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arXiv · 1803.00238

Shape model of the asteroid (2501) Lohja from long-term photometric observations

M. Husárik
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Abstract

We present lightcurves, shapes, and a 3D convex spin-axis model for the main-belt asteroid (2501) Lohja. The models were obtained with the lightcurve inversion process using combined dense photometric data from the apparitions between years 2006 and 2017. The analysis found a sidereal period of 3.80835\,hours, and a possible ecliptic pole solution (J2000.0), the prograde sense of rotation and main ratios of the ellipsoidal model.

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M. Husárik. 2018-03-01. Shape model of the asteroid (2501) Lohja from long-term photometric observations. https://arxiv.org/abs/1803.00238

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