Solar eclipse of November 15, 2096

Future annular solar eclipse
29°42′S 163°18′E / 29.7°S 163.3°E / -29.7; 163.3Max. width of band294 km (183 mi)Times (UTC)Greatest eclipse0:36:15ReferencesSaros144 (21 of 70)Catalog # (SE5000)9725

An annular solar eclipse will occur at the Moon's descending node of orbit between Wednesday, November 14 and Thursday, November 15, 2096, with a magnitude of 0.9237. 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.

Related eclipses

Eclipses in 2096

  • A penumbral lunar eclipse on May 7, 2096.
  • A total solar eclipse on May 22, 2096.
  • A penumbral lunar eclipse on June 6, 2096.
  • A penumbral lunar eclipse on October 31, 2096.
  • An annular solar eclipse on November 15, 2096.
  • A penumbral lunar eclipse on November 29, 2096.

Metonic

Tzolkinex

Half-Saros

  • Preceded by: Lunar eclipse of November 10, 2087
  • Followed by: Lunar eclipse of November 21, 2105

Tritos

Solar Saros 144

Inex

Triad

Solar eclipses of 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

Saros 144

It is a part of Saros cycle 144, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no total eclipses in the series. The series ends at member 70 as a partial eclipse on May 5, 2980. The longest duration of annularity will be 9 minutes, 52 seconds on December 29, 2168.

Series members 11–21 occur between 1901 and 2100:
11 12 13

July 30, 1916

August 10, 1934

August 20, 1952
14 15 16

August 31, 1970

September 11, 1988

September 22, 2006
17 18 19

October 2, 2024

October 14, 2042

October 24, 2060
20 21

November 4, 2078

November 15, 2096

References

  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.

External links

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