Solar eclipse of June 1, 2011

A partial solar eclipse occurred on June 1, 2011. 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. This eclipse is the second of four partial solar eclipses in 2011, with the others occurring on January 4, 2011, July 1, 2011, and November 25, 2011. The eclipse belonged to Saros 118 and was number 68 of 72 eclipses in the series.

Solar eclipse of June 1, 2011
Partial from Tromsø, Norway
Map
Type of eclipse
NaturePartial
Gamma1.213
Magnitude0.601
Maximum eclipse
Coordinates67.8°N 46.8°E / 67.8; 46.8
Times (UTC)
(P1) Partial begin19:25:17
Greatest eclipse21:17:18
(P4) Partial end23:06:57
References
Saros118 (68 of 72)
Catalog # (SE5000)9532

The eclipse was special since it occurred around midnight in Utsjoki, Finland, in Finnmark, Norway, and in Murmansk Oblast, Russia partially obscuring midnight sun.

Visibility


Animated path

Eclipses of 2011

Solar eclipses 2011–2014

This eclipse is a member of the 2011–2014 solar eclipse 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.[1][Note 1]

Saros 118

It is a part of Saros cycle 118, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650, hybrid eclipses on November 4, 1668 and November 15, 1686, and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. The longest duration of total was 6 minutes, 59 seconds on May 16, 1398.

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 descending node.

Notes
  1. The partial solar eclipses of January 4, 2011 and July 1, 2011 occurred in the previous semester series.

References
  1. 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.
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