The diurnal Yarkovsky effect of irregularly shaped asteroids
Yang-Bo Xu (1), Li-Yong Zhou (1), Hejiu Hui (2), Jian-Yang Li (3) ((1), School of Astronomy, Space Science, Nanjing University, (2) School of, Earth Sciences, Engineering, Nanjing University, (3) Planetary Science, Institute, USA)

TL;DR
This paper models the diurnal Yarkovsky effect on irregularly shaped asteroids using high-precision simulations, compares results with traditional models, and introduces an effective area metric for practical estimation.
Contribution
It provides a detailed 3D numerical analysis of the diurnal Yarkovsky effect on various asteroid shapes and introduces the effective area concept for better effect estimation.
Findings
Linear model is accurate for spherical asteroids in most cases.
Linear model overestimates the effect on biaxial ellipsoids by about 10%.
Effective area correlates linearly with Yarkovsky migration rate.
Abstract
The Yarkovsky effect plays an important role in the motions of small celestial bodies. Increasingly improving observations bring the need of high-accuracy modelling of the effect. Using a multiphysics software COMSOL, we model the diurnal Yarkovsky effect in three dimensions and compare the results with that derived from the widely adopted theoretical linear model. We find that the linear model presents a high accuracy for spherical asteroids in most cases. The ranges of parameters in which the relative error of the linear model is over 10\% are explored. For biaxial ellipsoidal asteroids (particularly oblate ones), the linear model systematically overestimates the transverse Yarkovsky force by 10\%. The diurnal effect on triaxial ellipsoids is periodic for which no linear model is available. Our numerical calculations show that the average effects on triaxial ellipsoids are…
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