The orbit of a planet is not a circle with the sun at the center. It's an ellipse with
the sun at one focus.
An ellipse is an 'egg shape', or 'oval', or 'squashed circle'. It has two foci (focuses)
and neither one is in the center.
So you can easily see that as the planet moves along the ellipse, its distance from the sun
changes, and there is a minimum distance (perihelion) and a maximum distance (aphelion).
Those don't change unless the shape of the ellipse changes, and the only way
that happens is through the gravitational influence of the other planets, which
is relatively tiny over the course of many millennia.
Two factors that affect a planets revolution are distance from the sun and size.
Mass and distance. The force decreases with the square of the distance, so mass has a lesser effect on the equation.
The length of the day would change if either the rotational speed of the the planet or the orbital distance from the sun changed. However, if you mean what factors affect the length of daylight, then that is different.
Gravity is the attraction between two or more bodies. It is propotional to their mass and inversely proportional to their distance.
When Earth orbits the sun, its eccentricity of the orbit is only 0.017. That's very close to 0, a perfect circle. So when it's at its closest to the sun (perihelion) , it doesn't make a difference.
Mass, distance.
the three factors that affect the weather are altitude the distance from the ocean and topagraphy! ***hopefully this helped you!
Two factors that affect a planets revolution are distance from the sun and size.
mass and distance ;)
mass and distance
it is mass and distance
mass and distance
i dont know maybe you guys do.
distance from the sea, ocean current
There are two factors that affect the gravitational attraction between two objects. The mass of each object and the distance between their centers of mass are the factors that affect the attraction.
If you're talking about the whole Earth, there are not many that affect the amount of energy. One factor is in the distance of the Earth from the Sun. The Earth gets slightly more energy from the Sun at the Perihelion (the closest point to the Sun) than the Aphelion (the furthest point away from the Sun). Another factor is how active the Sun is. The Earth is likely to receive less energy from the Sun at a solar minimum than a solar maximum in the 11 year cycle of the Sun (because the Sun is outputting less energy).
Distance and intervenng or close celestial bodies