Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Etymology  





2 Solar noon  





3 Nomenclature  





4 See also  





5 Notes  





6 References  





7 External links  














Noon






العربية
Avañe'
Aymar aru
Azərbaycanca

Banjar
 / Bân-lâm-gú
Bikol Central
Български
Català
Чӑвашла
Čeština
Dansk
الدارجة
Deutsch
Eesti
Ελληνικά
Emiliàn e rumagnòl
Español
Esperanto
Euskara
فارسی
Français
Frysk
Galego

/Hak-kâ-ngî

Hrvatski
Igbo
Bahasa Indonesia
Interlingua
Íslenska
Italiano
עברית
Jawa
Kabɩyɛ

Қазақша
Kiswahili
Kreyòl ayisyen
Latina
Latviešu
Lietuvių
Magyar
Bahasa Melayu
 / Mìng-dĕ̤ng-nḡ
Монгол
Nederlands

Norsk bokmål
Norsk nynorsk
Nouormand
Occitan
Oʻzbekcha / ўзбекча
پنجابی
Papiamentu
پښتو
Plattdüütsch
Polski
Português
Română
Runa Simi
Русский
Scots
Shqip
Sicilianu
Simple English
سنڌي
Slovenčina
Slovenščina
Soomaaliga
کوردی
Српски / srpski
Srpskohrvatski / српскохрватски
Sunda
Suomi
Svenska
ி
Татарча / tatarça
Тоҷикӣ
Türkçe
Українська
اردو
Vahcuengh
Tiếng Vit
Walon
West-Vlams
Winaray


Zazaki
Žemaitėška

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 




In other projects  



Wikimedia Commons
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


Baku Street at Noon (1861) by Alexey Bogolyubov, showing shadows falling vertically in the city of Baku

Noon (ormidday) is 12 o'clock in the daytime. It is written as 12 noon, 12:00 m. (for meridiem, literally 12:00 midday), 12 p.m. (for post meridiem, literally "after midday"), 12 pm, or 12:00 (using a 24-hour clock) or 1200 (military time). Solar noon is the time when the Sun appears to contact the local celestial meridian. This is when the Sun reaches its apparent highest point in the sky, at 12 noon apparent solar time and can be observed using a sundial. The local or clock time of solar noon depends on the date, longitude, and time zone, with Daylight Saving Time tending to place solar noon closer to 1:00pm.[1]

Etymology[edit]

The word noon is derived from Latin nona hora, the ninth canonical hour of the day, in reference to the Western Christian liturgical term Nones (liturgy), (number nine), one of the seven fixed prayer times in traditional Christian denominations. The Roman and Western European medieval monastic day began at 6:00 a.m. (06:00) at the equinox by modern timekeeping, so the ninth hour started at what is now 3:00 p.m. (15:00) at the equinox.[citation needed] In English, the meaning of the word shifted to midday and the time gradually moved back to 12:00 local time – that is, not taking into account the modern invention of time zones. The change began in the 12th century and was fixed by the 14th century.[2]

Solar noon[edit]

Solar noon, also known as the local apparent solar noon and Sun transit time (informally high noon),[3] is the moment when the Sun contacts the observer's meridian (culminationormeridian transit), reaching its highest position above the horizon on that day and casting the shortest shadow. This is also the origin of the terms ante meridiem (a.m.) and post meridiem (p.m.), as noted below. The Sun is directly overhead at solar noon at the Equator on the equinoxes, at the Tropic of Cancer (latitude 23°26′10.0″N) on the June solstice and at the Tropic of Capricorn (23°26′10.0″S) on the December solstice. In the Northern Hemisphere, north of the Tropic of Cancer, the Sun is due south of the observer at solar noon; in the Southern Hemisphere, south of the Tropic of Capricorn, it is due north.

The elapsed time from the local solar noon of one day to the next is exactly 24 hours on only four instances in any given year. This occurs when the effects of Earth's obliquity of ecliptic and its orbital speed around the Sun offset each other. These four days for the current epoch are centered on 11 February, 13 May, 26 July, and 3 November. It occurs at only one particular line of longitude in each instance. This line varies year to year, since Earth's true year is not an integer number of days. This event time and location also varies due to Earth's orbit being gravitationally perturbed by the planets. These four 24-hour days occur in both hemispheres simultaneously. The precise UTC times for these four days also mark when the opposite line of longitude, 180° away, experiences precisely 24 hours from local midnight to local midnight the next day. Thus, four varying great circles of longitude define from year to year when a 24-hour day (noon to noon or midnight to midnight) occurs.

The two longest time spans from noon to noon occur twice each year, around 20 June (24 hours plus 13 seconds) and 21 December (24 hours plus 30 seconds).

The shortest time spans occur twice each year, around 25 March (24 hours minus 18 seconds) and 13 September (24 hours minus 22 seconds).

For the same reasons, solar noon and "clock noon" are usually not the same. The equation of time shows that the reading of a clock at solar noon will be higher or lower than 12:00 by as much as 16 minutes. Additionally, due to the political nature of time zones, as well as the application of daylight saving time, it can be off by more than an hour.

Nomenclature[edit]

In the US, noon is commonly indicated by 12 p.m., and midnight by 12 a.m. While some argue that such usage is "improper"[4] based on the Latin meaning (a.m. stands for ante meridiem and p.m. for post meridiem, meaning "before midday" and "after midday" respectively), digital clocks are unable to display anything else, and an arbitrary decision must be made. An earlier standard of indicating noon as "12M" or "12m" (for "meridies"), which was specified in the U.S. GPO Government Style Manual,[5] has fallen into relative obscurity; the current edition of the GPO makes no mention of it.[6][7][nb 1] However, due to the lack of an international standard, the use of "12 a.m." and "12 p.m." can be confusing. Common alternative methods of representing these times are:

See also[edit]

Notes[edit]

  1. ^ The 29th edition of the U.S. GPO Government Printing Office Style Manual (2000) section 12.9

References[edit]

  1. ^ "The Sun as an Energy Resource".
  • ^ Online Etymology Dictionary
  • ^ "high noon". The Cambridge Advanced Learner's Dictionary & Thesaurus. Cambridge University Press. Retrieved 2016-12-19.
  • ^ Physics Laboratory FAQ "Times of Day"
  • ^ Style manual of the Government Printing Office / (Rev. ed.). Washington, D.C. 1923. hdl:2027/uc1.$b99665.
  • ^ "U.S. GPO Government Printing Office Style Manual Chapter 9". 2008. Retrieved 2009-06-11.
  • ^ "U.S. GPO Government Printing Office Style Manual Chapter 12". 2008. Retrieved 2009-06-11.
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=Noon&oldid=1222417244"

    Categories: 
    Parts of a day
    Time in astronomy
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
    All articles with unsourced statements
    Articles with unsourced statements from July 2023
    Articles that may contain original research from June 2011
    All articles that may contain original research
    Commons category link from Wikidata
    Articles with GND identifiers
    Articles with J9U identifiers
    Articles with LCCN identifiers
     



    This page was last edited on 5 May 2024, at 21:10 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki