On the use of the K-means algorithm for determination of mass distributions in dumbbell-like celestial bodies
From MaRDI portal
Publication:4568591
DOI10.20537/nd1801004zbMath1395.70015OpenAlexW2971255797WikidataQ130014283 ScholiaQ130014283MaRDI QIDQ4568591
Vasily I. Nikonov, A. D. German, Ekaterina Aleksandrovna Raspopova, Alexander A. Burov
Publication date: 22 June 2018
Published in: Nelineinaya Dinamika (Search for Journal in Brave)
Full work available at URL: http://mathnet.ru/eng/nd595
Stability for nonlinear problems in mechanics (70K20) Equilibria and periodic trajectories for nonlinear problems in mechanics (70K42) Two-body problems (70F05)
Related Items (3)
Isosceles tetrahedron and an equimomental system of a rigid body ⋮ On the approximation of a nearly dynamically symmetric rigid body by two balls ⋮ Multipole representation of the gravitational field of the Asteroid (16) Psyche
Cites Work
- Unnamed Item
- Small body surface gravity fields via spherical harmonic expansions
- Existence of a class of irregular bodies with a higher convergence rate of Laplace series for the gravitational potential
- Ellipsoids, material points and material segments
- On bifurcation and stability of steady motions of two gravitating bodies
- The gravitational potential of a homogeneous polyhedron or don't cut corners
- Exterior gravitation of a polyhedron derived and compared with harmonic and mascon gravitation representations of asteroid 4769 Castalia
- Double material segment as the model of irregular bodies
- Periodic orbits around a massive straight segment
- On the gravity of dumbbell-like bodies represented by a pair of intersecting balls
- Triangular Libration Points of the Generalized Restricted Circular Problem of Three Bodies for conjugate complex masses of attracting centers
- Non-linear stability of the equilibria in the gravity field of a finite straight segment
This page was built for publication: On the use of the K-means algorithm for determination of mass distributions in dumbbell-like celestial bodies