Reveal the defect

Yigal Fatal tells about the dragon that eats the sun and the moon, and about the expected solar eclipse on January 9

Yigal Fatal, editing - Avi Blizovsky, special for "Hidan"

In the diagram: solar eclipse

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On January 9, a total lunar eclipse will be seen in Israel. The eclipse will be visible on January 9 at very convenient times. It will start around a quarter to eight and end a little after midnight. In this lecture we will see how to calculate the eclipses and how to predict exactly when there will be an eclipse.
There are two theories about eclipses - one is scientific, and the other is correct - the dragon that eats the sun. As we know, the heavenly dragon is angry with humans because they are constantly sinning. That's why we have several deficiencies a year. In all cultures - a solar eclipse and a lunar eclipse is a punishment. And hence the name eclipse which indicates something defective, something bad that happens to the lights of the night and the day. This is also why during solar eclipses we see the same people going out and beating the drums to drive away the dragon. According to Genesis, the sun is the government of the day and the moon is the government of the night. These are two bodies designed to help a person, the government of the day and the night. Therefore when something happens to the sun it is a punishment. Without the moon you can still manage, without the sun you can't. Therefore the acuteness of a solar eclipse is more severe than a white eclipse.

Another reason why solar eclipses are scarier than white eclipses is that for an observer in a particular location solar eclipses are rarer than white eclipses. If they were not rare there would be no problem, one could continue to sin but since solar eclipses were really rare, actions must be taken so that the decree will pass from the world.
The Babylonians were the ones who discovered the legality of eclipse cycles, and it is strange to talk about myths of a people who knew the true causes of eclipses. However, as mentioned, not all the people controlled the taps of heaven. Those who knew this Torah were the aristocracy and aristocracy from China to South America and could rule the people ("If you don't pay me taxes, tomorrow I will raise the moon for you"). Imagine an astrologer predicting an eclipse, this is one of the only cases where an astrologer can be right and why take that away from him? There is a famous story of Columbus taking advantage of a total eclipse in America to extort gold from the natives. There is only one problem with this story Columbus thought he was in India and could not know what faults would occur in America.

And what does science say about that? We know that the moon, for example, is the best hand or clock there is. It never breaks down and completes a full cycle in about 29 and a half days. This is the synodical month on which the Hebrew month is built. If we look at the Earth-Moon system from the side, the Moon is at the beginning of the month between the Sun and the Earth, and from the Earth it cannot be seen because the sunlight falls on the side far from the Earth. We say about the moon that it is in the birth. In the quarter of the month we see both the dark part and the light part. In the middle of the month the moon is fully illuminated because it is behind the earth compared to the sun, then it begins to retreat until the new birth. The question is why don't we have an eclipse every month (actually two - a solar eclipse at the new moon and a lunar eclipse when the moon is full? Well, a month is 29 and a half days long. A new moon occurs when the three bodies - the earth, the moon and the sun are in one line. Therefore the moon has to make another small section of The cycle is to make up for the rotation of the Earth around the Moon. Therefore, the real cycle is two and a half days shorter: about 27 and a quarter days. This time is called the sidereal month, which means the Moon's orbit around the Earth in relation to a star that is at infinity and the rotation of the Earth around the Sun does not affect its position.
This is where the additional complications begin. The plane of the Moon's orbit around the Earth does not coincide with the Earth's orbit around the Sun. The difference between the routes is approximately 5 degrees. Therefore, eclipses will occur when the Moon is at one of the two points in its orbit on the line where its orbital plane crosses the milky plane. This line is called the line of knots. The point that is when the moon rises from south to north of the plane of incidence is called the rising knot and when it cuts the plane of Malacca from north to south it is the descending knot. Now, of course, two conditions need to be met for eclipses to occur: when the moon is on the line of conjunctions and it is also exactly at birth, there will be a solar eclipse. When the moon is in one of the conjunctions and the moon is full, a lunar eclipse will occur.
Apparently there is no problem - we have the period of time that the moon makes a revolution - we will take the common denominator between the sidereal month and the synodic month. But there are still some small complications that get in the way. For example, the fact that the moon is also affected by the sun's gravity. The point of intersection of the line of knots moves clockwise against the direction in which the Moon revolves around the Earth. Therefore we have a play relevant to eclipses that are not exactly the cycle of the moon's rotation around the earth. According to these calculations, the knot line makes a complete turn in a cycle of 18.6 years. This is the meeting of the lunar calendar with the solar calendar, as it is expressed in the Hebrew calendar. However, another small complication is related to the fact that the line of the apsides - the long string of the ellipse of the moon's orbit - also moves in the sky - counter-clockwise.
The period of time when the moon goes from one point of contact to the same point: 27 point 22 day - Dragon month. A multiple of the Dragon month in the synodic month gives the next eclipse in the same series, known as the Saros series: 18 years and 11 days. Each eclipse is better than the previous eclipse until the big eclipse in the middle, and then lesser eclipses. The Saros series can last 400 years. Of course, the frequency of eclipses is higher than once every 18 years, because the Moon, and the Earth's shadow are not points but large bodies, so the Moon does not have to be exactly on the plane of the conjunctions for there to be any eclipse.

