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

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

Departamento de Física y Matemáticas

Research output: Contribution to journal › Article › peer-review

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 language	English
Pages (from-to)	233-234
Journal	The Minor Planet Bulletin
Volume	45
Issue number	3
Publication status	Published - 1 Jul 2018

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http://adsabs.harvard.edu/abs/2018MPBu...45..233H

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@article{7182fbeb281643c2be6de6b5edcac8db,

title = "Lightcurves for Asteroids 2022 West and 18301 Konyukhov",

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.}",

year = "2018",

month = jul,

day = "1",

language = "English",

volume = "45",

pages = "233--234",

journal = "The Minor Planet Bulletin",

issn = "1052-8091",

number = "3",

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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

SN - 1052-8091

VL - 45

SP - 233

EP - 234

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

IS - 3

ER -

Lightcurves for Asteroids 2022 West and 18301 Konyukhov

Abstract

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