Which correctly describes the gravity between objects in the solar system?
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Which correctly describes
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Well, you see, it's like the universe's own way of playing "tug of war". Gravity is the invisible force that keeps objects in the solar system from floating away into space. Think of it as a cosmic hug that pulls everything together. It's like the sun saying, "Hey, planets, let's stick together!" So, to put it simply, the gravity between objects in the solar system is what keeps them from going on their own intergalactic joyrides. It's the universe's way of saying, "No way, buddy, you're staying put!"
The gravity between objects in the solar system can be described by Newton's law of universal gravitation. This law states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
To calculate the gravitational force between two objects in the solar system, you can use the following equation:
F = G * ((m1 * m2) / r^2)
Where:
- F is the gravitational force between the objects,
- G is the gravitational constant (approximately 6.67430 x 10^-11 N(m/kg)^2),
- m1 and m2 are the masses of the objects, and
- r is the distance between the centers of the objects.
This equation applies to any objects in the solar system, such as planets, moons, asteroids, and even the Sun. The force of gravity acts between all pairs of objects, but its strength depends on their masses and the distance between them.
It's important to note that the effects of gravity extend throughout the entire solar system, influencing the orbits, movements, and interactions of all celestial bodies within it.
as with all 2-body problems,
F = GMm/r^2