The Astronomical Journal, 161:112 (23pp), 2021 March https://doi.org/10.3847/1538-3881/abd4da © 2021. The American Astronomical Society. All rights reserved. Spin Change of Asteroid 2012 TC4 Probably by Radiation Torques Hee-Jae Lee1,2 , Josef Ďurech3 , David Vokrouhlický3 , Petr Pravec4, Hong-Kyu Moon2, William Ryan5, Myung-Jin Kim2, Chun-Hwey Kim1 , Young-Jun Choi2,6, Paolo Bacci7, Joe Pollock8, and Rolf Apitzsch9 1 Chungbuk National University, 1 Chungdae-ro, Seowon-gu, Cheongju, Chungbuk 28644, Republic of Korea;
[email protected] 2 Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea 3 Astronomical Institute, Faculty of Mathematics and Physics, Charles University, V Holešovičkách 2, 180 00 Prague 8, Czech Republic 4 Astronomical Institute, Academy of Sciences of the Czech Republic, Fričova 1, 251 65 Ondrejov,̌ Czech Republic 5 New Mexico Institute of Mining and Technology, Socorro, NM 87801, USA 6 University of Science and Technology, 217, Gajeong-ro, Yuseong-gu, Daejeon 34113, Republic of Korea 7 Gruppo Astrofili Montagna Pistoiese, 51028 San Marcello Piteglio, Province of Pistoia, Italy 8 Physics and Astronomy Department, Appalachian State University, Boone, NC 28608, USA 9 Wildberg Observatory, D-72218 Wildberg, Germany Received 2020 November 25; revised 2020 December 13; accepted 2020 December 16; published 2021 February 11 Abstract Asteroid 2012 TC4 is a small (∼10 m) near-Earth object that was observed during its Earth close approaches in 2012 and 2017. Earlier analyses of light curves revealed its excited rotation state. We collected all available photometric data from the two apparitions to reconstruct its rotation state and convex shape model.