| Total eclipse | |
 Map | |
| Gamma | 0.4207 |
|---|---|
| Magnitude | 1.0325 |
| Maximum eclipse | |
| Duration | 182 s (3 min 2 s) |
| Coordinates | 20°24′N1°24′W / 20.4°N 1.4°W /20.4; -1.4 |
| Max. width of band | 120 km (75 mi) |
| Times (UTC) | |
| Greatest eclipse | 12:27:00 |
| References | |
| Saros | 143 (20 of 72) |
| Catalog # (SE5000) | 9419 |
A totalsolar eclipse occurred at the Moon'sascending node of orbit on Friday, October 2, 1959,[1] with amagnitude of 1.0325. 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 total solar eclipse occurs when the Moon'sapparent 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 2.4 days beforeperigee (on October 4, 1959, at 21:10 UTC), the Moon's apparent diameter was larger.[2]
Totality was visible from northeasternMassachusetts and the southern tip ofNew Hampshire in theUnited States, theCanary Islands,Morocco,Spanish Sahara (today'sWest Sahara) including the capital cityLaayoune,French Mauritania (today'sMauritania),Mali Federation (part now belonging toMali),French Niger (today'sNiger),British Nigeria (today'sNigeria),British Cameroons andFrench Cameroons (now belonging toCameroon),French Chad (today'sChad) including the capital cityFort-Lamy, French Central Africa (today'sCentral African Republic),Sudan (part of the path of totality is now inSouth Sudan),Ethiopia, and theTrust Territory of Somaliland (today'sSomalia). A partial eclipse was visible for parts of easternNorth America, the easternCaribbean,Europe,Africa,West Asia, andCentral Asia.
Totality began overBoston, Massachusetts at sunrise. Viewing the eclipse was rained out, but it was reported that the brightening of the sky after the eclipse was a startling and impressive sight.[3] A few photographers captured the eclipse from airplanes above the clouds, and a multiple exposure was made atop the R. C. A. building in New York City.[4] The next total eclipse over Boston, thesolar eclipse of May 1, 2079, will also be a sunrise event.[5]
The event was also observed at the Canarian Island of Fuerteventura by a team of Dutch astronomers of the university of Utrecht and Amsterdam.[6][7]
Maurice Allais, a Frenchpolymath, reported the alleged anomalous behavior ofpendulums orgravimeters, later named asAllais effect. He first reported the effect after observing thesolar eclipse of June 30, 1954, and reported another observation of the effect during this solar eclipse using theparaconical pendulum he invented.[8]
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.[9]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1959 October 2 at 09:49:42.6 UTC |
| First Umbral External Contact | 1959 October 2 at 10:50:25.8 UTC |
| First Central Line | 1959 October 2 at 10:50:55.8 UTC |
| First Umbral Internal Contact | 1959 October 2 at 10:51:25.7 UTC |
| First Penumbral Internal Contact | 1959 October 2 at 12:08:39.3 UTC |
| Equatorial Conjunction | 1959 October 2 at 12:12:52.0 UTC |
| Greatest Eclipse | 1959 October 2 at 12:27:00.1 UTC |
| Greatest Duration | 1959 October 2 at 12:29:26.6 UTC |
| Ecliptic Conjunction | 1959 October 2 at 12:31:24.6 UTC |
| Last Penumbral Internal Contact | 1959 October 2 at 12:45:44.7 UTC |
| Last Umbral Internal Contact | 1959 October 2 at 14:02:42.2 UTC |
| Last Central Line | 1959 October 2 at 14:03:14.3 UTC |
| Last Umbral External Contact | 1959 October 2 at 14:03:46.4 UTC |
| Last Penumbral External Contact | 1959 October 2 at 15:04:19.6 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.03251 |
| Eclipse Obscuration | 1.06608 |
| Gamma | 0.42075 |
| Sun Right Ascension | 12h31m27.3s |
| Sun Declination | -03°23'42.1" |
| Sun Semi-Diameter | 15'58.8" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 12h31m57.6s |
| Moon Declination | -02°59'50.0" |
| Moon Semi-Diameter | 16'15.2" |
| Moon Equatorial Horizontal Parallax | 0°59'39.0" |
| ΔT | 33.0 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.
