Lightcurves for Asteroids 2022 West and 18301 Konyukhov

Sinhue A. R. Haro-Corzo, Luis A. Villegas, Lorenzo Olguin, Julio C. Saucedo, Maria E. Contreras, Pedro V. Sada, Sandra A. Ayala, Jaime R. Garza, Juan Segura-Sosa, Claudia P. Benitez-Benitez

Research output: Contribution to journalArticle

Abstract

We report photometric analysis of two main-belt asteroids observed at the Observatorio Astronomico Nacional in the Sierra San Pedro Martir, Baja California, México. For 18301 Konyukhov, our derived intrinsic rotation period is 2.6667 ± 0.0003 h with an amplitude of 0.16 mag. 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 ± 0.0031 h with an amplitude of 0.54 mag.
Original languageEnglish
Pages (from-to)233-234
JournalThe Minor Planet Bulletin
Volume45
Issue number3
Publication statusPublished - 1 Jul 2018

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    Haro-Corzo, S. A. R., Villegas, L. A., Olguin, L., Saucedo, J. C., Contreras, M. E., Sada, P. V., Ayala, S. A., Garza, J. R., Segura-Sosa, J., & Benitez-Benitez, C. P. (2018). Lightcurves for Asteroids 2022 West and 18301 Konyukhov. The Minor Planet Bulletin, 45(3), 233-234. http://adsabs.harvard.edu/abs/2018MPBu...45..233H