Lightcurves for asteroids 18301 Konyukhov and 2022 West

Sinhué A. R. Haro-Corzo; Luis A. Villegas; Lorenzo Olguín; Julio C. Saucedo; María E. Contreras; Pedro V. Sada; Sandra A. Ayala; Jaime R. Garza; Juan Segura-Sosa; Claudia P. Benítez-Benítez

Lightcurves for asteroids 18301 Konyukhov and 2022 West

Earth and Planetary Astrophysics 2018-06-14 v1

Authors: Sinhué A. R. Haro-Corzo , Luis A. Villegas , Lorenzo Olguín , Julio C. Saucedo , María E. Contreras , Pedro V. Sada , Sandra A. Ayala , Jaime R. Garza , Juan Segura-Sosa , Claudia P. Benítez-Benítez

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Abstract

We report photometric analysis of two main-belt asteroids observed at the Observatorio Astronomico Nacional in the Sierra San Pedro Martir, Baja California, M\'exico. For 18301 Konyukhov our derived intrinsic rotation period is 2.6667 $\pm$ 0.0003 h with an amplitude of 0.16 magnitudes. To the best of our knowledge, this is the first lightcurve reported for this asteroid. In the case of 2022 West our derived intrinsic rotation period is 14.1385 $\pm$ 0.0031 h with an amplitude of 0.54 magnitudes.

Keywords

asteroids lightcurves rotation period photometric analysis main-belt asteroids

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@article{arxiv.1806.05041,
  title  = {Lightcurves for asteroids 18301 Konyukhov and 2022 West},
  author = {Sinhué A. R. Haro-Corzo and Luis A. Villegas and Lorenzo Olguín and Julio C. Saucedo and María E. Contreras and Pedro V. Sada and Sandra A. Ayala and Jaime R. Garza and Juan Segura-Sosa and Claudia P. Benítez-Benítez},
  journal= {arXiv preprint arXiv:1806.05041},
  year   = {2018}
}

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2 pages, 2 figures

Lightcurves for asteroids 18301 Konyukhov and 2022 West

Abstract

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