World Library  
Flag as Inappropriate
Email this Article

Solar eclipse of November 25, 2049

Article Id: WHEBN0025356574
Reproduction Date:

Title: Solar eclipse of November 25, 2049  
Author: World Heritage Encyclopedia
Language: English
Subject: Solar eclipse of December 16, 2047, Solar eclipse of June 23, 2047, Solar eclipse of August 19, 1887, Solar Saros 143, Solar eclipse of July 1, 2076
Collection:
Publisher: World Heritage Encyclopedia
Publication
Date:
 

Solar eclipse of November 25, 2049

Solar eclipse of November 25, 2049
Map
Type of eclipse
Nature Hybrid
Gamma 0.2943
Magnitude 1.0057
Maximum eclipse
Duration 0m 38s
Coordinates 3.8S 95.2E
Max. width of band 21 km
Times (UTC)
Greatest eclipse 5:33:48
References
Saros 143 (25 of 72)
Catalog # (SE5000) 9618

A total solar eclipse will occur on November 25, 2049. It is a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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.

Images


Animated path

Related eclipses

Solar eclipses 2047-2050

Each member 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.

Note: Partial lunar eclises on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2047-2050
Ascending node   Descending node
118 June 23, 2047

Partial
123 December 16, 2047

Partial
128 June 11, 2048

Annular
133 December 5, 2048

Total
138 May 31, 2049

Annular
143 November 25, 2049

Hybrid
148 May 20, 2049

Hybrid
153 November 14, 2050

Partial

Saros 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887.[1]

Series members 17-28 occur between 1901 and 2100:
17 18 19

August 30, 1905

September 10, 1923

September 21, 1941
20 21 22

October 2, 1959

October 12, 1977

October 24, 1995
23 24 25

November 3, 2013

November 14, 2031

November 25, 2049
26 27 28

December 6, 2067

December 16, 2085

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).

This series has 21 eclipse events, progressing from north to south between July 1, 2000 and July 1, 2076.

July 1-2 April 19-20 February 5-7 November 24-25 September 12-13
117 119 121 123 125

July 1, 2000

April 19, 2004

February 7, 2008

November 25, 2011

September 13, 2015
127 129 131 133 135

July 2, 2019

April 20, 2023

February 6, 2027

November 25, 2030

September 12, 2034
137 139 141 143 145

July 2, 2038

April 20, 2042

February 5, 2046

November 25, 2049

September 12, 2053
147 149 151 153 155

July 1, 2057

April 20, 2061

February 5, 2065

November 24, 2068

September 12, 2072
157

July 1, 2076

Notes

  1. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros143.html

References

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements


This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and USA.gov, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for USA.gov and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
 
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
 
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.
 


Copyright © World Library Foundation. All rights reserved. eBooks from Project Gutenberg are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.