Solar eclipse of March 30, 2052

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, March 30, 2052, with a magnitude of 1.0466. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.5 days before perigee (on April 1, 2052, at 6:30 UTC), the Moon's apparent diameter will be larger.

The path of totality will be visible from parts of central Mexico, the extreme southern tip of Texas, southeastern Louisiana, southeastern Alabama, Florida, Georgia, and South Carolina. A partial solar eclipse will also be visible for parts of Hawaii, North America, Central America, the Caribbean, and northern South America.

This will be the 2nd total eclipse visible from the Florida panhandle and southwest Georgia in 6.6 years. It will also be the last total solar eclipse visible in the United States until May 11, 2078.

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.

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.

The partial solar eclipse on August 3, 2054 occurs in the next lunar year eclipse set.

This eclipse is a part of Saros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.