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

Resultado de la investigación

Resumen

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.
Idioma originalEnglish
Páginas (desde-hasta)233-234
PublicaciónThe Minor Planet Bulletin
Volumen45
N.º3
EstadoPublished - 1 jul 2018

Huella Profundice en los temas de investigación de 'Lightcurves for Asteroids 2022 West and 18301 Konyukhov'. En conjunto forman una huella única.

  • Citar esto

    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