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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asteroids
Lower California (Mexico)
asteroid belts

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Haro-Corzo, S. A. R., Villegas, L. A., Olguin, L., Saucedo, J. C., Contreras, M. E., Sada, P. V., ... Benitez-Benitez, C. P. (2018). Lightcurves for Asteroids 2022 West and 18301 Konyukhov. The Minor Planet Bulletin, 45(3), 233-234.
Haro-Corzo, Sinhue A. R. ; Villegas, Luis A. ; Olguin, Lorenzo ; Saucedo, Julio C. ; Contreras, Maria E. ; Sada, Pedro V. ; Ayala, Sandra A. ; Garza, Jaime R. ; Segura-Sosa, Juan ; Benitez-Benitez, Claudia P. / Lightcurves for Asteroids 2022 West and 18301 Konyukhov. In: The Minor Planet Bulletin. 2018 ; Vol. 45, No. 3. pp. 233-234.
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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{\'e}xico. 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.",
author = "Haro-Corzo, {Sinhue A. R.} and Villegas, {Luis A.} and Lorenzo Olguin and Saucedo, {Julio C.} and Contreras, {Maria E.} and Sada, {Pedro V.} and Ayala, {Sandra A.} and Garza, {Jaime R.} and Juan Segura-Sosa and Benitez-Benitez, {Claudia P.}",
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Haro-Corzo, SAR, Villegas, LA, Olguin, L, Saucedo, JC, Contreras, ME, Sada, PV, Ayala, SA, Garza, JR, Segura-Sosa, J & Benitez-Benitez, CP 2018, 'Lightcurves for Asteroids 2022 West and 18301 Konyukhov', The Minor Planet Bulletin, vol. 45, no. 3, pp. 233-234.

Lightcurves for Asteroids 2022 West and 18301 Konyukhov. / Haro-Corzo, Sinhue A. R.; Villegas, Luis A.; Olguin, Lorenzo; Saucedo, Julio C.; Contreras, Maria E.; Sada, Pedro V.; Ayala, Sandra A.; Garza, Jaime R.; Segura-Sosa, Juan; Benitez-Benitez, Claudia P.

In: The Minor Planet Bulletin, Vol. 45, No. 3, 01.07.2018, p. 233-234.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Lightcurves for Asteroids 2022 West and 18301 Konyukhov

AU - Haro-Corzo, Sinhue A. R.

AU - Villegas, Luis A.

AU - Olguin, Lorenzo

AU - Saucedo, Julio C.

AU - Contreras, Maria E.

AU - Sada, Pedro V.

AU - Ayala, Sandra A.

AU - Garza, Jaime R.

AU - Segura-Sosa, Juan

AU - Benitez-Benitez, Claudia P.

PY - 2018/7/1

Y1 - 2018/7/1

N2 - 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.

AB - 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.

M3 - Article

VL - 45

SP - 233

EP - 234

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

IS - 3

ER -

Haro-Corzo SAR, Villegas LA, Olguin L, Saucedo JC, Contreras ME, Sada PV et al. Lightcurves for Asteroids 2022 West and 18301 Konyukhov. The Minor Planet Bulletin. 2018 Jul 1;45(3):233-234.