To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
Languages
Recent
Show all languages
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

Solar eclipse of November 27, 2095

From Wikipedia, the free encyclopedia

Solar eclipse of November 27, 2095
Map
Type of eclipse
NatureAnnular
Gamma0.4903
Magnitude0.933
Maximum eclipse
Duration527 sec (8 m 47 s)
Coordinates7°12′N 169°48′E / 7.2°N 169.8°E / 7.2; 169.8
Max. width of band285 km (177 mi)
Times (UTC)
Greatest eclipse1:02:57
References
Saros134 (48 of 71)
Catalog # (SE5000)9723

An annular solar eclipse will occur on November 27, 2095. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

YouTube Encyclopedic

  • 1/3
    Views:
    2 112
    2 145
    2 159
  • Impresionantes Eclipses Lunares.TIPOS / Amazing Lunar Eclipses. TYPES [IGEO.TV]
  • 15th June 2014 Madeenah Fajr led by Sheikh Hameed
  • Saturday January 5, 2013: Shemot "Names"

Transcription

Related eclipses

Solar eclipses 2094–2098

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[1]

119 June 13, 2094

Partial
124 December 7, 2094

Partial
129 June 2, 2095

Total
134 November 27, 2095

Annular
139 May 22, 2096

Total
144 November 15, 2096

Annular
149 May 11, 2097

Total
154 November 4, 2097

Annular
  164 October 24, 2098

Partial

Tritos

Tzolkinex

  • Preceded: Solar eclipse of November 15, 2088
  • Followed: Solar eclipse of January 19, 2102

Saros 134

It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428. All eclipses in this series occur at the Moon’s descending node.[2]

Series members 32–48 occur between 1801 and 2100:
32 33 34

June 6, 1807

June 16, 1825

June 27, 1843
35 36 37

July 8, 1861

July 19, 1879

July 29, 1897
38 39 40

August 10, 1915

August 21, 1933

September 1, 1951
41 42 43

September 11, 1969

September 23, 1987

October 3, 2005
44 45 46

October 14, 2023

October 25, 2041

November 5, 2059
47 48

November 15, 2077

November 27, 2095

Notes

  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.

References

This page was last edited on 1 May 2023, at 13:51
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.