the sun rises in the west and sets in the east.
How high the sun is in the sky. The angle between the horizon and the sun. When the sun is directly overhead (eg, at the equator) the solar altitude is 90°. In Canberra in winter, the solar altitude is 30°.
Both lunar and solar eclipses are the result of positioning 3 astronomical bodies (earth, sun and moon) in a straight line relative to the observer. A solar eclipse is observed when the sun, moon, and earth are positioned in a straight line with an observer on the earth. A lunar eclipse is observed when the sun, earth, and moon are in a straight line with an observer on the earth. A lunar eclipse, as observed by an observer on the earth would appear as a solar eclipse as observed by an observer on the moon.
47 degrees.
The altitude of the sun is the angle between the sun and the observer's horizontal plane. It changes throughout the day as the sun rises and sets. At solar noon, when the sun is at its highest point in the sky, the altitude is its maximum.
The sun's altitude refers to its angle above the horizon, measured in degrees. This angle varies throughout the day and changes with the seasons due to the tilt of the Earth's axis and its orbit around the sun. At solar noon, the sun reaches its highest point in the sky for that day, which is when its altitude is at its maximum. The altitude can be calculated using the observer's latitude, the date, and the time of day.
There are different kinds of solar eclipses. A solar eclipse occurs when an astrological body blocks view of the sun. If the observer is standing on the earth, and the moon moves in between the observer and the sun, that is an eclipse. If the observer is standing on earth's moon, and the earth moves between the observer and the sun, that is also an eclipse.
During the Moon's revolution, an observer in space would see the moon, but would not be able to see it spin around. From far to the north, about the solar system, the moon would appear to make a squiggly
The observer of a solar eclipse would typically be located on Earth, witnessing the event as the moon passes between the sun and Earth, causing either a partial or total eclipse. The specific location on Earth where the observer would be situated would depend on where the eclipse is visible from.
solar flares appear as a dark spot
the tilt goes towards the sun, the seasons chang from winter to summer
The Moon comes between the Sun and the observer in this case.
solar altitude angle= (90 degree - zenith angle )