Results 11 to 20 of about 796 (181)
The physical and dynamical characteristics of the asteroid 4940 Polenov [PDF]
The asteroid (1986 QY4) 4940 Polenov is the first Solar system object whose 3D shape is determined using the observations from the newly built Astronomical Station Vidojevica (ASV).
Vchkova-Bebekovska E. +5 more
doaj +1 more source
Formation of asteroid pairs by rotational fission [PDF]
12 pages, 2 figures, 1 table + Supplementary ...
Pravec, Petr +25 more
openaire +5 more sources
On the rotation of cometary nuclei and small asteroids [PDF]
AbstractThe spin rate distributions of comet nuclei and small asteroids are compared, and it is shown that Whipple’s (1982) finding of a faster average rotation for the asteroid sample was due to observational biases. In fact, the presently available rotational data do not exhibit any clear differentiation among comet nuclei and asteroids, except ...
P. Farinella, P. Paolicchi, V. Zappalà
openaire +1 more source
Semi-analytical Ansatz for Approximating Dynamics of Asteroid Rotation Approaching Planet [PDF]
The main motivation of this research is the analytical exploration of the dynamics of asteroid rotation approaching planet, in view of future approach Apophis 2029 to Earth.
Sergey Ershkov
doaj +1 more source
We present photometric data for minor planets observed by the Transiting Exoplanet Survey Satellite during its Cycle 1 operations. In total, we extracted usable detections for 37,965 objects.
Andrew McNeill +5 more
doaj +1 more source
Preliminary refinement of rotation parameters of asteroids based on photogrammetric processing of on-orbit remote sensing images [PDF]
In recent years, asteroid exploration has become an important research direction in the field of deep space exploration. The weak gravitational environment of asteroids, as well as their complex topographic, geomorphic, and dynamic characteristics, pose ...
Z. Peng +7 more
doaj +1 more source
The Alinement of Asteroid Rotation [PDF]
Data have been accumulating since the beginning of this century that indicate that most, if not all, large asteroids have periodic lightcurves. The variations that are seen have periods of the order of several hours and can be understood as being caused by bodily rotation, accompanied by changes in shape and/or surface properties. Because corresponding
openaire +1 more source
Asteroid Photometric Phase Functions From Bayesian Lightcurve Inversion
Photometry is an important tool for characterizing the physical properties of asteroids. An asteroid’s photometric lightcurve and phase curve refer to the variation of the asteroid’s disk-integrated brightness in time and in phase angle (the Sun-asteroid-
Karri Muinonen +7 more
doaj +1 more source
THE ASTEROIDS' ROTATION PARAMETERS DETERMINATION USING PHOTOMETRICAL DATA
Presented a new method of determination of the asteroid rotation parameters.
N. R. Burlak +3 more
doaj +1 more source
Collisional and Rotational Disruption of Asteroids [PDF]
Asteroids are leftover pieces from the era of planet formation that help us understand conditions in the early Solar System. Unlike larger planetary bodies that were subject to global thermal modification during and subsequent to their formation, these small bodies have kept at least some unmodified primordial material from the solar nebula.
Walsh, K., Michel, P., Richardson, D.
openaire +3 more sources

