A total solar eclipse occurred on April 6, 1875. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible on the southern tip of Africa, across the Indian Ocean, and across southeastern Asia and Northern Philippines.
Solar eclipse of April 6, 1875 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.1292 |
Magnitude | 1.0547 |
Maximum eclipse | |
Duration | 277 s (4 min 37 s) |
Coordinates | 0°12′S 84°48′E / 0.2°S 84.8°E |
Max. width of band | 182 km (113 mi) |
Times (UTC) | |
Greatest eclipse | 6:37:26 |
References | |
Saros | 127 (50 of 82) |
Catalog # (SE5000) | 9222 |
Observations
editAstronomers J. N. Lockyer and Arthur Schuster traveled to observe the eclipse and measure spectral lines to determine the elemental contents of the solar corona.[1]
Related eclipses
editSaros 127
editThis eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 82 events. The series started with a partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular or hybrid eclipses in this set. The series ends at member 82 as a partial eclipse on March 21, 2452. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 31 at 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]
Series members 46–68 occur between 1801 and 2200: | ||
---|---|---|
46 | 47 | 48 |
February 21, 1803 |
March 4, 1821 |
March 15, 1839 |
49 | 50 | 51 |
March 25, 1857 |
April 6, 1875 |
April 16, 1893 |
52 | 53 | 54 |
April 28, 1911 |
May 9, 1929 |
May 20, 1947 |
55 | 56 | 57 |
May 30, 1965 |
June 11, 1983 |
June 21, 2001 |
58 | 59 | 60 |
July 2, 2019 |
July 13, 2037 |
July 24, 2055 |
61 | 62 | 63 |
August 3, 2073 |
August 15, 2091 |
August 26, 2109 |
64 | 65 | 66 |
September 6, 2127 |
September 16, 2145 |
September 28, 2163 |
67 | 68 | |
October 8, 2181 |
October 19, 2199 |
Notes
edit- ^ Lockyer, J. N.; Schuster, Arthur (1878). "Report on the Total Solar Eclipse of April 6, 1875" (PDF). Philosophical Transactions of the Royal Society of London. 169: 139–154. Bibcode:1878RSPT..169..139L. JSTOR 109303.
- ^ "NASA - Catalog of Solar Eclipses of Saros 127". eclipse.gsfc.nasa.gov.