Solar eclipse of November 15, 2096
Map
Type of eclipse
Nature	Annular
Gamma	−0.20
Magnitude	0.9237
Maximum eclipse
Duration	533 s (8 min 53 s)
Coordinates	29°42′S 163°18′E / 29.7°S 163.3°E / -29.7; 163.3
Max. width of band	294 km (183 mi)
Times (UTC)
Greatest eclipse	0:36:15
References
Saros	144 (21 of 70)
Catalog # (SE5000)	9725

An annular solar eclipse will occur on Wednesday, November 14 and Thursday, November 15, 2096. 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

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

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
Jul 30, 1916	Aug 10, 1934	Aug 20, 1952
14	15	16
Aug 31, 1970	Sep 11, 1988	Sep 22, 2006
17	18	19
Oct 2, 2024	Oct 14, 2042	Oct 24, 2060
20	21
Nov 4, 2078	Nov 15, 2096