| September 17 Descending node (full moon) | October 2 Ascending node (new moon) |
|---|---|
 | |
| Penumbral lunar eclipse Lunar Saros 117 | Total solar eclipse Solar Saros 143 |
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.[10]
| Solar eclipse series sets from 1957 to 1960 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | April 30, 1957 Annular (non-central) | 0.9992 | 123 | October 23, 1957 Total (non-central) | 1.0022 | |
| 128 | April 19, 1958 Annular | 0.275 | 133 | October 12, 1958 Total | −0.2951 | |
| 138 | April 8, 1959 Annular | −0.4546 | 143 | October 2, 1959 Total | 0.4207 | |
| 148 | March 27, 1960 Partial | −1.1537 | 153 | September 20, 1960 Partial | 1.2057 | |
This eclipse is a part ofSaros series 143, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 7, 1617. It contains total eclipses from June 24, 1797 throughOctober 24, 1995; hybrid eclipses fromNovember 3, 2013 throughDecember 6, 2067; and annular eclipses fromDecember 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2897. 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 was produced by member 16 at 3 minutes, 50 seconds onAugust 19, 1887, and the longest duration of annularity will be produced by member 51 at 4 minutes, 54 seconds on September 6, 2518. All eclipses in this series occur at the Moon’sascending node of orbit.[11]
| Series members 12–33 occur between 1801 and 2200: | ||
|---|---|---|
| 12 | 13 | 14 |
 July 6, 1815 |  July 17, 1833 |  July 28, 1851 |
| 15 | 16 | 17 |
 August 7, 1869 |  August 19, 1887 |  August 30, 1905 |
| 18 | 19 | 20 |
 September 10, 1923 |  September 21, 1941 | October 2, 1959 |
| 21 | 22 | 23 |
 October 12, 1977 |  October 24, 1995 |  November 3, 2013 |
| 24 | 25 | 26 |
 November 14, 2031 |  November 25, 2049 |  December 6, 2067 |
| 27 | 28 | 29 |
 December 16, 2085 |  December 29, 2103 |  January 8, 2122 |
| 30 | 31 | 32 |
 January 20, 2140 |  January 30, 2158 |  February 10, 2176 |
| 33 | ||
 February 21, 2194 | ||
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 ascending node.
| 22 eclipse events between December 13, 1898 and July 20, 1982 | ||||
|---|---|---|---|---|
| December 13–14 | October 1–2 | July 20–21 | May 9 | February 24–25 |
| 111 | 113 | 115 | 117 | 119 |
 December 13, 1898 |  July 21, 1906 |  May 9, 1910 |  February 25, 1914 | |
| 121 | 123 | 125 | 127 | 129 |
 December 14, 1917 |  October 1, 1921 |  July 20, 1925 |  May 9, 1929 |  February 24, 1933 |
| 131 | 133 | 135 | 137 | 139 |
 December 13, 1936 |  October 1, 1940 |  July 20, 1944 |  May 9, 1948 |  February 25, 1952 |
| 141 | 143 | 145 | 147 | 149 |
 December 14, 1955 | October 2, 1959 |  July 20, 1963 |  May 9, 1967 |  February 25, 1971 |
| 151 | 153 | 155 | ||
 December 13, 1974 |  October 2, 1978 |  July 20, 1982 | ||
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.
The partial solar eclipses on December 18, 2188 (part of Saros 164) and November 18, 2199 (part of Saros 165) are also a part of this series but are not included in the table below.
| Series members between 1801 and 2134 | ||||
|---|---|---|---|---|
 December 10, 1806 (Saros 129) |  November 9, 1817 (Saros 130) |  October 9, 1828 (Saros 131) |  September 7, 1839 (Saros 132) |  August 7, 1850 (Saros 133) |
 July 8, 1861 (Saros 134) |  June 6, 1872 (Saros 135) |  May 6, 1883 (Saros 136) |  April 6, 1894 (Saros 137) |  March 6, 1905 (Saros 138) |
 February 3, 1916 (Saros 139) |  January 3, 1927 (Saros 140) |  December 2, 1937 (Saros 141) |  November 1, 1948 (Saros 142) | October 2, 1959 (Saros 143) |
 August 31, 1970 (Saros 144) |  July 31, 1981 (Saros 145) |  June 30, 1992 (Saros 146) |  May 31, 2003 (Saros 147) |  April 29, 2014 (Saros 148) |
 March 29, 2025 (Saros 149) |  February 27, 2036 (Saros 150) |  January 26, 2047 (Saros 151) |  December 26, 2057 (Saros 152) |  November 24, 2068 (Saros 153) |
 October 24, 2079 (Saros 154) |  September 23, 2090 (Saros 155) |  August 24, 2101 (Saros 156) |  July 23, 2112 (Saros 157) |  June 23, 2123 (Saros 158) |
 May 23, 2134 (Saros 159) | ||||
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 10, 1815 (Saros 138) |  December 21, 1843 (Saros 139) |  November 30, 1872 (Saros 140) |
 November 11, 1901 (Saros 141) |  October 21, 1930 (Saros 142) | October 2, 1959 (Saros 143) |
 September 11, 1988 (Saros 144) |  August 21, 2017 (Saros 145) |  August 2, 2046 (Saros 146) |
 July 13, 2075 (Saros 147) |  June 22, 2104 (Saros 148) |  June 3, 2133 (Saros 149) |
 May 14, 2162 (Saros 150) |  April 23, 2191 (Saros 151) | |
.jpg)
