Want this question answered?
the eclipse starts at 10:00 p.m. eastern ___________________ Earth's experience of the solar eclipse is a happy coincidence of history. It just happens that we have a moon of the right size and favorable orbit. It will not always be so. In future ages, the moon will no longer be able to give us 'total' eclipses, because it is very slowly moving farther away from earth. At some point it will be too far to completely cover the face of the sun.
The moon is ALWAYS much closer to the Earth than it is to the sun. For a solar eclipse, the three bodies have to be lined up, with the moon in the 'middle'. The SIZE of the eclipse (I.E. area covered in shadow) changes if the moon is slightly closer or slightly farther away from Earth. If the Moon is closer to the earth, then the shadowed area is larger. If it is farther from the earth, then the shadowed area is smaller.
A solar eclipse happens when the Moon covers the Sun. The Moon is only about 1/4 the size of the Earth, and that is the reason the eclipse can't be seen (not even as a partial eclipse) from all parts of the Earth at once.A solar eclipse happens when the Moon covers the Sun. The Moon is only about 1/4 the size of the Earth, and that is the reason the eclipse can't be seen (not even as a partial eclipse) from all parts of the Earth at once.A solar eclipse happens when the Moon covers the Sun. The Moon is only about 1/4 the size of the Earth, and that is the reason the eclipse can't be seen (not even as a partial eclipse) from all parts of the Earth at once.A solar eclipse happens when the Moon covers the Sun. The Moon is only about 1/4 the size of the Earth, and that is the reason the eclipse can't be seen (not even as a partial eclipse) from all parts of the Earth at once.
No, you can't ever see a crescent Mars from Earth. Because Mars is farther from the sun than Earth is, there is no point at which less than half of Mars' illuminated size is facing Earth. In other words Mars will always appear as "full" or "gibbous."
Actually, the earth expands. Heat causes many things to expand in size, and the earth just happens to be one of those things. I hope I helped :)
size
The centripetal force decreases. F= mv^2/r = mGM/r^2
- By using seismic waves .
An onion because the earth has many different layers just like an onion
the moon is smaller but its closer. the sun is huge but its way farther away so that why they look the same size.
winter happens when the earth shifts on its axis. the shift moves certain of earth's land mass farther away from the sun. the added distance from the sun means less heat from the sun. less heat means merry x-mas, as in, BOY! do you see the size of those flakes?
the eclipse starts at 10:00 p.m. eastern ___________________ Earth's experience of the solar eclipse is a happy coincidence of history. It just happens that we have a moon of the right size and favorable orbit. It will not always be so. In future ages, the moon will no longer be able to give us 'total' eclipses, because it is very slowly moving farther away from earth. At some point it will be too far to completely cover the face of the sun.
The moon is ALWAYS much closer to the Earth than it is to the sun. For a solar eclipse, the three bodies have to be lined up, with the moon in the 'middle'. The SIZE of the eclipse (I.E. area covered in shadow) changes if the moon is slightly closer or slightly farther away from Earth. If the Moon is closer to the earth, then the shadowed area is larger. If it is farther from the earth, then the shadowed area is smaller.
if a planet was close to earth it would cause earthquakes and more. if it collided if earth depending on the size if it is big it will collide with earth.
i believe the answer is it will vary in a cyclic manner because the earth moves farther away from the sun in summer in the northern hemisphere and then closer in the winter
The sun is approximately 400 times the size of the moon, however, it is also approximately 400 times farther away. This relationship cancels out and makes the sun and the moon appear observationally to be the same size on earth.
objects look bigger the closer to you they are. the moon is small, but close to earth. the sun is much larger, but much farther away.