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• W3207863387 abstract "Context. The rotation state of small asteroids is affected by the Yarkovsky–O’Keefe–Radzievskii–Paddack (YORP) effect, which is a net torque caused by solar radiation directly reflected and thermally reemitted from the surface. Due to this effect, the rotation period slowly changes, which can be most easily measured in light curves because the shift in the rotation phase accumulates over time quadratically. Aims. By new photometric observations of selected near-Earth asteroids, we want to enlarge the sample of asteroids with a detected YORP effect. Methods. We collected archived light curves and carried out new photometric observations for asteroids (10115) 1992 SK, (1620) Geographos, and (1685) Toro. We applied the method of light curve inversion to fit observations with a convex shape model. The YORP effect was modeled as a linear change of the rotation frequency υ ≡ d ω ∕d t and optimized together with other spin and shape parameters. Results. We detected the acceleration υ = (8.3 ± 0.6) × 10 −8 rad d −2 of the rotation for asteroid (10115) 1992 SK. This observed value agrees well with the theoretical value of YORP-induced spin-up computed for our shape and spin model. For (1685) Toro, we obtained υ = (3.3 ± 0.3) × 10 −9 rad d −2 , which confirms an earlier tentative YORP detection. For (1620) Geographos, we confirmed the previously detected YORP acceleration and derived an updated value of υ with a smaller uncertainty. We also included the effect of solar precession into our inversion algorithm, and we show that there are hints of this effect in Geographos’ data. Conclusions. The detected change of the spin rate of (10115) 1992 SK has increased the total number of asteroids with YORP detection to ten. In all ten cases, the d ω ∕d t value is positive, so the rotation of these asteroids is accelerated. It is unlikely to be just a statistical fluke, but it is probably a real feature that needs to be explained." @default.
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• W3207863387 date "2021-12-20" @default.
• W3207863387 modified "2023-10-18" @default.
• W3207863387 title "Rotation acceleration of asteroids (10115) 1992 SK, (1685) Toro, and (1620) Geographos due to the YORP effect" @default.
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• W3207863387 cites W1981341927 @default.
• W3207863387 cites W1987427957 @default.
• W3207863387 cites W2007451448 @default.
• W3207863387 cites W2015574826 @default.
• W3207863387 cites W2016543750 @default.
• W3207863387 cites W2025336978 @default.
• W3207863387 cites W2040806618 @default.
• W3207863387 cites W2054250517 @default.
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• W3207863387 cites W2153350740 @default.
• W3207863387 cites W2396160526 @default.
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• W3207863387 cites W2768224373 @default.
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• W3207863387 doi "https://doi.org/10.1051/0004-6361/202141844" @default.
• W3207863387 hasPublicationYear "2021" @default.
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