1453 Fennia: A Hungaria Binary

Details 1453 Fennia: A Hungaria Binary 1453 Fennia: A Hungaria Binary

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mpbu...35...73w&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 the Hungaria asteroid 1453 Fennia show that it is a binary with a primary rotation period of 4.4121 ± 0.0001 h. The amplitude of the primary lightcurve alone is 0.10 ± 0.01 mag. Mutual eclipse occultation events indicate a lower limit of the secondary-to-primary ratio of 0.28 ± 0.02. The orbital period of the system is 22.99 ± 0.01 h.

Affiliated with

Also associated with

No associations

Rating

1453 Fennia: A Hungaria Binary 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 1453 Fennia: A Hungaria Binary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 1453 Fennia: A Hungaria Binary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1573072