Hostname: page-component-6bf8c574d5-8gtf8 Total loading time: 0 Render date: 2025-02-17T11:58:53.308Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometry and spin rates of 4 NEAs recently observed by the Mexican Asteroid Photometry Campaign

Published online by Cambridge University Press:  03 March 2020

J. C. Saucedo ,
S. A. Ayala-Gómez ,
M. E. Contreras ,
S. A. R. Haro-Corzo ,
P. A. Loera-González ,
L. Olgun  and
P. A. Valdés-Sada
J. C. Saucedo
Affiliation:
Departamento de Investigación en Fsica, Universidad de Sonora Blvd. Rosales y Colosio, Ed. 3H, 83190Hermosillo, Sonora, México email: [email protected]
S. A. Ayala-Gómez
Affiliation:
FCFM–Universidad Autónoma de Nuevo León
M. E. Contreras
Affiliation:
Departamento de Investigación en Fsica, Universidad de Sonora Blvd. Rosales y Colosio, Ed. 3H, 83190Hermosillo, Sonora, México email: [email protected]
S. A. R. Haro-Corzo
Affiliation:
ENES–Universidad Nacional Autónoma de México
P. A. Loera-González
Affiliation:
Departamento de Investigación en Fsica, Universidad de Sonora Blvd. Rosales y Colosio, Ed. 3H, 83190Hermosillo, Sonora, México email: [email protected]
L. Olgun
Affiliation:
Departamento de Investigación en Fsica, Universidad de Sonora Blvd. Rosales y Colosio, Ed. 3H, 83190Hermosillo, Sonora, México email: [email protected]
P. A. Valdés-Sada
Affiliation:
DFM–Universidad de Monterrey
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present photometric observations of (4055) Magellan, (143404) 2003 BD44, 2014 JO25 and (3122) Florence, four potentially hazardous Near Earth Asteroids (NEAs). The data were taken near their approaches to Earth by 3 observatories participating in the Mexican Asteroid Photometry Campaign (CMFA). The results obtained: light curves, spin rates, amplitudes and errors, are in general agreement with those obtained by others. During the day of a NEAs maximum approach to our planet, its light curve may present significant changes. In the spin rate, however, only minute changes are observed. 2014 JO25 is briefly discussed in this regard.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 31 - 34
Copyright
© International Astronomical Union 2020

References

Birlan, M., Vaduvescu, O., Tudorica, A., Sonka, A., Nedelcu, A., Galad, A. Colas, F., Pozo, N. F., Barr, A., Toma, R., Comsa, I., Rocher, P., Lainey, V., Vidican, D., Asher, D., Opriseanu, C., Vancea, C., Colque, J. P., Soto, C.P., Rekola, R., and Unda-Sanzana, E., 2010, A&A, 511, A40 Google Scholar
Durech, J.D, Sidorin, V., and Kaasalainen, M., 2010, A&A, 513, A46 Google Scholar
Franco, L., Bacci, P., Maestripieri, M., Baj, G., Battista, G., Galli, G., Marchini, A., Noschese, A., Valvasori, A., Caselli, C., Barbieri, L., Facchini, M. , 2017, MPBu 45, 174 Google Scholar
Haro-Corzo, S. A. R., Villegas, L. A., Olgun, L., Saucedo, J. C., Contreras, M. E., Sada, P. V., Ayala, S. A., Garza, J. R., Segura-Sosa, J. & Bentez-Bentez, C. P., 2018, MPBu, 45, 233 Google Scholar
Sada, P. V., Navarro-Meza, S., Reyes-Ruiz, M., Olgun, L., Saucedo, J. C., Loera-González, P., 2016, MPBu, 43, 154 Google Scholar
Sada, P. V., Olgun, L., Saucedo, J. C., Loera-González, P., Cantú-Sánchez, L., Garza, J. R., Ayala-Gómez, S. A., Avilés, A., Pérez-Tijerina, E., Navarro-Meza, S., Silva, J.S., Reyes-Ruiz, M., Segura-Sosa, J., López-Valdivia, R., & Álvarez-Santana, F., 2017, MPBu, 44, 239 Google Scholar
Sada, P., Loera-González, P., Olgun, L., Saucedo-Morales, J. C., Ayala, S. A.& Garza, J. R., 2018, MPBu, 45, 122 Google Scholar
Stetson, P., 1987, PASP, 99, 191 CrossRefGoogle Scholar
Waszczak, A., Chang, C. K., Ofek, E. O., Laher, R., Masci, F., Levitan, D., Surace, J., Cheng, Y. C., Huen, W., Kinoshita, D., Helou, G., Prince, T. A., and Kulkarniet, S., 2015, AJ, 150, 35 CrossRefGoogle Scholar
Vaduvescu, O., 2017a, MPBu, 44, 335 Google Scholar
Warner, B. D., 2017b, MPBu, 44, 327 Google Scholar