Solar eclipse of April 16, 1893
Map
Type of eclipse
Nature	Total
Gamma	−0.1764
Magnitude	1.0556
Maximum eclipse
Duration	287 s (4 min 47 s)
Coordinates	1°18′N 34°36′W / 1.3°N 34.6°W / 1.3; -34.6
Max. width of band	186 km (116 mi)
Times (UTC)
Greatest eclipse	14:36:11
References
Saros	127 (51 of 82)
Catalog # (SE5000)	9264

A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, April 16, 1893, with a magnitude of 1.0556. 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. Occurring about 1.3 days before perigee (on April 17, 1893, at 21:50 UTC), the Moon's apparent diameter was larger.^[1]

The path of totality was visible from parts of the modern-day countries of Chile, Argentina, Paraguay, Brazil, Senegal, Mauritania, Mali, southern Algeria, Niger, Chad, and Sudan. A partial solar eclipse was also visible for parts of South America, Africa, and Southern Europe.

According to Edward S. Holden, John Martin Schaeberle discovered a comet like object on the plates of the eclipse from Chile. The comet was 0.8 Moon diameters from the Moon.^[2]

Schaeberle observed the eclipse and made drawings of the Corona:

Predicted by Schaeberle	Observed by Schaeberle
Observed by Schaeberle

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.^[3]

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of April 1893

April 16 Ascending node (new moon)	April 30 Descending node (full moon)
Total solar eclipse Solar Saros 127	Penumbral lunar eclipse Lunar Saros 139

• A total solar eclipse on April 16.
• A penumbral lunar eclipse on April 30.
• A penumbral lunar eclipse on September 25.
• An annular solar eclipse on October 9.
• A penumbral lunar eclipse on October 25.

• Preceded by: Solar eclipse of June 28, 1889
• Followed by: Solar eclipse of February 1, 1897

• Preceded by: Solar eclipse of March 5, 1886
• Followed by: Solar eclipse of May 28, 1900

• Preceded by: Lunar eclipse of April 10, 1884
• Followed by: Lunar eclipse of April 22, 1902

• Preceded by: Solar eclipse of May 17, 1882
• Followed by: Solar eclipse of March 17, 1904

• Preceded by: Solar eclipse of April 6, 1875
• Followed by: Solar eclipse of April 28, 1911

• Preceded by: Solar eclipse of May 6, 1864
• Followed by: Solar eclipse of March 28, 1922

• Preceded by: Solar eclipse of June 16, 1806
• Followed by: Solar eclipse of February 16, 1980

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]

The partial solar eclipse on August 20, 1895 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1892 to 1895
Ascending node				Descending node
Saros	Map	Gamma		Saros	Map	Gamma
117	April 26, 1892 Total	−0.8870		122	October 20, 1892 Partial	1.0286
127	April 16, 1893 Total	−0.1764		132	October 9, 1893 Annular	0.2866
137	April 6, 1894 Hybrid	0.5740		142	September 29, 1894 Total	−0.4573
147	March 26, 1895 Partial	1.3565		152	September 18, 1895 Partial	−1.1469

This 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.^[5]

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

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). All eclipses in this table occur at the Moon's ascending node.

23 eclipse events between February 3, 1859 and June 29, 1946
February 1–3	November 21–22	September 8–10	June 28–29	April 16–18
109	111	113	115	117
February 3, 1859	November 21, 1862		June 28, 1870	April 16, 1874
119	121	123	125	127
February 2, 1878	November 21, 1881	September 8, 1885	June 28, 1889	April 16, 1893
129	131	133	135	137
February 1, 1897	November 22, 1900	September 9, 1904	June 28, 1908	April 17, 1912
139	141	143	145	147
February 3, 1916	November 22, 1919	September 10, 1923	June 29, 1927	April 18, 1931
149	151	153	155
February 3, 1935	November 21, 1938	September 10, 1942	June 29, 1946

