Solar eclipse of April 28, 1930
| Solar eclipse of April 28, 1930 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Hybrid |
| Gamma | 0.473 |
| Magnitude | 1.0003 |
| Maximum eclipse | |
| Duration | 1 s (0 min 1 s) |
| Coordinates | 39°24′N 121°12′W / 39.4°N 121.2°W |
| Max. width of band | 1 km (0.62 mi) |
| Times (UTC) | |
| Greatest eclipse | 19:03:34 |
| References | |
| Saros | 137 (31 of 70) |
| Catalog # (SE5000) | 9351 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, April 28, 1930, with a magnitude of 1.0003. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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.
The path of totality crossed the eastern Pacific Ocean, northwestern United States, central and eastern Canada, and northern Labrador of the Dominion of Newfoundland (today's Newfoundland and Labrador in Canada).
Observations[edit]
During a hybrid solar 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 in both the total and annular portion of the path. A series of Baily's beads on the lunar limb provided an excellent opportunity to measure the size and shape of the Earth, as well as the mountains and valleys on the lunar limb. Scientists recorded the precise time of each phase of the eclipse in Camptonville, California. Because the duration of totality was just more than 1 second, the photographic film needed to be inserted quickly after the start of totality. In addition, scientists recorded audio images with a long-wave receiver on an aircraft at the Mare Island Naval Shipyard. Each image had a time accurate to 1/5 second.
Prior to it, the hybrid solar eclipse of April 17, 1912, also belonging to Solar Saros 137, also occurred with a magnitude close to 1. Observations were made near Paris, France. Similar observations were also made during the annular solar eclipses of May 9, 1948 in Rebun Island, Japan and May 20, 1966 in Greece and Turkey, also belonging to the same solar Saros cycle.[1]
Related eclipses[edit]
Eclipses in 1930[edit]
- A partial lunar eclipse on April 13, 1930.
- A hybrid solar eclipse on April 28, 1930.
- A partial lunar eclipse on October 7, 1930.
- A total solar eclipse on October 21, 1930.
Metonic[edit]
- Preceded by: Solar eclipse of July 9, 1926
- Followed by: Solar eclipse of February 14, 1934
Tzolkinex[edit]
- Preceded by: Solar eclipse of March 17, 1923
- Followed by: Solar eclipse of June 8, 1937
Half-Saros[edit]
- Preceded by: Lunar eclipse of April 22, 1921
- Followed by: Lunar eclipse of May 3, 1939
Tritos[edit]
- Preceded by: Solar eclipse of May 29, 1919
- Followed by: Solar eclipse of March 27, 1941
Solar Saros 137[edit]
- Preceded by: Solar eclipse of April 17, 1912
- Followed by: Solar eclipse of May 9, 1948
Inex[edit]
- Preceded by: Solar eclipse of May 18, 1901
- Followed by: Solar eclipse of April 8, 1959
Triad[edit]
- Preceded by: Solar eclipse of June 27, 1843
- Followed by: Solar eclipse of February 26, 2017
Solar eclipses of 1928–1931[edit]
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.[2]
The partial solar eclipse on June 17, 1928 occurs in the previous lunar year eclipse set, and the partial solar eclipse on September 12, 1931 occurs in the next lunar year eclipse set.
| Solar eclipse series sets from 1928 to 1931 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | May 19, 1928 Total (non-central) |
1.0048 | 122 | November 12, 1928 Partial |
1.0861 | |
| 127 | May 9, 1929 Total |
−0.2887 | 132 | November 1, 1929 Annular |
0.3514 | |
| 137 | April 28, 1930 Hybrid |
0.473 | 142 | October 21, 1930 Total |
−0.3804 | |
| 147 | April 18, 1931 Partial |
1.2643 | 152 | October 11, 1931 Partial |
−1.0607 | |
Saros 137[edit]
This eclipse is a part of Saros series 137, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 25, 1389. It contains total eclipses from August 20, 1533 through December 6, 1695; the first set of hybrid eclipses from December 17, 1713 through February 11, 1804; the first set of annular eclipses from February 21, 1822 through March 25, 1876; the second set of hybrid eclipses from April 6, 1894 through April 28, 1930; and the second set of annular eclipses from May 9, 1948 through April 13, 2507. The series ends at member 70 as a partial eclipse on June 28, 2633. 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 11 at 2 minutes, 55 seconds on September 10, 1569, and the longest duration of annularity will be produced by member 59 at 7 minutes, 5 seconds on February 28, 2435. All eclipses in this series occur at the Moon’s ascending node of orbit.[3]
| Series members 24–46 occur between 1801 and 2200: | ||
|---|---|---|
| 24 | 25 | 26 |
 February 11, 1804 |
 February 21, 1822 |
 March 4, 1840 |
| 27 | 28 | 29 |
 March 15, 1858 |
 March 25, 1876 |
 April 6, 1894 |
| 30 | 31 | 32 |
 April 17, 1912 |
April 28, 1930 |
 May 9, 1948 |
| 33 | 34 | 35 |
 May 20, 1966 |
 May 30, 1984 |
 June 10, 2002 |
| 36 | 37 | 38 |
 June 21, 2020 |
 July 2, 2038 |
 July 12, 2056 |
| 39 | 40 | 41 |
 July 24, 2074 |
 August 3, 2092 |
 August 15, 2110 |
| 42 | 43 | 44 |
 August 25, 2128 |
 September 6, 2146 |
 September 16, 2164 |
| 45 | 46 | |
 September 27, 2182 |
 October 9, 2200 | |
Inex series[edit]
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.
| Inex series members between 1901 and 2100: | ||
|---|---|---|
 May 18, 1901 (Saros 136) |
April 28, 1930 (Saros 137) |
 April 8, 1959 (Saros 138) |
 March 18, 1988 (Saros 139) |
 February 26, 2017 (Saros 140) |
 February 5, 2046 (Saros 141) |
 January 16, 2075 (Saros 142) |
||
Notes[edit]
- ^ Xavier M. Jubier. "Eclipse hybride de Soleil du 28 avril 1930 depuis l'ouest des États-Unis ou l'est du Canada (Hybrid Solar Eclipse of 1930 April 28 in western USA or eastern Canada)". Archived from the original on 11 January 2019.
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
- ^ "NASA - Catalog of Solar Eclipses of Saros 137". eclipse.gsfc.nasa.gov.
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- The solar eclipse of April 28, 1930 Popular Astronomy, Vol. 38, p. 537, Makemson, Maud W. [1]
- The Central Solar Eclipse of April 28, 1930 Journal of the Royal Astronomical Society of Canada, Vol. 24, p. 55 [2]
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