Astrometry and Photometry of Potentially Dangerous Asteroid 65690 (1991 DG)

In 2020, two telescopes of the State Astrophysical Observatory of the Russian Academy of Sciences, ZA-320M and MTM-500M, obtained series of observations of the potentially dangerous asteroid 65690 (1991 DG) during its approach to the Earth and carried out their astrometric and photometric processing. Using the coordinates of the asteroid and observations from the MRS site, the orbit of the asteroid was clarified, and the circumstances of the approaches to the Earth and Mars were determined, and an assessment was made of the influence of nongravitational effects on its orbit. Based on the results of photometric processing of the asteroid, a light curve was constructed and the period of its axial rotation was determined: P = 4.3193 ± 0.0028 h.

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Publication Details

Journal
Solar System Research
Published
2024-09-09
DOI
https://doi.org/10.1134/s0038094624700369
Primary Topic
Astro and Planetary Science
Type
article
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article

Astrometry and Photometry of Potentially Dangerous Asteroid 65690 (1991 DG)

S.N. Petrova, K. N. Naumov, С. Д. Цекмейстер, Д. Л. Горшанов et al.
Solar System Research
Astro and Planetary Science
article

Astrometry and Photometry of Potentially Dangerous Asteroid 65690 (1991 DG)

S.N. Petrova, K. N. Naumov, С. Д. Цекмейстер, Д. Л. Горшанов, A. V. Devyatkin, A. A. Martyusheva, В. Н. Львов
article en

Abstract

In 2020, two telescopes of the State Astrophysical Observatory of the Russian Academy of Sciences, ZA-320M and MTM-500M, obtained series of observations of the potentially dangerous asteroid 65690 (1991 DG) during its approach to the Earth and carried out their astrometric and photometric processing. Using the coordinates of the asteroid and observations from the MRS site, the orbit of the asteroid was clarified, and the circumstances of the approaches to the Earth and Mars were determined, and an assessment was made of the influence of nongravitational effects on its orbit. Based on the results of photometric processing of the asteroid, a light curve was constructed and the period of its axial rotation was determined: P = 4.3193 ± 0.0028 h.

Solar System ResearchVol. 58(5)
Pulkovo Observatory (RU)
Openalex Percentile: Top 89%
Astro and Planetary Science
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