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The '''Perseids''' are a prolific [[meteor shower]] associated with the [[comet Swift–Tuttle]]. The meteors are called the Perseids because the point from which they appear to hail (called the [[radiant (meteor shower)|radiant]]) lies in the [[constellation]] [[Perseus (constellation)|Perseus]].
The '''Perseids''' are a prolific [[meteor shower]] associated with the [[comet Swift–Tuttle]]. The meteors are called the Perseids because the point from which they appear to hail (called the [[radiant (meteor shower)|radiant]]) lies in the [[constellation]] [[Perseus (constellation)|Perseus]].

==Etymology==
==Etymology==
The name is derived from the word [[Perseidai]] (Greek : Περσείδαι), the sons of [[Perseus]] in [[Greek mythology]].
The name is derived from the word [[Perseidai]] (Greek : Περσείδαι), the sons of [[Perseus]] in [[Greek mythology]].


==Characteristics==
==Characteristics==
[[File:Perseid Meteors and Comet Swift-Tuttle.png|thumb|A near-Earth perspective of its orbit, the radiant of the Perseid meteor shower, and the orbit of the shower’s parent comet, 109P/Swift-Tuttle, to show their spatial relationships on August 12 00:00 UTC. The Perseid debris cloud is fairly wide (~0.1 AU), filling the frame.]]
[[File:Perseid Meteors and Comet Swift-Tuttle.png|thumb|A near-Earth perspective of its orbit, the radiant of the Perseid meteor shower, and the orbit of the shower's parent comet, 109P/Swift-Tuttle, to show their spatial relationships on August 12 00:00 UTC. The Perseid debris cloud is fairly wide (~0.1 AU), filling the frame.]]
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.<ref>{{cite web|author=Dan Vergano|url=https://www.usatoday.com/story/tech/sciencefair/2013/08/08/perseids-2013-meteor/2628521/ |title=Perseid meteor shower to light up night sky this weekend |publisher=Usatoday.com |date=2010-08-07 |accessdate=2013-08-12}}</ref> 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.<ref>{{Cite web
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.<ref>{{cite web|author=Dan Vergano|url=https://www.usatoday.com/story/tech/sciencefair/2013/08/08/perseids-2013-meteor/2628521/ |title=Perseid meteor shower to light up night sky this weekend |publisher=Usatoday.com |date=2010-08-07 |accessdate=2013-08-12}}</ref> 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.<ref>{{Cite web
|title = The 2004 Perseid Meteor Shower
|title = The 2004 Perseid Meteor Shower
Line 36: Line 37:
|archivedate = March 20, 2010
|archivedate = March 20, 2010
|df =
|df =
}}</ref> 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.<ref>{{Cite book
}}</ref> 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.<ref>{{Cite book
| title = The Cosmic Dust Connection
| title = The Cosmic Dust Connection
| editor = J. Mayo Greenberg
| editor = J. Mayo Greenberg
Line 44: Line 45:
| author= D.W. Hughes
| author= D.W. Hughes
| page = 375
| page = 375
| url = https://books.google.com/books?id=5MH0CAAAQBAJ&pg=PA375
| accessdate = 2015-07-24
| url = https://books.google.com/books?id=5MH0CAAAQBAJ&lpg=PA373&ots=GgKojXHkNT&dq=perseid%20dust%20stream&pg=PA375#v=onepage&q=perseid%20dust%20stream&f=false
}}</ref>
}}</ref>


