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Dynamics around small irregularly shaped objects modeled as a mass dipole. [PDF]
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2022
(162173) Ryugu is a near-Earth C-type (i.e., carbonaceous) asteroid. It has been, after Itokawa, the second target for an asteroidal sample return, thanks to the JAXA Hayabusa2 mission (Watanabe et al. 2019). Most interestingly, Ryugu in situ observations in 2018–2019 have confirmed, as expected from its classification, the presence of significant ...
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(162173) Ryugu is a near-Earth C-type (i.e., carbonaceous) asteroid. It has been, after Itokawa, the second target for an asteroidal sample return, thanks to the JAXA Hayabusa2 mission (Watanabe et al. 2019). Most interestingly, Ryugu in situ observations in 2018–2019 have confirmed, as expected from its classification, the presence of significant ...
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2022
(101955) Bennu is a near-Earth carbonaceous asteroid, suggested to belong to the taxonomic class B or more likely to the rare class F (Belskaya et al. 2005) from its spectro-polarimetric properties (Cellino et al. 2018). It has been the target of the NASA OSIRIS-REx sample return mission, which rendezvoused with it in late 2018 and collected samples in
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(101955) Bennu is a near-Earth carbonaceous asteroid, suggested to belong to the taxonomic class B or more likely to the rare class F (Belskaya et al. 2005) from its spectro-polarimetric properties (Cellino et al. 2018). It has been the target of the NASA OSIRIS-REx sample return mission, which rendezvoused with it in late 2018 and collected samples in
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Solar Sail Body-Fixed Hovering over Elongated Asteroids
, 2016Solar sail spacecraft are proposed to accomplish body-fixed hovering missions over elongated asteroids. The body-fixed hovering flight is to maintain a fixed position relative to the surface of the spinning asteroid. A solar sail without fuel consumption
Xiangyuan Zeng +3 more
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Asteroid Fragmentation and Evolution of Asteroids
Annual Review of Earth and Planetary Sciences, 2000To understand the complex collisional history of asteroids and explain their observed characteristics, it is necessary to be able to describe the fundamental physics of large-scale impact events. Because data collected on collisional outcomes is derived from small-scale laboratory experiments, success at describing asteroid evolution hinges ...
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