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24.07.2018 10:00
After a three-year break, we will be able to see the complete eclipse of the moon on Friday, July 27th.
Photo Illustration
Author:
SHUTTERSTOCK
The complete phase lasts almost 104 minutes. It took three years
"Only" 73 minutes
An extraordinary eclipse length is given by the moon that runs through
near the middle of the shadow (so-called umbra) of the Earth. In good weather, it will be
The moon will appear above the horizon at 8:24 pm just at the start time
partial excitation. As indicated by the height of the moon (see table), together
the eclipse will go relatively close to the horizon. This is good
an opportunity for interesting photographers and hunters. Zatmenie
will end on Saturday, July 28 about 20 minutes after midnight. Another complete
the lunar eclipse will be the morning of Monday, January 21, 2019, and its full
the phase will last 102 minutes
The shadow of the Earth falls on the surface of the Moon
The eclipse of the Moon is an astronomical phenomenon in which the shadow of the earth falls
the surface of the Moon. It happens in time around fulfillment, when the moon is during its
The orbital movement approaches the Sun-Extended Earth connector
will enter the shadow of the Earth. But it's not a shadow of the surface of the earth,
geometric shadow but shadow influenced by the atmosphere of the Earth
If the Earth was without atmosphere, the shadow of the Earth would be restrained,
homogeneous and would not be seen in it. There are no eclipses
however, the darkening of the monthly disc is over; its center is reddish and circled
Grey. The properties of each shadow depend on these parts of the earth
the atmospheres through which the respective sun rays have passed. It's a change
the index of refraction with the height above the latte of the Earth to its geometric shadow, by that
moreover, the closer they are to the surface of the earth
The whole eclipse will take place
relatively close to the horizon. This is a good opportunity for photographers and hunters
interesting images
A ring of light that runs through the atmosphere grows so much that
can light up the entire lunar disc slightly in the shadow of the earth. In the interior
a part of the shadow is another attenuation due to the diffusion of the light on the molecules
air (we thank him for the blue color of the day sky) and also disperse on
dust and cloud cover. This is how the violet and blue rays are the weakest
with regard to the red and the orange, who then in the sunlight
prevail. The course of the density (and therefore the refractive index) of the upper atmospheres has
air pollution is very variable, and therefore the brightness and color of the moon to
From observations of eclipses in the past, the relationship between magnitude
the shadow of the Earth, the brightness and color of the moon on one side and the volcanic
the meteoric activity of the other, which conditions the amount of dust in
about 100 km, and thus the bending and scattering of light. Watch the monthly
so that the degree of total dedusting and contamination can be determined
the atmosphere of the Earth in places where the sun comes out at the time of the eclipse or
In the morning and in the evening, it rains in the center of the disc of the month.
it turns into a characteristic reddish shade. Let's move on
a moment of the Earth on the side of the moon in the passage
the shadow of the Earth. The view that would appear to the astronaut was represented
The French artist and astronomer Lucien Rudaux, living between 1874 and 1940
1947. At that time, the astronaut would see the eclipse of the Sun with the edge of darkness
the disk of the Earth would be lined with a reddish ring of morning and evening harnesses, which
would surround the white pearl crown of the sun. The astronaut would be around the moon
the landscape with its reddish color resembled the surface of Mars
An observation experiment will provide a telescope
A less striking phenomenon is the flattening of the Earth's shadow. Really observed
the flattening of the earth's shadow is much larger than the Earth itself. It is possible
explain by flattening the atmosphere that is caused by the rotation of the Earth and the Earth
higher density (and therefore lower thickness) of the cold polar atmosphere.
From the precise astronomical observation of the moon moon,
flattening of the atmosphere is up to four times greater than the flattening of the earth
The burial of the moon is an astronomical phenomenon, but it denies the # 39; s atmosphere
Earth and is at the forefront of astronomy, geophysics and meteorology. In terms of
earthly shadow observer of the Earth advance the moon of his is
edge to the west. This proves that the Moon is actually
it moves from west to east. However, we feel its apparent movement of
horizon is in the west. This impulse gives us the rotation of the earth.
The circular shape of the Earth's shadow on the moon led to old Greeks
astronomers to conclude that the Earth is a ball. Attraction experience
will provide a view through the telescope that is suitable for mounting on a tripod or
other improvised position
Situation in the sky at the time of maximum excitation at 22:22
Mesiac will be at that time in the Capricorn Constellation. below
The moon towards the horizon will be striking with its reddish color Mars.
To the right of them directly above the southern point will be Saturn, which will be at that time
in the constellation Strelec. In the direction of this constellation lies the center of our galaxy,
whose disk we see in the sky like the Milky Way – the little
a visible light belt of places without pollution of the night
sky. Even further west to the west, it will be possible to see the star
Antares strikes with its flashing and blushing light. It's starry
field, the brightest constellation of Scorpio stars.
The next star map shows the situation above the southwest horizon, where
Further to the right of Antares, Jupiter will shine
at that time in the constellation Libra
Complete eclipse of the moon on July 27 | min. LSEČ | Height of the Moon above the horizon | ||
---|---|---|---|---|
Start of a partial eclipse | 20.24 | 0º | ||
Start of the total exchange | 21.30 | ] End of the complete eclipse | 23.13 | 18º |
End of the partial eclipse | 00.19, July 28 | 21º |
More d & # 3939; information on eclipses
SAV, vv
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