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March 29, 2025 solar eclipse times Event Time (UTC) First penumbral external contact 2025 March 29 at 08:51:52.5 UTC Greatest eclipse 2025 March 29 at 10:48:36.1 UTC Ecliptic conjunction 2025 March 29 at 10:58:59.4 UTC Equatorial conjunction 2025 March 29 at 11:47:27.0 UTC Last penumbral external contact 2025 March 29 at 12:44:54.0 UTC
A partial solar eclipse will occur at the Moon’s descending node of orbit on Sunday, September 21, 2025, [1] with a magnitude of 0.855. A solar eclipse occurs when the Moon passes between the Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth.
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. [a] The table contains the date and time of the greatest eclipse (in dynamical time , which in this case is the time when the axis of the Moon's shadow cone passes closest to the centre of Earth; this is in ...
For the first time since 2022, a total lunar eclipse will cause the moon to turn red as it passes through the Earth's shadow. ... the new moon as it is the time when the sky is the darkest. In ...
"The good news is that the weather will be dry and cooperative across much of the United States as the last minutes of 2024 wind down and the first moments of 2025 begin," said AccuWeather ...
Eclipse path of totality cuts across 13 U.S. states Mexico's Pacific coast will be the first location in continental North America to experience totality, which will occur about 11:07 a.m. PDT ...
The path of the total solar eclipse that will cross Louisiana on May 11, 2078. From 1900 to 2100, the state of Louisiana will have recorded a total of 84 solar eclipses, three of which are annular eclipses and four of which are total eclipses. The three annular solar eclipses occurred on November 22, 1919; April 7, 1940; and May 30, 1984.
A total eclipse occurs on average every 18 months [11] when the dark silhouette of the Moon completely obscures the bright light of the Sun, allowing the much fainter solar corona to be visible. During an eclipse, totality occurs only along a narrow track on the surface of Earth. [12] This narrow track is called the path of totality. [13]