| Solar eclipse of April 28, 1911 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Total |
| Gamma | −0.2294 |
| Magnitude | 1.0562 |
| Maximum eclipse | |
| Duration | 297 sec (4 m 57 s) |
| Coordinates | 1°54′N 151°54′W / 1.9°N 151.9°W |
| Max. width of band | 190 km (120 mi) |
| Times (UTC) | |
| Greatest eclipse | 22:27:22 |
| References | |
| Saros | 127 (52 of 82) |
| Catalog # (SE5000) | 9306 |
A total solar eclipse occurred on 28 April 1911.[1][2][3] 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. Totality was visible from southeastern tip of Australia, Tonga, American Samoa and Cook Islands. Places west of International Date Line witnessed the eclipse on Saturday 29 April 1911.
Related eclipses
Solar eclipses 1910–1913
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.[4]
| Solar eclipse series sets from 1910–1913 | ||||
|---|---|---|---|---|
| Ascending node | Descending node | |||
| 117 | May 9, 1910 Total |
122 | November 2, 1910 Partial | |
| 127 | April 28, 1911 Total |
132 | October 22, 1911 Annular | |
| 137 | April 17, 1912 Hybrid |
142 | October 10, 1912 Total | |
| 147 | April 6, 1913 Partial |
152 | September 30, 1913 Partial | |
Saros 127
It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular eclipses in this series. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occurs at the Moon’s ascending node.[5]
| Series members 52–68 occur between 1901 and 2200 | ||
|---|---|---|
| 52 | 53 | 54 |
April 28, 1911 |
 May 9, 1929 |
 May 20, 1947 |
| 55 | 56 | 57 |
 May 30, 1965 |
 June 11, 1983 |
 June 21, 2001 |
| 58 | 59 | 60 |
 July 2, 2019 |
 July 13, 2037 |
 July 24, 2055 |
| 61 | 62 | 63 |
 August 3, 2073 |
 August 15, 2091 |
August 26, 2109 (Partial) |
| 64 | 65 | 66 |
| September 6, 2127 (Partial | September 16, 2145 (Partial) | September 28, 2163 (Partial) |
| 67 | 68 | |
| October 8, 2181 (Partial) | October 19, 2199 (Partial) | |
See also
Notes
- ↑ "SOLAR ECLIPSE TODAY WILL BE ADVANTAGE TO SCIENCE". Billings Evening Journal. Billings, Montana. 1911-04-28. p. 3. Retrieved 2023-11-03 – via Newspapers.com.
- ↑ "The eclipse to be seen". The Southern Star. Bega, New South Wales, Australia. 1911-04-29. p. 2. Retrieved 2023-11-03 – via Newspapers.com.
- ↑ "TO-DAY'S SOLAR ECLIPSE". The Sun. Sydney, New South Wales, Australia. 1911-04-29. p. 1. Retrieved 2023-11-03 – via Newspapers.com.
- ↑ 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.
- ↑ "Solar Saros series 127". NASA Goddard Space Flight Center. NASA. Retrieved 2 November 2017.
References
- NASA graphics
- Report on the total solar eclipse of 1911, April 28 Tonga Island, South Pacific
.jpg.webp)
