Solar eclipse of March 28, 1968
Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse occurred at the Moon's ascending node of orbit between Thursday, March 28 and Friday, March 29, 1968,[1] with a magnitude of 0.899. 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 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 of eastern Oceania and Antarctica.
Eclipse details
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 | 1968 March 28 at 20:44:13.8 UTC |
| Equatorial Conjunction | 1968 March 28 at 21:53:55.7 UTC |
| Ecliptic Conjunction | 1968 March 28 at 22:48:36.8 UTC |
| Greatest Eclipse | 1968 March 28 at 23:00:30.4 UTC |
| Last Penumbral External Contact | 1968 March 29 at 01:17:17.4 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.89902 |
| Eclipse Obscuration | 0.84205 |
| Gamma | −1.03704 |
| Sun Right Ascension | 00h30m35.2s |
| Sun Declination | +03°18'09.3" |
| Sun Semi-Diameter | 16'01.0" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 00h32m24.8s |
| Moon Declination | +02°28'24.8" |
| Moon Semi-Diameter | 14'57.5" |
| Moon Equatorial Horizontal Parallax | 0°54'53.9" |
| ΔT | 38.5 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| March 28 Ascending node (new moon) |
April 13 Descending node (full moon) |
|---|---|
| File:SE1968Mar28P.png | File:Lunar eclipse chart close-1968Apr13.png |
| Partial solar eclipse Solar Saros 119 |
Total lunar eclipse Lunar Saros 131 |
Related eclipses
Eclipses in 1968
- A partial solar eclipse on March 28.
- A total lunar eclipse on April 13.
- A total solar eclipse on September 22.
- A total lunar eclipse on October 6.
Metonic
- Preceded by: Solar eclipse of June 10, 1964
- Followed by: Solar eclipse of January 16, 1972
Tzolkinex
- Preceded by: Solar eclipse of February 15, 1961
- Followed by: Solar eclipse of May 11, 1975
Half-Saros
- Preceded by: Lunar eclipse of March 24, 1959
- Followed by: Lunar eclipse of April 4, 1977
Tritos
- Preceded by: Solar eclipse of April 30, 1957
- Followed by: Solar eclipse of February 26, 1979
Solar Saros 119
- Preceded by: Solar eclipse of March 18, 1950
- Followed by: Solar eclipse of April 9, 1986
Inex
- Preceded by: Solar eclipse of April 19, 1939
- Followed by: Solar eclipse of March 9, 1997
Triad
- Preceded by: Solar eclipse of May 27, 1881
- Followed by: Solar eclipse of January 27, 2055
Solar eclipses of 1968–1971
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.[3]
The partial solar eclipse on July 22, 1971 occurs in the next lunar year eclipse set.
| Solar eclipse series sets from 1968 to 1971 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | March 28, 1968 File:SE1968Mar28P.png Partial |
−1.037 | 124 | September 22, 1968 File:SE1968Sep22T.png Total |
0.9451 | |
| 129 | March 18, 1969 File:SE1969Mar18A.png Annular |
−0.2704 | 134 | September 11, 1969 File:SE1969Sep11A.png Annular |
0.2201 | |
| 139 File:C72pct (4321372614).jpg Totality in Williamston, NC USA |
March 7, 1970 File:SE1970Mar07T.png Total |
0.4473 | 144 | August 31, 1970 File:SE1970Aug31A.png Annular |
−0.5364 | |
| 149 | February 25, 1971 File:SE1971Feb25P.png Partial |
1.1188 | 154 | August 20, 1971 File:SE1971Aug20P.png Partial |
−1.2659 | |
Saros 119
Template:Solar Saros series 119
Metonic series
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.
| 20 eclipse events between June 10, 1964 and August 21, 2036 | ||||
|---|---|---|---|---|
| June 10–11 | March 28–29 | January 14–16 | November 3 | August 21–22 |
| 117 | 119 | 121 | 123 | 125 |
| File:SE1964Jun10P.png June 10, 1964 |
File:SE1968Mar28P.png March 28, 1968 |
File:SE1972Jan16A.png January 16, 1972 |
File:SE1975Nov03P.png November 3, 1975 |
File:SE1979Aug22A.png August 22, 1979 |
| 127 | 129 | 131 | 133 | 135 |
| File:SE1983Jun11T.png June 11, 1983 |
File:SE1987Mar29H.png March 29, 1987 |
File:SE1991Jan15A.png January 15, 1991 |
File:SE1994Nov03T.png November 3, 1994 |
File:SE1998Aug22A.png August 22, 1998 |
| 137 | 139 | 141 | 143 | 145 |
| File:SE2002Jun10A.png June 10, 2002 |
File:SE2006Mar29T.png March 29, 2006 |
File:SE2010Jan15A.png January 15, 2010 |
File:SE2013Nov03H.png November 3, 2013 |
File:SE2017Aug21T.png August 21, 2017 |
| 147 | 149 | 151 | 153 | 155 |
| File:SE2021Jun10A.png June 10, 2021 |
File:SE2025Mar29P.png March 29, 2025 |
File:SE2029Jan14P.png January 14, 2029 |
File:SE2032Nov03P.png November 3, 2032 |
File:SE2036Aug21P.png August 21, 2036 |
Tritos series
Template:Solar Tritos series 2000 December 25
Inex series
Template:Solar Inex series 2026 February 17
References
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External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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