Summary
A partial solar eclipse will occur on Tuesday, April 11, 2051. 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.
| Solar eclipse of April 11, 2051 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | 1.0169 |
| Magnitude | 0.9849 |
| Maximum eclipse | |
| Coordinates | 71°36′N 32°12′E / 71.6°N 32.2°E |
| Times (UTC) | |
| Greatest eclipse | 2:10:39 |
| References | |
| Saros | 120 (63 of 71) |
| Catalog # (SE5000) | 9621 |
The umbral shadow of the Moon will pass just above the north pole of the Earth. It will be the largest partial solar eclipse in 21st century.[1]
The maximal phase of the partial eclipse (0.98) will be recorded in Barents Sea. The eclipse will be observed on the north-east of Europe and practically throughout in Asia, on north on Canada and Greenland and everywhere in US state Alaska.
Related eclipses edit
Solar eclipses 2051–2054 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]
| Solar eclipse series sets from 2051 to 2054 | ||||
|---|---|---|---|---|
| Descending node | Ascending node | |||
| Saros | Map | Saros | Map | |
| 120 | April 11, 2051 Partial |
125 | October 4, 2051 Partial | |
| 130 | March 30, 2052 Total |
135 | September 22, 2052 Annular | |
| 140 | March 20, 2053 Annular |
145 | September 12, 2053 Total | |
| 150 | March 9, 2054 Partial |
155 | September 2, 2054 Partial | |
Saros 120 edit
This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and total eclipses from June 8, 1564, through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon’s descending node.
| Series members 55–65 occur between 1901 and 2100 | |||
|---|---|---|---|
| 55 | 56 | 57 | |
 January 14, 1907 |
 January 24, 1925 |
 February 4, 1943 | |
| 58 | 59 | 60 | |
 February 15, 1961 |
 February 26, 1979 |
 March 9, 1997 | |
| 61 | 62 | 63 | |
 March 20, 2015 |
 March 30, 2033 |
April 11, 2051 64 65  April 21, 2069 |
 May 2, 2087 |
References edit
External links edit
- http://eclipse.gsfc.nasa.gov/SEplot/SEplot2051/SE2051Apr11P.GIF