| Partial eclipse | |
 Map | |
| Gamma | −1.027 |
|---|---|
| Magnitude | 0.9638 |
| Maximum eclipse | |
| Coordinates | 61°30′S107°30′E / 61.5°S 107.5°E /-61.5; 107.5 |
| Times (UTC) | |
| Greatest eclipse | 21:13:01 |
| References | |
| Saros | 152 (9 of 70) |
| Catalog # (SE5000) | 9397 |
A partialsolar eclipse occurred at the Moon'sdescending node of orbit on Friday, October 21, 1949,[1] with amagnitude of 0.9638. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial eclipse was visible for parts ofAustralia,Oceania, andAntarctica.
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.[2]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1949 October 21 at 19:15:33.6 UTC |
| Greatest Eclipse | 1949 October 21 at 21:13:00.6 UTC |
| Ecliptic Conjunction | 1949 October 21 at 21:23:16.5 UTC |
| Equatorial Conjunction | 1949 October 21 at 22:05:37.5 UTC |
| Last Penumbral External Contact | 1949 October 21 at 23:10:06.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.96380 |
| Eclipse Obscuration | 0.96320 |
| Gamma | −1.02696 |
| Sun Right Ascension | 13h44m32.4s |
| Sun Declination | -10°48'59.9" |
| Sun Semi-Diameter | 16'04.3" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 13h42m37.9s |
| Moon Declination | -11°45'16.5" |
| Moon Semi-Diameter | 16'43.7" |
| Moon Equatorial Horizontal Parallax | 1°01'23.6" |
| ΔT | 29.1 s |
This eclipse is part of aneclipse 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 afortnight.
| October 7 Ascending node (full moon) | October 21 Descending node (new moon) |
|---|---|
 | |
| Total lunar eclipse Lunar Saros 126 | Partial solar eclipse Solar Saros 152 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[3]
The partial solar eclipses onJanuary 3, 1946 andJune 29, 1946 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 1946 to 1949 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | May 30, 1946 Partial | −1.0711 | 122 | November 23, 1946 Partial | 1.105 | |
| 127 | May 20, 1947 Total | −0.3528 | 132 | November 12, 1947 Annular | 0.3743 | |
| 137 | May 9, 1948 Annular | 0.4133 | 142 | November 1, 1948 Total | −0.3517 | |
| 147 | April 28, 1949 Partial | 1.2068 | 152 | October 21, 1949 Partial | −1.027 | |
This eclipse is a part ofSaros series 152, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 26, 1805. It contains total eclipses fromNovember 2, 1967 through September 14, 2490; hybrid eclipses from September 26, 2508 through October 17, 2544; and annular eclipses from October 29, 2562 through June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality will be produced by member 30 at 5 minutes, 16 seconds on June 9, 2328, and the longest duration of annularity will be produced by member 53 at 5 minutes, 20 seconds on February 16, 2743. All eclipses in this series occur at the Moon’sdescending node of orbit.[4]
| Series members 1–22 occur between 1805 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
 July 26, 1805 |  August 6, 1823 |  August 16, 1841 |
| 4 | 5 | 6 |
 August 28, 1859 |  September 7, 1877 |  September 18, 1895 |
| 7 | 8 | 9 |
 September 30, 1913 |  October 11, 1931 | October 21, 1949 |
| 10 | 11 | 12 |
 November 2, 1967 |  November 12, 1985 |  November 23, 2003 |
| 13 | 14 | 15 |
 December 4, 2021 |  December 15, 2039 |  December 26, 2057 |
| 16 | 17 | 18 |
 January 6, 2076 |  January 16, 2094 |  January 29, 2112 |
| 19 | 20 | 21 |
 February 8, 2130 |  February 19, 2148 |  March 2, 2166 |
| 22 | ||
 March 12, 2184 | ||
Themetonic 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 descending node.
| 22 eclipse events between March 16, 1866 and August 9, 1953 | ||||
|---|---|---|---|---|
| March 16–17 | January 1–3 | October 20–22 | August 9–10 | May 27–29 |
| 108 | 110 | 112 | 114 | 116 |
 March 16, 1866 |  August 9, 1877 |  May 27, 1881 | ||
| 118 | 120 | 122 | 124 | 126 |
 March 16, 1885 |  January 1, 1889 |  October 20, 1892 |  August 9, 1896 |  May 28, 1900 |
| 128 | 130 | 132 | 134 | 136 |
 March 17, 1904 |  January 3, 1908 |  October 22, 1911 |  August 10, 1915 |  May 29, 1919 |
| 138 | 140 | 142 | 144 | 146 |
 March 17, 1923 |  January 3, 1927 |  October 21, 1930 |  August 10, 1934 |  May 29, 1938 |
| 148 | 150 | 152 | 154 | |
 March 16, 1942 |  January 3, 1946 | October 21, 1949 |  August 9, 1953 | |
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 1982 | ||||
|---|---|---|---|---|
 November 29, 1807 (Saros 139) |  October 29, 1818 (Saros 140) |  September 28, 1829 (Saros 141) |  August 27, 1840 (Saros 142) |  July 28, 1851 (Saros 143) |
 June 27, 1862 (Saros 144) |  May 26, 1873 (Saros 145) |  April 25, 1884 (Saros 146) |  March 26, 1895 (Saros 147) |  February 23, 1906 (Saros 148) |
 January 23, 1917 (Saros 149) |  December 24, 1927 (Saros 150) |  November 21, 1938 (Saros 151) | October 21, 1949 (Saros 152) |  September 20, 1960 (Saros 153) |
 August 20, 1971 (Saros 154) |  July 20, 1982 (Saros 155) | |||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 | ||
|---|---|---|
 January 30, 1805 (Saros 147) |  January 9, 1834 (Saros 148) |  December 21, 1862 (Saros 149) |
 December 1, 1891 (Saros 150) |  November 10, 1920 (Saros 151) | October 21, 1949 (Saros 152) |
 October 2, 1978 (Saros 153) |  September 11, 2007 (Saros 154) |  August 21, 2036 (Saros 155) |
 August 2, 2065 (Saros 156) |  July 12, 2094 (Saros 157) |  June 23, 2123 (Saros 158) |
 June 3, 2152 (Saros 159) |  May 13, 2181 (Saros 160) | |
.jpg)
