A total solar eclipse will occur at the Moon's ascending node of orbit on Friday, November 14, 2031, with a magnitude of 1.0106. It is a hybrid event, with portions of its central path near sunrise and sunset as an annular eclipse. 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 hybrid solar eclipse is a rare type of solar eclipse that changes its appearance from annular to total and back as the Moon's shadow moves across the Earth's surface. Totality occurs between the annularity paths across the surface of the Earth, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 3.1 days before perigee (on November 17, 2031, at 22:00 UTC), the Moon's apparent diameter will be larger.
Since most of the path of this eclipse is narrow and passes over the Pacific Ocean, no land areas will witness totality. However, annularity will be visible from parts of Panama near sunset. A partial eclipse will be visible for parts of northern Oceania, Hawaii, southern North America, Central America, the Caribbean, and northwestern South America.
<br />Animated path
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.
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) 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.