A Fast Ellipsoid Model for Asteroids Inverted From Lightcurves
Xiaoping Lu, Haibin Zhao, Zhong You

TL;DR
This paper introduces a rapid method to reconstruct asteroid shapes as ellipsoids from lightcurve data, enabling estimation of physical parameters with reasonable accuracy using a curvature-based brightness integration and optimization techniques.
Contribution
The paper presents a novel, efficient approach for asteroid shape modeling from lightcurves assuming an ellipsoid shape, improving speed and simplicity over existing methods.
Findings
Accurate estimation of asteroid physical parameters
Generation of simple ellipsoid shape models
Effective use of curvature function and Lebedev Quadrature
Abstract
The research about asteroids attracts more and more attention recently, especially focusing on their physical structures, such as the spin axis, the rotation period and the shape. The long distance between Earth observers and asteroids makes it impossible to get the shape and other parameters of asteroids directly with the exception of the NEAs (Near Earth Asteroids) and others passed by some spacecrafts. Generally photometric measurement is still the main way to obtain the research data for asteroids now, i.e. the lightcurves recording the brightness and positions of asteroids. Supposing that the shape of the asteroid is a triaxial ellipsoid with a stable spinning status, a new method is present in this article to reconstruct the shape models of asteroids from the lightcurves, with the other physical parameters together. By applying a special curvature function, the method calculates…
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