A solar eclipse occurs when the Moon hides the Sun from certain points on Earth. As fate would have it, the distance of the moon is 400 times smaller than the distance to the sun, but its size is also smaller. But the ellipse of the moon's orbit is quite large and when it is relatively close to the earth it hides the sun and there is a large excess. And when the moon is far away its apparent size is smaller than the apparent size of the sun and then we see an annular eclipse. A total solar eclipse can reach a maximum of up to 11 minutes. when the moon is at its closest point and the sun is at its furthest point.

A solar eclipse is only visible in areas where the moon's shadow falls on the earth. The shadow moves quickly across the earth. And so he will see from the outlined area the shape of a rainbow on the surface of the earth.

There are cases when we see a partial eclipse - where the moon is below the line of conjunctions and the shadow almost misses the earth and then we see a partial eclipse in the areas close to one of the poles - as happened about a week ago, on December 25, 2000. As mentioned, the moon does not have to be on the line of conjunctions. A solar eclipse can also occur when the moon is plus or minus 15 thousand kilometers above and below the line of conjunctions. In a lunar eclipse, the story is different, because the moon enters the shadow of the earth, that is, everyone who is on the earth on the side where the moon is seen - sees the eclipse.
The moon passes during its movement through the partial shadow, then it stays in the full shadow area and goes out again into the partial shadow area. The full shadow area is 3-3.5 lunar radii. In a lunar eclipse it is only allowed to be a little more than 6,000 km plus or minus from the line of contact. This means that lunar eclipses are 2.5 times more rare than solar eclipses. In a year there are at least 2 eclipses that must be solar eclipses and a maximum of 7 eclipses that are mostly solar eclipses. From a probabilistic point of view there are more solar eclipses than lunar eclipses but since lunar eclipses are seen by all the inhabitants of half of the earth and solar eclipses in one place are seen on average only once every 400 years, in practice you can see much more white eclipses.

The upcoming eclipse, as expected on January 9 begins when the eastern side of the moon meets the penumbra at a quarter to eight. But we will begin to see a proper eclipse as the moon approaches the full shadow region. The border is not sharp because the Earth has an atmosphere, and the Earth allows the red rays to enter and not the blue ones. Therefore when the moon enters the full shadow, at 20:41 it will take on a reddish color.
At 21.49 the last point of light leaves the partial shadow, then we will see the western side in blue and the eastern side in yellowish red.
This eclipse is a northern eclipse, which means the moon is above the Melaka plane at the time of the eclipse. This means that the moon will reflect lights reaching it from the northern hemisphere of the earth. Hemisphere covered in January by clouds. If the earth is covered with clouds at a height of 10 km which are rain clouds, the shadow will be stronger and the moon will be darker.
The peak of the eclipse will be at 22:22. The size of the eclipse, that is, how many radii of the moon it is from the edge of the shadow to the center of the maximum 1.8 This means that the moon will be exactly in the center, meaning the most hidden from the sun and then the moon will be very dark. There was such an eclipse a few years ago and they hardly saw the moon.
At 22:50 the moon came out of the full shadow and at midnight we will already start to see it shining brighter and brighter. The eclipse will end three minutes before one o'clock. Another important data - the eastern part of the moon is below at sunrise. Towards midnight the east will be on the right and the western part of the moon on the left, and towards sunset the east will be up.

The next total solar eclipse will be in June 2001 in Africa - and will include areas such as Victoria Falls, Madagascar. It will be a 4 minute eclipse. The next eclipse that will be visible from Israel and in which only half of the sun will be hidden will occur in 2005 and its path will pass between Madrid, Libya and Aswan. By the way, it will be an annular defect. The next solar eclipse that can be seen from the surrounding and somewhat friendlier places will be seen in Antalya in May 2006, and then it will be visible from there. In Israel they will see 80 percent. And as we have seen, the sun shines 400 thousand times more than a full moon, and therefore even 2 percent of it is enough light for people in this area to barely feel the eclipse.

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