The eclipse will take place during the night of July 16. Unlike solar eclipses, lunar can be seen from anywhere in the world that the satellite has over its horizon at the time of the phenomenon. In this case, that happens in Europe, Africa, Asia, Australia and South America. In Spain, it will start at 10:01 PM (peninsular time). At 23:30, the phase of maximum darkness will occur and will end at 00:59. It can be seen directly or from telescopes. If it is observed through one of these instruments, it will be possible to appreciate the advance of the shadow covering the Moon and details of its surface such as craters and mountains. The partial eclipse can be seen directly or from telescopes The National Museum of Science and Technology (MUNCYT) of Alcobendas

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(Madrid), in collaboration with the Sweden Email List Astronomical Center of Ávila, has organized an astronomical observation with 12 motorized telescopes, starting at 10 pm. The event will be complemented by the observation of Jupiter and Saturn, which will be visible throughout the night. To attend this activity, it is necessary to book in advance through the email [email protected] . How does a lunar eclipse occur? During a lunar eclipse, the Earth stands between the Sun and the Moon and casts a shadow that covers the satellite. For it to occur, it is necessary that the three celestial bodies are aligned and that the satellite is in the full moon phase. There are three types of lunar eclipses: penumbral, partial, and total. In the penumbra , the Moon is covered by

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the part of the outermost and weakest terrestrial shadow, the penumbra. Therefore, the concealment is very slight and barely perceptible. Partial eclipses occur when the satellite is hidden by the umbra, the inner part of the shadow cast by the Earth. It is possible to distinguish when the shadow makes contact with the Moon, although the phenomenon does not present a good definition due to the presence of the atmosphere, unless it is observed by a telescope. In totals , the umbra completely hides the Moon. Since the diameter of our planet is four times larger than the lunar diameter, its shadow is also wider and the totality phase of the eclipse can last more than an hour and a half. In addition, the satellite turns reddish in color because the

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