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elliptical orbit with earth at one focus.
The Earth's distance from the moon or Mars is always changing. The closest the moon can get to Earth is 225,622 miles. The farthest it can get is 252,088 miles. The closest possible distance from Earth to Mars is 33.9 million miles. Therefore the Earth is always much closer to the moon than Mars, no matter where they are in orbit.
Depending on where Mercury is relative to the Earth as the two planets orbit the sun, the distance from Mercury to Earth varies from 77.3x106km and 221.9x106km.
Earth is part of our solar system.
The light year is not a practical unit for measuring interplanetary distances. It is usually reserved for dealing with the distances between the stars, which is far greater. A better unit for grasping the Earth-Jupiter distance would be the A.U., or astronomical unit, equal to the Earth-Sun distance, 93 million miles, or 150 million kilometers. Also, the distance between Earth and Jupiter is constantly changing, since both bodies follow separate orbits around the sun.
The moon is under the influence of both the Earth's and the Sun's gravitational pull.
The Earth's changing distance from the Sun during the year causes the seasons.
distance between the earth and the sun.
distance between the earth and sun
It is not changing the local election results in Huddersfield or changing the distance between Earth and Neptune
elliptical orbit with earth at one focus.
elliptical orbit with earth at one focus.
It is changing because the orbit of Earth is not a perfect circle. It is sort of oval and is called an elipse.
Unfortunately there is no simple answer to that. The distance is constantly changing as the planets move in their orbits.
when the moon is beetween the earth and sun
The distance of the Earth from the sun does not contribute to the changing seasons. Although this distance does change (since the Earth's orbit is elliptical, not perfectly circular) the amount of the change is not great enough to affect the seasons. It is the angle of incidence of solar radiation, which in turn is affected by the axial tilt of the Earth and its revolution around the sun, which creates the changing seasons.
The Earth's orbit around the Sun is elliptical, not a perfect circle. This means that the distance between the Sun and Earth is constantly altering during the orbit of the Earth.