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]].<ref>{{cite web|url=https://www.timeanddate.com/astronomy/meteor-shower/perseid.html|publisher=timeanddate.com|title=Perseids Meteor Shower 2018
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]].<ref>{{cite web|url=https://www.timeanddate.com/astronomy/meteor-shower/perseid.html|publisher=timeanddate.com|title=Perseids Meteor Shower 2018
|accessdate=2018-07-30}}</ref> 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.<ref>http://meteorshowersonline.com/what_is.html</ref> While many meteors arrive between dawn and noon, they are usually not visible due to daylight. Some can also be seen before midnight, often [[Earth-grazing fireball|grazing the Earth’s atmosphere]] to produce long bright trails and sometimes fireballs. Most Perseids burn up in the atmosphere while at heights above {{convert|80|km|mi}}.<ref name="Meteorwatch"/>
|accessdate=2018-07-30}}</ref> 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.<ref>http://meteorshowersonline.com/what_is.html</ref> While many meteors arrive between dawn and noon, they are usually not visible due to daylight. Some can also be seen before midnight, often [[Earth-grazing fireball|grazing the Earth's atmosphere]] to produce long bright trails and sometimes fireballs. Most Perseids burn up in the atmosphere while at heights above {{convert|80|km|mi}}.<ref name="Meteorwatch"/>
[[File:The 2010 Perseids over the VLT.jpg|thumb|The 2010 Perseids over the [[ESO]]'s [[Very Large Telescope|VLT]]]]
[[File:The 2010 Perseids over the VLT.jpg|thumb|The 2010 Perseids over the [[ESO]]'s [[Very Large Telescope|VLT]]]]
{| style="margin:auto; clear:left" | class="wikitable"
{| style="margin:auto; clear:left" | class="wikitable"
Line 58: Line 58:
|style="text-align:center;"|2018
|style="text-align:center;"|2018
|style="text-align:center;"|July 17 – August 24
|style="text-align:center;"|July 17 – August 24
|August 11-13<ref>{{cite web|url=https://www.space.com/32868-perseid-meteor-shower-guide.html|publisher=Space.com|title=Perseid Meteor Shower 2018: When, Where & How to See It|author=Sarah Lewin|date=July 9, 2018|accessdate=20 July 2018}}</ref> ([[Zenithal Hourly Rate|ZHR<sub>max</sub>]] 60)
|August 11–13<ref>{{cite web|url=https://www.space.com/32868-perseid-meteor-shower-guide.html|publisher=Space.com|title=Perseid Meteor Shower 2018: When, Where & How to See It|author=Sarah Lewin|date=July 9, 2018|accessdate=20 July 2018}}</ref> ([[Zenithal Hourly Rate|ZHR<sub>max</sub>]] 60)
|-
|-
|style="text-align:center;"|2017
|style="text-align:center;"|2017

Revision as of 14:39, 25 December 2018

For the mythological term, see Perseides. For the Mycenaean royal house, see Perseid dynasty.
Perseids (PER)
Perseids in 2017 as seen from the White Desert, Egypt
Pronunciation/ˈpɜːrsiɪdz/
Discovery date36 CE (first record)[1][2]
Parent bodyComet Swift–Tuttle[3]
Radiant
ConstellationPerseus
Right ascension03h 04m [3]
Declination+58°[3]
Properties
Occurs duringJuly 17 – August 24
Date of peakAugust 12
Velocity58[4] km/s
Zenithal hourly rate100[3]
See also: List of meteor showers

The Perseids are a prolific meteor shower associated with the comet Swift–Tuttle. The meteors are called the Perseids because the point from which they appear to hail (called the radiant) lies in the constellation Perseus.

Etymology

The name is derived from the word Perseidai (Greek : Περσείδαι), the sons of Perseus in Greek mythology.

Characteristics

A near-Earth perspective of its orbit, the radiant of the Perseid meteor shower, and the orbit of the shower's parent comet, 109P/Swift-Tuttle, to show their spatial relationships on August 12 00:00 UTC. The Perseid debris cloud is fairly wide (~0.1 AU), filling the frame.

