A multicolored, long Perseid striking the sky just to the left of Milky Way, 2009
|Discovery date||36 AD (first record)|
|Parent body||Comet Swift–Tuttle|
|Right ascension||03h 04m|
|Date of peak||August 12 (July 23–August 20)|
|Zenithal hourly rate||80|
The Perseids // are a prolific meteor shower associated with the comet Swift–Tuttle. The Perseids are so called because the point from which they appear to come, called the radiant, lies in the constellation Perseus. The name derives in part from the word Perseides (Περσείδες), a term found in Greek mythology referring to the sons of Perseus.
The stream of debris is called the Perseid cloud and stretches along the orbit of the comet Swift–Tuttle. The cloud consists of particles ejected by the comet as it travels on its 133-year orbit. Most of the particles have been part of the cloud for around a thousand years. However, there is also a relatively young filament of dust in the stream that was pulled off the comet in 1865, which can give an early mini-peak the day before the maximum shower. The dimensions of the cloud in the vicinity of the Earth are estimated to be approximately 0.1 astronomical units (AU) across and 0.8 AU along the latter’s orbit, spread out by annual interactions with the Earth’s gravity.
The shower is visible from mid-July each year, with the peak in activity between 9 and 14 August, depending on the particular location of the stream. During the peak, the rate of meteors reaches 60 or more per hour. They can be seen all across the sky; however, because of the shower’s radiant in the constellation of Perseus, the Perseids are primarily visible in the Northern Hemisphere. As with many meteor showers the visible rate is greatest in the pre-dawn hours, since more meteoroids are scooped up by the side of the Earth moving forward into the stream, corresponding to local times between midnight and noon, as can be seen in the accompanying diagram. While many meteors arrive between dawn and noon, they are usually not visible due to daylight. Some can also be seen before midnight, often grazing the Earth’s atmosphere to produce long bright trails and sometimes fireballs. Most Perseids burn up in the atmosphere while at heights above 80 kilometres (50 mi).
|Year||Perseids active between||Peak of shower|
|2015||July 17 – August 24||August 12–13 (ZHRmax 100?) (New moon Aug 14)|
|2014||July 17 – August 24||August 13 (ZHRmax 68) (Full moon Aug 10)|
|2013||July 17 – August 24||August 12 (ZHRmax 109)|
|2012||July 17 – August 24||August 12 (ZHRmax 122)|
|2011||July 17 – August 24||August 12 (ZHRmax 58) (Full moon Aug 13)|
|2010||July 23 – August 24||August 12 (ZHRmax 142)|
|2009||July 14 – August 24||August 13 (ZHRmax 173) (the estimated peak was 173, but fainter meteors were washed out by a gibbous Moon.)|
|2008||July 25 – August 24||August 13 (ZHRmax 116)|
|2007||July 19 – August 25||August 13 (ZHRmax 93)|
|2004||August 12 (ZHRmax >200)|
|1992||August 11 outburst under an Aug 13 full moon|
The earliest information on this meteor shower is found in Chinese annals in A.D. 36. However, credit for recognising the shower's annual appearance is given to Adolphe Quetelet, who reported in 1835 that there was a shower emanating from the constellation Perseus. Some Catholics refer to the Perseids as the "tears of Saint Lawrence", since 10 August is the date of that saint's martyrdom. In Roman times it was believed that the meteor shower were nothing more than an ejaculation of god Inuo-Priapus that fertilized the fields. The transition in favor of the Christian saint Lorenzo was facilitated, as was the case with many other pagan festivals, by the Catholic Church. It is believed that the saint was chosen as phonetically assonant with that of Larentia, female counterpart of Priapus also celebrated during the date of August 10 whit Priapus.
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- "NASA All Sky Fireball Network: Perseid End Height". NASA Meteor Watch on Facebook. 2012-08-11. Retrieved 2012-11-19.
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- "Perseids 2012: visual data quicklook". Imo.net. 2012-10-22. Retrieved 2014-04-20.
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- "How to See the Best Meteor Showers of the Year: Tools, Tips and 'Save the Dates'". nasa.gov. Retrieved 2010-08-12.
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- "Perseids 2008: visual data quicklook". Imo.net. 2009-06-06. Retrieved 2009-08-11.
- Perseids 2007: first results
- Brown. "The Perseids 1992. New outburst announces return of P/Swift-Tuttle". Bibcode:1992JIMO...20..192B.
- "Science: Tears of St. Lawrence". TIME. 1926-08-23. Retrieved 2009-08-12.
- Media related to Perseids at Wikimedia Commons
- Worldwide viewing times for the 2015 Perseids meteor shower
- Gary Kronk's Meteor Showers page
- Perseid Observing Conditions (The International Project for Radio Meteor Observation)
- 2014 Perseids Radio results (RMOB)
- Perseid Visibility Map (2014 NASA Meteoroid Environment Office)
- 2009 Perseid Meteor Fireball
- NASA website on the Perseid shower of 2009
- Sky & Telescope Magazine - Perseids at Their Prime
- 2012 Image of Perseids emanating from the radiant