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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 part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close ...
A total lunar eclipse occurred at the Moon’s descending node of orbit on Friday, July 27, 2018, [1] with an umbral magnitude of 1.6100. It was a central lunar eclipse, in which part of the Moon passed through the center of the Earth's shadow.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, July 6, 1982, [1] with an umbral magnitude of 1.7180. It was a central lunar eclipse, in which part of the Moon passed through the center of the Earth's shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened ...
A total lunar eclipse occurred at the Moon’s descending node of orbit on Friday, September 27, 1996, [1] with an umbral magnitude of 1.2395. 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 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 1.5 days after apogee (on June 23, 1964, at 12:30 UTC), the Moon's apparent diameter was smaller.