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
December 21, 1805 (Saros 119)	November 19, 1816 (Saros 120)	October 20, 1827 (Saros 121)	September 18, 1838 (Saros 122)	August 18, 1849 (Saros 123)
July 18, 1860 (Saros 124)	June 18, 1871 (Saros 125)	May 17, 1882 (Saros 126)	April 16, 1893 (Saros 127)	March 17, 1904 (Saros 128)
February 14, 1915 (Saros 129)	January 14, 1926 (Saros 130)	December 13, 1936 (Saros 131)	November 12, 1947 (Saros 132)	October 12, 1958 (Saros 133)
September 11, 1969 (Saros 134)	August 10, 1980 (Saros 135)	July 11, 1991 (Saros 136)	June 10, 2002 (Saros 137)	May 10, 2013 (Saros 138)
April 8, 2024 (Saros 139)	March 9, 2035 (Saros 140)	February 5, 2046 (Saros 141)	January 5, 2057 (Saros 142)	December 6, 2067 (Saros 143)
November 4, 2078 (Saros 144)	October 4, 2089 (Saros 145)	September 4, 2100 (Saros 146)	August 4, 2111 (Saros 147)	July 4, 2122 (Saros 148)
June 3, 2133 (Saros 149)	May 3, 2144 (Saros 150)	April 2, 2155 (Saros 151)	March 2, 2166 (Saros 152)	January 29, 2177 (Saros 153)
December 29, 2187 (Saros 154)	November 28, 2198 (Saros 155)

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
June 16, 1806 (Saros 124)	May 27, 1835 (Saros 125)	May 6, 1864 (Saros 126)
April 16, 1893 (Saros 127)	March 28, 1922 (Saros 128)	March 7, 1951 (Saros 129)
February 16, 1980 (Saros 130)	January 26, 2009 (Saros 131)	January 5, 2038 (Saros 132)
December 17, 2066 (Saros 133)	November 27, 2095 (Saros 134)	November 6, 2124 (Saros 135)
October 17, 2153 (Saros 136)	September 27, 2182 (Saros 137)

• NASA graphics
  • Googlemap
  • NASA Besselian elements
• Fotos of Solar Corona April 16, 1893
• [1],[2], [3] Eclipse of April 16, 1893. Contact print from the original glass plate negative.] Lick Observatory Plate Archive, Mt. Hamilton.
• Mabel Loomis Todd (1900). Total Eclipses of the Sun. Little, Brown.

