Results 11 to 20 of about 486,437 (201)
Stability of a Rotating Asteroid Housing a Space Station [PDF]
Today there are numerous studies on asteroid mining. They elaborate on selecting the right objects, prospecting missions, potential asteroid redirection, and the mining process itself.
Thomas I. Maindl +2 more
doaj +4 more sources
The dependence of asteroid rotation on composition
Context. The rotational properties of asteroids provide critical information about not only their internal structure, but also their collisional and thermal histories.
Dyer T. J. +6 more
doaj +2 more sources
Mirror formation control in the vicinity of an asteroid [PDF]
Two strategies are presented for the positioning and control of a spacecraft formation designed to focus sunlight onto a point on the surface of asteroid, thereby sublimating the material and ejecting debris creating thrust.
Vasile, M. +8 more
core +8 more sources
On the consequences of a fragmentation due to a NEO mitigation strategy [PDF]
The fragmentation of an Earth threatening asteroid as a result of a hazard mitigation mission is examined in this paper. The minimum required energy for a successful impulsive deflection of a threatening object is computed and compared with the energy ...
Vasile, M. +6 more
core +8 more sources
We have considered here a novel particular model for dynamics of a non-rigid asteroid rotation, assuming the added mass model instead of the concept of Viscoelastic Oblate Rotators to describe the physically reasonable response of a ‘rubble pile ...
Sergey Ershkov, Dmytro Leshchenko
doaj +1 more source
Cohesive regolith on fast rotating asteroids [PDF]
Accepted for publication in ...
Sánchez, Paul, Scheeres, Daniel J.
openaire +2 more sources
Consequences of asteroid fragmentation during impact hazard mitigation [PDF]
The consequences of the fragmentation of an Earth-threatening asteroid due to an attempted deflection are examined in this paper. The minimum required energy for a successful impulsive deflection of a threatening object is computed and compared to the ...
Vasile, M. +2 more
core +3 more sources
Physical Properties of the Young Asteroid Pair 2010 UM26 and 2010 RN221
The main belt asteroids 458271 (2010 UM26) and 2010 RN221 share almost identical orbital elements, and currently appear as comoving objects ∼30″ apart in the plane of the sky.
David Jewitt +3 more
doaj +1 more source
ROTATIONAL PROPERTIES OF THE MARIA ASTEROID FAMILY [PDF]
Maria family is regarded as an old-type (~3 +/- 1 Gyr) asteroid family which has experienced substantial collisional and dynamical evolution in the Main-belt. It is located nearby the 3:1 Jupter mean motion resonance area that supplies Near-Earth asteroids (NEAs) to the inner Solar System.
Kim M.-J. +15 more
openaire +4 more sources
Passive sorting of asteroid material using solar radiation pressure [PDF]
Understanding dust dynamics in asteroid environments is key for future science missions to asteroids and, in the long-term, also for asteroid exploitation.
Sanchez Cuartielles, Joan-Pau +2 more
core +6 more sources

