CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory

Resultado de la investigación

Resumen

CCD photometry of six asteroids was obtained at the Universidad de Monterrey Observatory during January and February 2008. The resulting synodic rotation periods and amplitudes are as follows: 1292 Luce, 6.9541 ± 0.0002 h, 0.20 ± 0.01 mag; 1303 Luthera, 5.878 ± 0.003 h, 0.08 ± 0.01 mag; 1900 Katyusha, 9.4999 ± 0.0001 h, 0.72 ± 0.02 mag, 2807 Karl Marx, 8.842 ± 0.001 h, 0.40 ± 0.05 mag; 3409 Abramov, 7.791 ± 0.002 h, 0.55 ± 0.02 mag; and 9117 Aude, 2.8156 ± 0.0001 h, 0.20 ± 0.01 mag.
Idioma originalEnglish
Páginas (desde-hasta)105-107
PublicaciónThe Minor Planet Bulletin
Volumen35
EstadoPublished - 1 sep 2008

Huella Profundice en los temas de investigación de 'CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory'. En conjunto forman una huella única.

  • Citar esto