Lightcurve Photometry and H-G Parameters for 1077 Campanula

Details Lightcurve Photometry and H-G Parameters for 1077 Campanula Lightcurve Photometry and H-G Parameters for 1077 Campanula

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012mpbu...39...67f&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Physics

Scientific paper

Photometric observations of main-belt asteroid 1077 Campanula ware made at two observatories over 10 nights from 2011 September-November. Analysis of the resulting data found a synodic period P = 3.85085 ± 0.00005 h with an amplitude AV = 0.24 ± 0.01 mag (corrected to zero phase). The measured absolute magnitude, H = 12.50 ± 0.02 mag, slope parameter G = 0.24 ± 0.03, and color index V-R = 0.40 ± 0.07 mag are consistent with a medium albedo M or S-type object. The diameter is estimated to be D = 9 ± 2 km.

Affiliated with

Also associated with

No associations

Rating

Lightcurve Photometry and H-G Parameters for 1077 Campanula does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Lightcurve Photometry and H-G Parameters for 1077 Campanula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Lightcurve Photometry and H-G Parameters for 1077 Campanula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1119259