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The Quadrantids (QUA) are a meteor shower that peaks in early January and whose radiant lies in the constellation Boötes.The zenithal hourly rate (ZHR) of this shower can be as high as that of two other reliably rich meteor showers, the Perseids in August and the Geminids in December, [4] yet Quadrantid meteors are not seen as often as those of the two other showers because the time frame of ...
After the Quadrantids, there is a bit of a lull in meteor shower activity, and the next one won’t occur until April. Here are the remaining showers to anticipate and their peak dates in 2025 ...
Peak activity is predicted to occur from 10 p.m. to 1 a.m. EST, during which the Quadrantids can produce about 120 meteors per hour, according to the AMS. Quadrantids, 1st meteor shower of 2025 ...
The Quadrantid meteor shower peaks between Thursday, Jan. 2 and Friday, Jan. 3 this year. They are predicted to be the strongest on Jan. 3 at 12:45 p.m. ET, according to the American Meteor Society.
This list of meteor streams and peak activity times is based on data from the International Meteor Organization while most of the parent body associations are from Gary W. Kronk book, Meteor Showers: A Descriptive Catalog, Enslow Publishers, New Jersey, ISBN 0-89490-071-4, and from Peter Jenniskens's book, "Meteor Showers and Their Parent ...
The Geminids are a prolific meteor shower with 3200 Phaethon (which is thought to be an Apollo asteroid [4] with a "rock comet" orbit. [5]) being the parent body. [6]Because of this, it would make this shower, along with the Quadrantids, the only major meteor showers not originating from a comet.
The best time to see Quadrantids meteor shower in North American will be around 5 a.m. to dawn. Here are some tips for viewing.
In 2007 astronomers determined that the annual January Quadrantid meteor shower may have originated with the disintegration of Comet C/1490 Y1, approximately a century after it was first identified in 1490 by Chinese, Japanese, and Korean astronomers. [9] [10] A connection with asteroid (196256) 2003 EH 1 has also been suggested. [4]