel method for estimating the gravity of an asteroid.
KW - augmented elliptic Hill three-body problem
KW - gravitational irregularity
KW - solar radiation pressure
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U2 - 10.1007/s42064-020-0080-y
DO - 10.1007/s42064-020-0080-y
M3 - Article
AN - SCOPUS:85092636840
SN - 2522-0098
VL - 4
SP - 309
EP - 329
JO - Astrodynamics
JF - Astrodynamics
IS - 4
ER -