Solar eclipse of June 11, 2067


An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067, with a magnitude of 0.967. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus. An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 4.3 days before apogee, the Moon's apparent diameter will be smaller.
This solar eclipse is notable as it is the closest eclipse in Saros 138 to the subsolar point with an eclipse gamma of -0.0387.
The path of annularity will be visible from parts of Kiribati, Ecuador, northern Peru, extreme southern Colombia, and extreme western Brazil. A partial solar eclipse will also be visible for parts of Oceania, Hawaii, southern North America, Central America, the Caribbean, and western South America.

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 contact2067 June 11 at 17:41:42.1 UTC
First umbral external contact2067 June 11 at 18:45:02.0 UTC
First central line2067 June 11 at 18:46:37.3 UTC
First umbral internal contact2067 June 11 at 18:48:12.5 UTC
First penumbral internal contact2067 June 11 at 19:51:38.7 UTC
Greatest eclipse2067 June 11 at 20:42:26.4 UTC
Equatorial conjunction2067 June 11 at 20:42:35.2 UTC
Ecliptic conjunction2067 June 11 at 20:42:53.4 UTC
Greatest duration2067 June 11 at 20:43:57.1 UTC
Last penumbral internal contact2067 June 11 at 21:33:13.1 UTC
Last umbral internal contact2067 June 11 at 22:36:38.6 UTC
Last central line2067 June 11 at 22:38:16.2 UTC
Last umbral external contact2067 June 11 at 22:39:53.8 UTC
Last penumbral external contact2067 June 11 at 23:43:15.9 UTC

ParameterValue
Eclipse magnitude0.96702
Eclipse obscuration0.93513
Gamma−0.03865
Sun right ascension05h20m58.3s
Sun declination+23°07'36.6"
Sun semi-diameter15'45.1"
Sun equatorial horizontal parallax08.7"
Moon right ascension05h20m58.0s
Moon declination+23°05'29.3"
Moon semi-diameter15'00.0"
Moon equatorial horizontal parallax0°55'03.2"
ΔT95.6 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. The first and last eclipse in this sequence is separated by one synodic month.
May 28
Ascending node
June 11
Descending node
June 27
Ascending node
Penumbral lunar eclipse
Lunar Saros 112		Annular solar eclipse
Solar Saros 138		Penumbral lunar eclipse
Lunar Saros 150

Related eclipses

Eclipses in 2067

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 138

Inex

Triad