v t e Solar eclipses
Features	Baily's beads (diamond ring) Shadow bands Solar prominence Stellar corona helmet streamer
Lists of eclipses	By era Antiquity Middle Ages Modern era 16th 17th 18th 19th 20th 21st 22nd Future Saros series (list) 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 Visibility Australia British Isles China Israel Philippines Russia Turkey Ukraine United States Historical Mursili's eclipse (1312 BC) Assyrian eclipse (763 BC) Eclipse of Thales (585 BC) Muhammad's eclipse (632 AD)
Total/hybrid eclipses → next total/hybrid	1133 1185 1560 1598 1652 1654 1673 1706 1715 1724 1766 1778 1780 1806 1816 1824 1842 1851 1853 1857 1858 1860 1865 1867 1868 1869 1870 1871 1874 1875 1878 1882 1883 1885 1886 1887 Jan. 1889 Dec. 1889 1893 1896 1898 1900 1901 1903 1904 1905 1907 Jan. 1908 Dec. 1908 1909 1910 1911 Apr. 1912 Oct. 1912 1914 1916 1918 1919 1921 1922 1923 1925 1926 1927 1928 1929 Apr. 1930 Oct. 1930 1932 1934 1936 1937 1938 1939 1940 1941 1943 Jan. 1944 1945 1947 1948 1950 1952 1954 1955 1956 1957 1958 1959 1961 1962 1963 1965 1966 1967 1968 1970 1972 1973 1974 1976 1977 1979 1980 1981 1983 1984 1985 1986 1987 1988 1990 1991 1992 1994 1995 1997 1998 1999 2001 2002 2003 2005 2006 2008 2009 2010 2012 2013 2015 2016 2017 2019 2020 2021 2023 2024 → 2026 2027 2028 2030 2031 2033 2034 2035 2037 2038 2039 2041 2042 2043 2044 2045 2046 2048 2049 2050 2052 2053 2055 Jan. 2057 Dec. 2057 2059 2060 2061 2063 2064 2066 2067 2068 2070 2071 2072 2073 2075 2076 2077 2078 2079 2081 2082 2084 2086 2088 2089 2090 2091 2093 2094 2095 2096 2097 2099 2100 2186
Annular eclipses → next annular	1820 1854 1879 1889 1900 1901 1903 1904 1905 1907 1908 1911 1914 Feb. 1915 Aug. 1915 1916 1917 1918 1919 1921 1922 1923 1925 1926 1927 1929 1932 Feb. 1933 Aug. 1933 1934 1935 1936 1937 1939 1940 1941 1943 Jul. 1944 1945 1947 1948 1950 Mar. 1951 Sep. 1951 1952 Jan. 1954 Dec. 1954 1955 1957 1958 1959 1961 1962 1963 1965 1966 Mar. 1969 Sep. 1969 1970 1972 Jan. 1973 Dec. 1973 1976 1977 1979 1980 1981 1983 1984 1987 1988 1990 1991 1992 1994 1995 1998 1999 2001 2002 2003 2005 2006 2008 2009 2010 2012 2013 2014 2016 2017 2019 2020 2021 2023 → 2024 2026 2027 2028 2030 2031 2032 2034 2035 2036 Jan. 2038 Jul. 2038 2039 2041 2042 2043 2044 2045 2046 2048 2049 2052 2053 Jan. 2056 Jul. 2056 2057 2059 2060 2061 2063 2064 2066 2067 2070 2071 Jan. 2074 Jul. 2074 2075 2077 2078 2079 2081 2082 2084 Jun. 2085 Dec. 2085 2088 2089 Feb. 2092 Aug. 2092 2093 2095 2096 2097 2099 2100
Partial eclipses → next partial	Jan. 1639 Nov. 1873 Apr. 1902 May 1902 Oct. 1902 Feb. 1906 Jul. 1906 Aug. 1906 Dec. 1909 Nov. 1910 Apr. 1913 Aug. 1913 Sep. 1913 Dec. 1916 Jan. 1917 Jun. 1917 Jul. 1917 May 1920 Nov. 1920 Mar. 1924 Jul. 1924 Aug. 1924 Dec. 1927 Jun. 1928 Nov. 1928 Apr. 1931 Sep. 1931 Oct. 1931 Jan. 1935 Feb. 1935 Jun. 1935 Jul. 1935 Nov. 1938 Mar. 1942 Aug. 1942 Sep. 1942 Jan. 1946 May 1946 Jun. 1946 Nov. 1946 Apr. 1949 Oct. 1949 Feb. 1953 Jul. 1953 Aug. 1953 Dec. 1956 Mar. 1960 Sep. 1960 Jan. 1964 Jun. 1964 Jul. 1964 Dec. 1964 May 1967 Mar. 1968 Feb. 1971 Jul. 1971 Aug. 1971 Dec. 1974 May 1975 Nov. 1975 Apr. 1978 Oct. 1978 Jan. 1982 Jun. 1982 Jul. 1982 Dec. 1982 May 1985 Apr. 1986 Mar. 1989 Aug. 1989 Dec. 1992 May 1993 Nov. 1993 Apr. 1996 Oct. 1996 Sep. 1997 Feb. 2000 1 Jul. 2000 31 Jul. 2000 Dec. 2000 Apr. 2004 Oct. 2004 Mar. 2007 Sep. 2007 Jan. 2011 Jun. 2011 Jul. 2011 Nov. 2011 Oct. 2014 Sep. 2015 Feb. 2018 Jul. 2018 Aug. 2018 Jan. 2019 Apr. 2022 Oct. 2022 → Mar. 2025 Sep. 2025 Jan. 2029 Jun. 2029 Jul. 2029 Dec. 2029 2032 2033 Feb. 2036 Jul. 2036 Aug. 2036 2037 May 2040 Nov. 2040 Jan. 2047 Jun. 2047 Jul. 2047 Dec. 2047 2050 Apr. 2051 Oct. 2051 Mar. 2054 Aug. 2054 Sep. 2054 2055 May 2058 Jun. 2058 Nov. 2058 Mar. 2062 Sep. 2062 Feb. 2065 Jul. 2065 Aug. 2065 Dec. 2065 2068 Apr. 2069 May 2069 Oct. 2069 2072 2073 Jun. 2076 Jul. 2076 Nov. 2076 Feb. 2083 Jul. 2083 Aug. 2083 2084 2086 May 2087 Jun. 2087 Oct. 2087 2090 2091 Jun. 2094 Jul. 2094 Dec. 2094 Apr. 2098 Sep. 2098 Oct. 2098
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