Add to ORKGPhotometric observations are the primary source of information on the bulk of the asteroid population. The macroscopic shapes, rotational states, and scattering parameters of asteroids ca be deduced from photometric measurements of total brightness in different viewing/illumination geometries. Shape classes include convex, nonconvex, and binary objects, while rotational states include relaxed rotation, precessing motion, and mutually orbiting configurations. We discuss the role of lightcurve inversion in light of results from other sources
Context. In the past decade, more than one hundred asteroid models were derived using the lightcurve...
International audienceAims:We present physical models of ten asteroids obtained by means of lightcur...
Context. Information about shapes and spin states of individual asteroids is important for the study...
Aims. Shape and spin state are basic physical characteristics of an asteroid. They can be derived f...
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconst...
Context. Rotation properties (spin-axis direction and rotation period) and coarse shape models of as...
Copyright ESO. The original version is available at www.aanda.org.International audienceThe larger n...
International audienceContext. The shapes and spin states of asteroids observed with photometric tec...
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconst...
Context. The larger number of models of asteroid shapes and their rotational states derived by the l...
We investigate the photometric accuracy of the sparse data from astrometric surveys available on Ast...
Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost ...
Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almo...
Context. Information about the spin state of asteroids is important for our understanding of the dyn...
Context. In the past decade, more than one hundred asteroid models were derived using the lightcurve...
International audienceAims:We present physical models of ten asteroids obtained by means of lightcur...
Context. Information about shapes and spin states of individual asteroids is important for the study...
Aims. Shape and spin state are basic physical characteristics of an asteroid. They can be derived f...
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconst...
Context. Rotation properties (spin-axis direction and rotation period) and coarse shape models of as...
Copyright ESO. The original version is available at www.aanda.org.International audienceThe larger n...
International audienceContext. The shapes and spin states of asteroids observed with photometric tec...
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconst...
Context. The larger number of models of asteroid shapes and their rotational states derived by the l...
We investigate the photometric accuracy of the sparse data from astrometric surveys available on Ast...
Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost ...
Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almo...
Context. Information about the spin state of asteroids is important for our understanding of the dyn...
Context. In the past decade, more than one hundred asteroid models were derived using the lightcurve...
International audienceAims:We present physical models of ten asteroids obtained by means of lightcur...
Context. Information about shapes and spin states of individual asteroids is important for the study...