Solar eclipse of May 30, 1984
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, May 30, 1984,[1] with a magnitude of 0.998. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). The Moon's apparent diameter was near the average diameter because it occurred 6.6 days after apogee (on May 24, 1984, at 2:00 UTC) and 7.8 days before perigee (on June 7, 1984, at 12:20 UTC).[2]
This was the first annular solar eclipse visible in the United States in 33 years.
Annularity was visible in Mexico, Louisiana, Mississippi, Alabama, Georgia, South Carolina, North Carolina and Virginia in the United States, the Azores Islands, Morocco and Algeria. A partial eclipse was visible for parts of Hawaii, North America, Central America, the Caribbean, northern South America, Western Europe, and Northwest Africa.
Observations
During this eclipse, the apex of the moon's umbral cone was very close to the Earth's surface, and the magnitude was very large. The edges of the moon and the sun were very close to each other as seen from the Earth. Images of the chromosphere and Baily's beads on the lunar limb, which are usually only visible during a total solar eclipse, could also be taken. A team of the University of Florida took images, about half of which being those of the chromosphere and the other half the photosphere, in Greenville, South Carolina.[3][4] Jay Pasachoff led a team from Williams College, Massachusetts to Picayune, Mississippi.[5]
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.[6]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1984 May 30 at 13:55:14.3 UTC |
| First Umbral External Contact | 1984 May 30 at 14:57:46.9 UTC |
| First Central Line | 1984 May 30 at 14:58:22.6 UTC |
| Greatest Duration | 1984 May 30 at 14:58:22.6 UTC |
| First Umbral Internal Contact | 1984 May 30 at 14:58:58.3 UTC |
| First Penumbral Internal Contact | 1984 May 30 at 16:06:12.7 UTC |
| Greatest Eclipse | 1984 May 30 at 16:45:41.5 UTC |
| Ecliptic Conjunction | 1984 May 30 at 16:48:44.8 UTC |
| Equatorial Conjunction | 1984 May 30 at 16:53:32.9 UTC |
| Last Penumbral Internal Contact | 1984 May 30 at 17:25:00.1 UTC |
| Last Umbral Internal Contact | 1984 May 30 at 18:32:21.8 UTC |
| Last Central Line | 1984 May 30 at 18:32:54.6 UTC |
| Last Umbral External Contact | 1984 May 30 at 18:33:27.3 UTC |
| Last Penumbral External Contact | 1984 May 30 at 19:35:58.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.99801 |
| Eclipse Obscuration | 0.99602 |
| Gamma | 0.27552 |
| Sun Right Ascension | 04h31m02.1s |
| Sun Declination | +21°52'05.5" |
| Sun Semi-Diameter | 15'46.4" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h30m45.4s |
| Moon Declination | +22°07'14.4" |
| Moon Semi-Diameter | 15'30.3" |
| Moon Equatorial Horizontal Parallax | 0°56'54.1" |
| ΔT | 54.0 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. The first and last eclipse in this sequence is separated by one synodic month.
| May 15 Descending node (full moon) |
May 30 Ascending node (new moon) |
June 13 Descending node (full moon) |
|---|---|---|
| File:Lunar eclipse chart close-1984May15.png | File:SE1984May30A.png | File:Lunar eclipse chart close-1984Jun13.png |
| Penumbral lunar eclipse Lunar Saros 111 |
Annular solar eclipse Solar Saros 137 |
Penumbral lunar eclipse Lunar Saros 149 |
Related eclipses
Eclipses in 1984
- A penumbral lunar eclipse on May 15.
- An annular solar eclipse on May 30.
- A penumbral lunar eclipse on June 13.
- A penumbral lunar eclipse on November 8.
- A total solar eclipse on November 22.
Metonic
- Preceded by: Solar eclipse of August 10, 1980
- Followed by: Solar eclipse of March 18, 1988
Tzolkinex
- Preceded by: Solar eclipse of April 18, 1977
- Followed by: Solar eclipse of July 11, 1991
Half-Saros
- Preceded by: Lunar eclipse of May 25, 1975
- Followed by: Lunar eclipse of June 4, 1993
Tritos
- Preceded by: Solar eclipse of June 30, 1973
- Followed by: Solar eclipse of April 29, 1995
Solar Saros 137
- Preceded by: Solar eclipse of May 20, 1966
- Followed by: Solar eclipse of June 10, 2002
Inex
- Preceded by: Solar eclipse of June 20, 1955
- Followed by: Solar eclipse of May 10, 2013
Triad
- Preceded by: Solar eclipse of July 29, 1897
- Followed by: Solar eclipse of March 31, 2071
Solar eclipses of 1982–1985
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.[7]
The partial solar eclipses on January 25, 1982 and July 20, 1982 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 1982 to 1985 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | June 21, 1982 File:SE1982Jun21P.png Partial |
−1.2102 | 122 | December 15, 1982 File:SE1982Dec15P.png Partial |
1.1293 | |
| 127 | June 11, 1983 File:SE1983Jun11T.png Total |
−0.4947 | 132 | December 4, 1983 File:SE1983Dec04A.png Annular |
0.4015 | |
| 137 | May 30, 1984 File:SE1984May30A.png Annular |
0.2755 | 142 File:Solar eclipse of 22 November 1984.JPG Partial in Gisborne, New Zealand |
November 22, 1984 File:SE1984Nov22T.png Total |
−0.3132 | |
| 147 | May 19, 1985 File:SE1985May19P.png Partial |
1.072 | 152 | November 12, 1985 File:SE1985Nov12T.png Total |
−0.9795 | |
Saros 137
Template:Solar Saros series 137
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.
Tritos series
Template:Solar Tritos series 2006 March 29
Inex series
Template:Solar Inex series 2013 May 10
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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