Results 31 to 40 of about 13,644 (233)
Formation of asteroid pairs by rotational fission [PDF]
12 pages, 2 figures, 1 table + Supplementary ...
Pravec, Petr +25 more
openaire +5 more sources
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
Deflecting small asteroids using laser ablation : Deep space navigation and asteroid orbit control for LightTouch2 Mission [PDF]
This paper presents a low-cost, low mass, mission design to successfully intercept and deflect a small and faint, 4 m in diameter asteroid. Intended to be launched after 2025, the laser-ablating mission, LightTouch2 will be used to deflect the orbit of ...
Branco, Joao +4 more
core +1 more source
A New Large Super-Fast Rotator: (335433) 2005 UW163 [PDF]
Asteroids of size larger than 150 m generally do not have rotation periods smaller than 2.2 hours. This spin cutoff is believed to be due to the gravitationally bound rubble-pile structures of the asteroids.
Chang, Chan-Kao +7 more
core +3 more sources
The Apollo Group Asteroid 2008 OS9: Discovery, Orbit, Rotation and the Yarkovsky/YORP Effects
A project for astrometric and photometric observations of asteroids at the Baldone Observatory is described. One of the most important results of the project is the discovery of 2008 OS9, a 600 meter asteroid of the NEO Apollo group.
Černis K. +4 more
doaj +1 more source
Photometry and shape modeling of Mars crosser asteroid (1011) Laodamia [PDF]
An analysis of photometric observations of Mars crosser asteroid 1011 Laodamia conducted at Bulgarian National Astronomical Observatory Rozhen over a twelve year interval (2002, 2003, 2004, 2006, 2007, 2008, 2011, 2012 and 2013) is made.
Apostolovska G. +5 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
313 new asteroid rotation periods from Palomar Transient Factory observations [PDF]
A new asteroid rotation period survey have been carried out by using the Palomar Transient Factory (PTF). Twelve consecutive PTF fields, which covered an area of 87 deg$^2$ in the ecliptic plane, were observed in $R$ band with a cadence of $\sim$20 min ...
Chang, Chan-Kao +13 more
core +3 more sources
The main motivation of this research is the semi-analytical exploration of the dynamics of an asteroid that is attacked while approaching a planet (with an inelastic collision of the projectile normally to the surface of the asteroid occurring just ...
Sergey Ershkov
doaj +1 more source
The dynamics of asteroid rotation, governed by YORP effect: the kinematic ansatz
The main motivation of this research is the analytical exploration of the dynamics of asteroid rotation when it moves in elliptic orbit through Space.
Ershkov, Sergey V., Shamin, Roman V.
core +1 more source

