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Meteoprog also maintains a weather archive, which encompasses historical weather data from around the globe spanning the past 75 years. The data collected and stored by Meteoprog aids in understanding weather pattern shifts over time, enabling predictions about future weather changes across the coming days, months, or even years.
This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [5] The penumbral lunar eclipse on July 18, 2027 occurs in the next lunar year eclipse set.
A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.2 days after apogee (on July 5, 1982, at 2:30 UTC), the Moon's apparent diameter was smaller. [2] It was the longest total lunar eclipse since the 1859 eclipse.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Monday, April 24, 1967, [1] with an umbral magnitude of 1.3356. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Wednesday, May 26, 2021, [1] with an umbral magnitude of 1.0112. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow.
Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller.
A total solar eclipse occurred at the Moon's descending node of orbit between Friday, June 8 and Saturday, June 9, 1956, [1] with a magnitude of 1.0581. 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 eclipse will pass over the southern Galápagos Islands (with a total eclipse of 4 minutes occurring over the southern tip of Española Island), the northern tip of Ecuador (with a total eclipse of 3 minutes and 26 seconds on Isla Santa Rosa), central Colombia (4 minutes and 50 seconds over Bogota), central Venezuela, and northern Guyana (7 ...