Results 1 to 10 of about 440 (144)

Satellite Formation around the Largest Asteroids

open access: yesThe Astrophysical Journal Letters
Abstract Satellites around large asteroids are preferentially found among those with the most rapid rotation and elongated shape. The taxonomic statistics are similarly skewed; in total, 13 asteroids larger than 100 km are known to have satellites, but none have been discovered among S-type asteroids.
Walsh, Kevin   +5 more
openaire   +3 more sources

A contact binary satellite of the asteroid (152830) Dinkinesh [PDF]

open access: yesNature
Abstract Asteroids with diameters less than about 5 km have complex histories because they are small enough for radiative torques (that is, YORP, short for the Yarkovsky–O’Keefe–Radzievskii–Paddack effect) 1 to be a notable factor in their evolution 2
Harold F. Levison   +118 more
openaire   +6 more sources

On the stability of the satellites of asteroid 87 Sylvia [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2009
he triple asteroidal system (87) Sylvia is composed of a 280-km primary and two small moonlets named Romulus and Remus (Marchis et al 2005). Sylvia is located in the main asteroid belt. The satellites are in nearly equatorial circular orbits around the primary.
Winter, O. C.   +7 more
openaire   +4 more sources

Trojan Asteroid Satellites, Rings, and Activity

open access: yesSpace Science Reviews, 2023
AbstractThe Lucy mission will encounter five Jupiter Trojans during its mission with three of the five already known to be multiple systems. These include a near-equal-mass binary, a small and widely separated satellite, and one intermediate-size satellite system.
Keith S. Noll   +8 more
openaire   +2 more sources

Magnetic field of planets, satellites and asteroids [PDF]

open access: yesAstronomical School’s Report, 2012
Origin of magnetic field of the solar system bodies, features and structure of magnetic field of planets of terrestrial type, giant planets, Moon, galilean satellites and asteroids are considered.
openaire   +2 more sources

Orbits of very distant asteroid satellites

open access: yesAstronomy & Astrophysics
The very wide binary asteroid (VWBA) population is a small subset of the population of known binary and multiple asteroids made of systems with very distant satellites and long orbital periods, on the order of tens to hundreds of days. The origin of these systems is debatable, and most members of this population are poorly characterized.
Kate Minker   +2 more
  +7 more sources

Inflatable Dome for Moon, Mars, Asteroids, and Satellites

open access: yesAIAA SPACE 2007 Conference & Exposition, 2007
On a planet without atmosphere, sustaining human life is very difficult and dangerous, especially during short sunlit period when low temperature prevails. To counter these environmental stresses, the author offer an innovative artificial "Evergreen" dome, an inflated hemisphere with interiors continuously providing a climate like that of Florida ...
openaire   +2 more sources

Asteroid Satellite Discovery Optimization

open access: yes
The discovery of asteroid-satellite systems not only reveals the formation and evolution mechanisms of small solar system bodies but also provides insights into the optimization of complex systems. This paper proposes a heuristic optimization algorithm based on the principles of asteroid-satellite discovery.
openaire   +2 more sources

Asteroid Satellite Inspired Optimization

open access: yes
Asteroid satellite systems, as important binary or multi-body structures in the solar system, are of great significance to the study of astrophysics and orbital mechanics. This paper proposes a heuristic optimization algorithm based on the asteroid satellite discovery process—the Asteroid Satellite Inspired Optimization (ASIO) algorithm. This algorithm
openaire   +1 more source

Asteroid-Satellite Perturbation Optimization

open access: yes
Asteroid-Satellite Perturbation Optimization (ASP-O) is a complex nonlinear dynamical problem, characterized by gravitational interactions between the primary asteroid and its satellite, as well as orbital variations caused by external perturbations.
openaire   +1 more source

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