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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.
This total solar eclipse had a maximum duration of 6 minutes and 38.86 seconds. The longest possible duration of a total solar eclipse is 7 minutes and 32 seconds. 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 ...
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
The next total solar eclipse to pass over any part of the contiguous United States will be in 2044. The last time Rochester was in the path of totality was 1925; the next time will be in 2144.
Here’s a list of some of the major events for the total solar eclipse on April 8 in New York, Texas, Indiana, Kentucky, Ohio, Arkansas, Illinois, Maine, Pennsylvania and Washington, D.C. Want to ...
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 (ring). An annular ...
Below is a list of timings for some U.S. cities along the path of totality, according to NASA. Dallas: Partial eclipse begins at 12:23 p.m. CT and totality at 1:40 p.m. CT.
A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, September 4, 2100, [1] with a magnitude of 1.0402. 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.