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.[5] 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.[6] 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.[7]

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.[8] 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.[9] 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).[10]

The 2010 Perseids over the ESO's VLT
Year Perseids active between Peak of shower
2018 July 17 – August 24 August 11–13[11] (ZHRmax 60)
2017 July 17 – August 24 August 12[12]
2016 July 17 – August 24 August 11–12 [13] (ZHRmax 150)
2015 July 17 – August 24 August 12–13[14] (ZHRmax 95) (New moon Aug 14)
2014 July 17 – August 24 August 13 (ZHRmax 68)[15] (Full moon Aug 10)
2013 July 17 – August 24 August 12 (ZHRmax 109)[16]
2012 July 17 – August 24 August 12 (ZHRmax 122)[17]
2011 July 17 – August 24 August 12 (ZHRmax 58)[18] (Full moon Aug 13)[19]
2010 July 23 – August 24 August 12 (ZHRmax 142)[20]
2009 July 14 – August 24 August 13 (ZHRmax 173) (the estimated peak was 173,[21] but fainter meteors were washed out by a gibbous Moon.)
2008 July 25 – August 24[22] August 13 (ZHRmax 116)[22]
2007 July 19 – August 25[23] August 13 (ZHRmax 93)[23]
2006 August 12/13 (ZHRmax 100)[24]
2005 August 12 (ZHR max 90[25])[26]
2004 August 12 (ZHRmax >200)[4]
1994 (ZHRmax >200)[2]
1993 (ZHRmax 200–500)[2]
1992 August 11 outburst under an August 13 full moon[27]
1883 August 9 or earlier[28] August 11 (ZHRmax 43)[28]
1864 (ZHRmax >100)[2]
1863 (ZHRmax 109–215)[2]
1861 (ZHRmax 78–102)[2]
1858 (ZHRmax 37–88)[2]
1839 (ZHRmax 165)[2]

Historical observations and associations

A Perseid in 2007

Some Catholics refer to the Perseids as the "tears of Saint Lawrence", suspended in the sky but returning to earth once a year on August 10, the canonical date of that saint's martyrdom in 258 AD.[29] The saint is said to have been burned alive on a gridiron, and this tradition is almost certainly the origin of the Mediterranean folk legend that the shooting stars are the sparks of that fire and that during the night of August 9–10 its cooled embers appear in the ground under plants, and which are known as the "coal of Saint Lawrence".[30][31] The transition in favor of the Catholic saint and his feast day on August 10 and away from pagan gods and their festivals, known as Christianization, was facilitated by the phonetic assonance of the Latin name Laurentius with Larentia.[32][33]

In 1835, Adolphe Quetelet identified the shower as emanating from the constellation Perseus.[1][2] In 1866, after the perihelion passage of Swift-Tuttle in 1862, the Italian astronomer Giovanni Virginio Schiaparelli discovered the link between meteor showers and comets. The finding is contained in an exchange of letters with Angelo Secchi.

In his song "Rocky Mountain High", American singer-songwriter John Denver refers to his experience watching the Perseid meteor shower during a family camping trip in the mountains near Aspen, Colorado, with the chorus lyric, "I've seen it raining fire in the sky."

In the popular Japanese band Sandaime J Soul Brothers's song "R.Y.U.S.E.I" (Meteor), they describe the Perseid meteor as falling like an evening rain shower – its shooting stars like raindrops pulling their tails behind them.

In the song “RPG,” by Japanese band Sekai no Owari, the narrator mentions watching the Perseid meteor shower on the night something “precious to them fell apart.”

