Simply because the Earth's path around the sun is not a circle. Earth's orbit is an ellipse - meaning its distance from the sun varies according to the time of year.
The minimum distance between the Earth and the Sun occurs during perihelion, which is when the Earth is closest to the Sun in its elliptical orbit. This usually happens around January 3rd of each year.
One "Astronomical Unit" is (more or less) the average distance between the Sun and Earth.
Not at all. It depends up on Mass and the distance . Here Mass is constant . but distance is not .The distance between Earth and Sun is not always the same in an year.because of the elliptical orbit of the Earth.
An increase in the distance between Earth and the Sun would cause the gravitational force between them to decrease. Conversely, a decrease in the mass of either the Earth or the Sun would also result in a decrease in the gravitational force between them.
It is the average distance between the centres of the two objects.
It is the distance between the earth and moon.
distance
152,098,232 kilometers.
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.
The minimum distance between the Earth and the Sun occurs during perihelion, which is when the Earth is closest to the Sun in its elliptical orbit. This usually happens around January 3rd of each year.
... the first week of July.
Aphelion, which generally occurs in July.
The Earth reaches its greatest distance from the Sun during the summer season in the Northern Hemisphere. Though it may seem counterintuitive, the distance between the Earth and the Sun varies due to the elliptical shape of Earth's orbit, with the Earth being farthest from the Sun during the summer months.
about 8 light minutes
Your 152 million kilometers is 152,000 megameters.
scale
D. Alignment of the Universe does not contribute to the changing of seasons. The changing of seasons is primarily influenced by the tilt of the Earth's axis as it orbits the Sun (B), along with the varying distance between the Earth and the Sun (C) throughout the year. The distance between the Earth and the Moon (A) mainly affects tides on Earth.