Ursids

History

The Ursids were probably discovered by William F. Denning, who observed them for several years around the start of the 20th century. While there were sporadic observations after, the first coordinated studies of the shower didn't begin until Dr. A. Bečvář observed an outburst of 169 per hour in 1945. Further observations in the 1970s and ongoing to current have established a relationship with comet 8P/Tuttle. Peter Jenniskens and Esko Lyytinen discovered that outbursts could happen when comet Tuttle was at aphelion because some meteoroids get trapped in the 7/6 orbital resonance with Jupiter.

Technical information

Earlier observations described an average radiant of RA=, DEC=, with maximum occurring at a solar longitude of 270.66 deg (about December 22), with the duration being established as December 17–24.

The Ursids have a particularly narrow stream, prompting veteran meteor observer, Norman W. McLeod, III (Florida) to comment that the Ursids "must be a compact stream like the Quadrantids. You have to be within 12 hours of maximum to see much."

References

|author-link=Gary W. Kronk |archive-url=https://web.archive.org/web/20130724160438/http://meteorshowersonline.com/showers/ursids.html |archive-date=2013-07-24 |url-status=dead |access-date=2012-11-17}}

References

1. [https://www.imo.net/resources/calendar/#Ursids IMO Meteor Shower Calendar: Ursids (URS)]
2. (2011). "Patrick Moore's Data Book of Astronomy". [[Cambridge University Press]].