References

  1. ^ a b Dr. Bill Cooke; Danielle Moser; Rhiannon Blaauw (2012-08-11). "NASA Chat: Stay 'Up All Night' to Watch the Perseids!" (PDF). NASA. p. 55. Retrieved 2013-08-16. {{cite web}}: Unknown parameter |last-author-amp= ignored (|name-list-style= suggested) (help)
  2. ^ a b c d e f g h i Gary W. Kronk. "Observing the Perseids". Meteor Showers Online. Retrieved 2009-08-12.
  3. ^ a b c d Moore, Patrick; Rees, Robin (2011), Patrick Moore's Data Book of Astronomy (2nd ed.), Cambridge University Press, p. 275, ISBN 0521899354
  4. ^ a b Żołądek, P.; et al. (October 2009), "The 2004 Perseid meteor shower – Polish Fireball Network double station preliminary results", Journal of the International Meteor Organization, 37 (5): 161–163, Bibcode:2009JIMO...37..161Z
  5. ^ Dan Vergano (2010-08-07). "Perseid meteor shower to light up night sky this weekend". Usatoday.com. Retrieved 2013-08-12.
  6. ^ Dr. Tony Phillips (June 25, 2004). "The 2004 Perseid Meteor Shower". Science@NASA. Archived from the original on March 20, 2010. Retrieved 2010-03-12. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  7. ^ D.W. Hughes (1996). "Cometary Dust Loss: Meteoroid Streams and the Inner Solar System Dust Cloud". In J. Mayo Greenberg (ed.). The Cosmic Dust Connection. Springer Science & Business Media. p. 375.
  8. ^ "Perseids Meteor Shower 2018". timeanddate.com. Retrieved 2018-07-30.
  9. ^ http://meteorshowersonline.com/what_is.html
  10. ^ "NASA All Sky Fireball Network: Perseid End Height". NASA Meteor Watch on Facebook. 2012-08-11. Retrieved 2012-11-19.
  11. ^ Sarah Lewin (July 9, 2018). "Perseid Meteor Shower 2018: When, Where & How to See It". Space.com. Retrieved 20 July 2018.
  12. ^ Sarah Lewin (July 26, 2017). "Perseid Meteor Shower 2017: When, Where & How to See It". Space.com. Retrieved 27 July 2017.
  13. ^ "Perseid Meteor Shower 2016: When, Where & How to See It". Retrieved 2016-07-18.
  14. ^ "Meteor Showers 2015". NASA. Retrieved 2015-08-09.
  15. ^ "Perseids 2014: visual data quicklook". Imo.net. 2014-08-13. Archived from the original on 2016-10-24. Retrieved 2014-08-13. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  16. ^ "Perseids 2013: visual data quicklook". Imo.net. 2013-09-23. Archived from the original on 2016-10-24. Retrieved 2014-04-20. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  17. ^ "Perseids 2012: visual data quicklook". Imo.net. 2012-10-22. Archived from the original on 2014-04-21. Retrieved 2014-04-20. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  18. ^ "Perseids 2011: visual data quicklook". Imo.net. 2011-10-06. Archived from the original on 2013-11-06. Retrieved 2014-04-20. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  19. ^ "How to See the Best Meteor Showers of the Year: Tools, Tips and 'Save the Dates'". nasa.gov. Retrieved 2010-11-16.
  20. ^ "How to See the Best Meteor Showers of the Year: Tools, Tips and 'Save the Dates'". nasa.gov. Retrieved 2010-08-12.
  21. ^ "Perseids 2009: visual data quicklook". Imo.net. 2010-04-26. Archived from the original on 2016-10-16. Retrieved 2009-08-11. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  22. ^ a b "Perseids 2008: visual data quicklook". Imo.net. 2009-06-06. Archived from the original on 2016-10-24. Retrieved 2009-08-11. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  23. ^ a b Perseids 2007: first results Archived 2011-09-27 at the Wayback Machine
  24. ^ EAAS
  25. ^ http://www.imo.net/perseids-2005-visual/
  26. ^ https://science.nasa.gov/science-news/science-at-nasa/2005/22jul_perseids2005
  27. ^ Brown. "The Perseids 1992. New outburst announces return of P/Swift-Tuttle". Bibcode:1992JIMO...20..192B. {{cite journal}}: Cite journal requires |journal= (help)
  28. ^ a b Corder, H (22 October 1883). "1883Obs.....6..338C Page 338". adsabs.harvard.edu. Retrieved 3 November 2018.
  29. ^ "Science: Tears of St. Lawrence". TIME. 1926-08-23. Retrieved 2009-08-12.
  30. ^ Template:It Falling stars and coal under the basil
  31. ^ Template:It The Coal of Saint Lawrence
  32. ^ Template:It Castrum Inui
  33. ^ "SHOOTING STARS". utestudents BLOG.
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