Diverse configurations of binary asteroids explained by multi-generation satellites. [PDF]
IntroductionNear-Earth asteroids and small main-belt asteroids (MBAs) with diameters between 200 m and 20 km are thought to be rubble piles. Most of their satellites are believed to be born from rotational mass shedding of the primary body, where the spin-up of a primary asteroid triggers mass shedding, creating a transient debris disk that finally re ...
Dai WY +12 more
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BroadSCOPE: An Optical Broadband Seismic Sensor for Planetary Exploration. [PDF]
Marusiak AG +19 more
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Asteroid sample return missions are critical for understanding our Solar System. [PDF]
Bates H.
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The Hazardous NEOs of the Future: Long-term Predictions under Uncertainty. [PDF]
Fuentes-Muñoz O +3 more
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Non-gravitational acceleration indicative of cometary activity of near-Earth object. [PDF]
Farnocchia D +14 more
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Phylogenetic position of the enigmatic starfish family Podosphaerasteridae (Asteroidea, Valvatida) with a morphological observation of the skeletal structure by micro-CT. [PDF]
Hiruta SF, Kobayashi I, Fujita T.
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Giving AI agents a sense of control facilitates reinforcement learning in multitasking scenarios. [PDF]
Österdiekhoff A +3 more
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Modular Platform for Rapidly Investigating Long-Distance Propagation of Human Neural Network Activity. [PDF]
Patel MD +6 more
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Potential metabolic viability on asteroid chemistry. [PDF]
Fisher T, Ferriere R.
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<sup>16</sup>O poor cosmic spherules from near-Earth CY chondrite asteroids. [PDF]
Van Ginneken M +11 more
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