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The longest annular solar eclipse of the 21st century took place on January 15, 2010, with a duration of 11 minutes and 7.8 seconds. The maximum possible duration is 12 minutes and 29 seconds. The eclipse of May 20, 2050, will be the second hybrid eclipse in the span of less than one year, the first one being on November 25, 2049.
This is a list of solar eclipses visible from the United States between 1901 and 2100. All eclipses whose path of totality or annularity passes through the land territory of the current fifty U.S. states and the District of Columbia are included. All types of solar eclipses, whether recent, upcoming, or in the past, are also included.
A partial solar eclipse will occur at the Moon’s ascending node of orbit on Saturday, March 29, 2025, [1] with a magnitude of 0.9376. 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.
The first partial solar eclipse of 2025, on March 29, will be visible from a slice of the northeastern United States and Canada as well as Greenland, Iceland, and parts of Europe and northwest Africa.
March 29, 2025 — Partial solar eclipse. ... According to NASA, the date listed for each eclipse coincides with the local date of where the eclipse is set to occur. Lunar Eclipses 2024.
Eclipse Season Dates for 2025: March 14, 2025: Total Lunar Eclipse in Virgo. March 29, 2025: Partial Solar Eclipse in Aries. September 7, 2025: Total Lunar Eclipse in Pisces.
List of solar eclipses in the Middle Ages (5th to 15th century) Modern history. List of solar eclipses in the 16th century; List of solar eclipses in the 17th century; List of solar eclipses in the 18th century; List of solar eclipses in the 19th century; List of solar eclipses in the 20th century; List of solar eclipses in the 21st century; Future
Solar eclipses are grouped by their saros number, each series lasts between 1200 and 1600 years and contains from 69 to 87 solar eclipses (most often 70 to 73). Solar eclipses in odd series exist at the ascending node of the Moon's orbit, and even series occur at the descending nodes.