Photometry and model of near-Earth asteroid 2021 DW1 from one apparition

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Título: Photometry and model of near-Earth asteroid 2021 DW1 from one apparition
Autor/es: Kwiatkowski, T. | Koleńczuk, P. | Kryszczynska, Agnieszka | Oszkiewicz, Dagmara | Kamiński, K. | Kamińska, M.K. | Troianskyi, Volodymyr | Skiff, Brian | Moskovitz, Nicholas A. | Kashuba, V. | Kim, Myung-Jin | Kim, T. | Mottola, S. | Santana-Ros, Toni | Kluwak, T. | Buzzi, Luca | Bacci, P. | Birtwhistle, P. | Miles, R. | Chatelain, Joseph
Centro, Departamento o Servicio: Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal
Palabras clave: Methods: observational | Techniques: photometric | Minor planets, asteroids: individual: 2021 DW1
Área/s de conocimiento: Física Aplicada
Fecha de publicación: 10-dic-2021
Editor: EDP Sciences
Cita bibliográfica: Astronomy & Astrophysics. 2021, 656: A126. https://doi.org/10.1051/0004-6361/202142013
Resumen: Aims. Very small asteroids (VSAs, objects with diameters smaller than about 150 m) can be spun up by the YORP effect to rotation periods as short as tens of seconds. This effect has been observed for many of them. It is also hypothesised, that in the same process their spin axes are asymptotically drawn to the position perpendicular to the orbital plane. So far this effect has been observed only for one VSA and needs further verification. For that, spin axes of several other VSAs should be determined by observing their brightness variations at many different positions on the sky. Methods. On 4 March 2021 at 9 UTC a 30-m in diameter near-Earth asteroid 2021 DW1 passed the Earth at a distance of 570 000 km, reaching the maximum brightness of V = 14.6 mag. We observed it photometrically from 2 March, when it was visible at V = 16.5 mag, until 7 March (V = 18.2 mag). During that time 2021 DW1 swept a 170° long arc in the northern sky, spanning solar phase angles in the range from 36° to 86°. This made it an excellent target for physical characterisation, including spin axis and shape derivation. Results. Convex inversion of the asteroid lightcurves gives a sidereal period of rotation Psid = 0.013760 ± 0.000001 h, and two solutions for the spin axis ecliptic coordinates: (A) λ1 = 57° ± 10°, β1 = 29° ± 10° and (B) λ2 = 67° ± 10°, β2 = −40° ± 10°. The magnitude-phase curve can be fitted with a standard H, G function with H = 24.8 ± 0.5 mag and an assumed G = 0.24. The asteroid colour indices are g − i = 0.79 ± 0.01 mag, and i − z = 0.01 ± 0.02 mag which indicates an S taxonomic class, with an average geometric albedo pV = 0.23 ± 0.02. The asteroid effective diameter, derived from H and pV, is Deff = 30 ± 10 m. Conclusions. It was found that the inclination of the spin axis of 2021 DW1 is not perpendicular to the orbital plane (obliquity ϵ = 54° ± 10° or ϵ = 123° ± 10°). More spin axes of VSAs should be determined to check, if 2021 DW1 is an exception or a typical case.
Patrocinador/es: T.K., A.K., and D.O. were supported by a grant No.2017/25/B/ST9/00740 from the National Science Centre, Poland. T. Kim was supported by the Korea Astronomy and Space Science Institute under the R&D program (Project No. 2020-1-600-05) supervised by the Ministry of Science and ICT (MSIT), and the National Research Foundation of Korea (NRF) Grant No. 2020R1A2C3011091, funded by MSIT. The work by T.S.-R. was carried out through a grant APOSTD/2019/046 by Generalitat Valenciana (Spain). He was also supported by the MINECO (Spanish Ministry of Economy) through a grant RTI2018-095076-B-C21 (MINECO/FEDER, UE).
URI: http://hdl.handle.net/10045/120746
ISSN: 0004-6361 (Print) | 1432-0746 (Online)
DOI: 10.1051/0004-6361/202142013
Idioma: eng
Tipo: info:eu-repo/semantics/article
Derechos: © ESO 2021
Revisión científica: si
Versión del editor: https://doi.org/10.1051/0004-6361/202142013
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