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Fig. 3 Asteroid rotation period vs. diameter.
To look for SFRs and to conduct a comprehensive study on asteroid rotation, we initiated a project to survey asteroid rotation periods using the iPTF since February 2013.
A similar result was also obtained using the asteroid rotation periods derived from the iPTF archive data (Waszczak et al. 2015).
Eight campaigns to survey asteroid rotation periods have been carried out using the intermediate Palomar Transient Factory in the past 3 years.
With the collected asteroid rotation periods, we found a lower spin-rate limit for C-type asteroids (i.e., lower bulk density) when compared with S-type asteroids.
However, even conservatively optimistic simulations of small asteroid detumbling scenarios indicate that such a method could take over a year to arrest the asteroid rotation.
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Eventually, our model asteroids reach rotation states that approach regular motion of the spin axis in the body frame.
Their stability is examined against the distance to the asteroid and the rotation rate of the asteroid, to uncover the influence of highly non-spherical gravitational field and the rotation of the asteroid on the orbital motion.
The NEOCam mission would use an infra-red camera to garner information on asteroid size, shape, rotation and composition.
In particular, the orbital reorientation effect is influential when realistic asteroid shapes and rotations are accounted for.
The rotation of asteroids causes difficulties in the exploration of asteroids or prevention of asteroids impact on the Earth.
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