Solar eclipse of January 4, 2011


A partial solar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, January 4, 2011, with a magnitude of 0.8576. 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 was the first of four partial solar eclipses in 2011, with the others occurring on June 1, 2011|June 1], July 1, 2011|July 1], and November 25, 2011|November 25].
The greatest eclipse occurred at 08:51 UTC in northern Sweden. At that time, the axis of the Moon's shadow passed a mere 510 km above Earth's surface.
The eclipse was visible near sunrise over most of Europe before moving over central Asia. It ended at sunset over east Asia. It was visible as a minor partial eclipse over north Africa and the Middle East.

Images

Animated path

Eclipse timing

Places experiencing partial eclipse

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.
EventTime
First Penumbral External Contact2011 January 4 at 06:41:18.7 UTC
Greatest Eclipse2011 January 4 at 08:51:42.4 UTC
Ecliptic Conjunction2011 January 4 at 09:03:43.1 UTC
Equatorial Conjunction2011 January 4 at 09:16:20.6 UTC
Last Penumbral External Contact2011 January 4 at 11:02:01.4 UTC

ParameterValue
Eclipse Magnitude0.85759
Eclipse Obscuration0.79839
Gamma1.06265
Sun Right Ascension18h59m14.9s
Sun Declination-22°44'21.1"
Sun Semi-Diameter16'15.9"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension18h58m23.8s
Moon Declination-21°46'01.2"
Moon Semi-Diameter15'18.1"
Moon Equatorial Horizontal Parallax0°56'09.6"
ΔT66.3 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months 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.
December 21
Descending node
January 4
Ascending node
Total lunar eclipse
Lunar Saros 125
Partial solar eclipse
Solar Saros 151

Related eclipses

Eclipses in 2011

Saros 151

Metonic series

Tritos series

Inex series