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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.
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.
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 ...
Eclipse Magnitude 1.03673 Eclipse Obscuration 1.07481 Gamma −0.95261 Sun Right Ascension 16h43m32.4s Sun Declination -22°16'29.4" Sun Semi-Diameter 16'13.6" Sun Equatorial Horizontal Parallax 08.9" Moon Right Ascension 16h42m35.0s Moon Declination -23°13'22.3" Moon Semi-Diameter 16'44.7" Moon Equatorial Horizontal Parallax 1°01'27.3" ΔT
Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.1 days after perigee (on March 28, 2006, at 8:10 UTC), the Moon's apparent diameter was larger. [4] This was the second solar eclipse visible in Africa within just 6 months.
A partial solar eclipse occurred at the Moon's descending node of orbit between Saturday, January 5 and Sunday, January 6, 2019, [1] [2] with a magnitude of 0.7145. 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.
VV Cephei, also known as HD 208816, is an eclipsing binary star system located in the constellation Cepheus.It is both a B[e] star and shell star.As a 5th magnitude star, it is visible to the naked eye under good observing conditions.
An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [ 3 ] The partial solar eclipses on March 16, 1942 and September 10, 1942 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 30, 1946 and November 23, 1946 ...