Solar_eclipse_of_June_28,_1908 Knowpia

Solar eclipse of June 28, 1908
Solar eclipse of June 28, 1908
	Map
Type of eclipse
Nature	Annular
Gamma	0.1389
Magnitude	0.9655
Maximum eclipse
Duration	240 s (4 min 0 s)
Coordinates	31°24′N 67°12′W / 31.4°N 67.2°W
Max. width of band	126 km (78 mi)
Times (UTC)
Greatest eclipse	16:29:51
References
Saros	135 (33 of 71)
Catalog # (SE5000)	9300

An annular solar eclipse occurred on June 28, 1908.^[1]^[2]^[3] 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.

Places inside the annular eclipse included a part of North America including a part of Central Mexico around Mexico City and Orlando and Daytona Beach, Florida in the USA which occurred in the morning hours. In Africa, it included Rosso, Mauritania, the northernmost part of Senegal, Bamako and the southwestern French Sudan (now Mali), the southwesternmost part of Upper Volta (now Burkina Faso) and northern British Gold Coast (now Ghana) which occurred before sunset.

Related eclipses edit

Solar eclipses 1906–1909 edit

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.^[4]

Solar eclipse series sets from 1906 to 1909
Ascending node		Descending node
115	July 21, 1906 Partial	120	January 14, 1907 Total
125	July 10, 1907 Annular	130	January 3, 1908 Total
135	June 28, 1908 Annular	140	December 23, 1908 Hybrid
145	June 17, 1909 Hybrid	150	December 12, 1909 Partial

Saros 135 edit

It is a part of Saros cycle 135, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305, hybrid eclipses on March 8, 2323 and March 18, 2341 and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. The longest duration of totality will be 2 minutes, 27 seconds on May 12, 2431.

Series members 27–43 occur between 1800 and 2100:
27	28	29
Apr 24, 1800	May 5, 1818	May 15, 1836
30	31	32
May 26, 1854	Jun 6, 1872	Jun 17, 1890
33	34	35
Jun 28, 1908	Jul 9, 1926	Jul 20, 1944
36	37	38
Jul 31, 1962	Aug 10, 1980	Aug 22, 1998
39	40	41
Sep 1, 2016	Sep 12, 2034	Sep 22, 2052
42	43
Oct 4, 2070	Oct 14, 2088

Notes edit

^ "Eclipse of the sun visible here Sunday". The Atlanta Constitution. Atlanta, Georgia. 1908-06-27. p. 6. Retrieved 2023-11-01 – via Newspapers.com.
^ "Splendid View of Yesterday's Phenomenon". Daily Mirror. London, London, England. 1908-06-29. p. 3. Retrieved 2023-11-01 – via Newspapers.com.
^ "SUN'S PARTIAL ECLIPSE VIEWED BY THOUSANDS". The Pittsburgh Post. Pittsburgh, Pennsylvania. 1908-06-29. p. 3. Retrieved 2023-11-01 – via Newspapers.com.
^ 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.