Each planetary body in the solar system has a gravitational effect on every other planet of the solar system as well as being affected by, and having an effect on, the Sun. Gravitational effects include tides, planet shapes, friction within a body, orbit, tilt, meteorite and asteroid impacts and avoidance of impacts, and atmospheres.
gravity not to sure tho
To calculate weight on other planets, you can use the formula: Weight Mass x Gravity. The mass of an object remains the same, but the gravity on different planets varies. You can find the gravity of a planet by looking it up online or using a formula. Then, multiply the mass of the object by the gravity of the planet to find the weight on that planet.
Yes. The sun is attracted by the gravity of the planets just as the planets are attracted by the sun. Since the sun is more massive it does not move as much, bu the gravity of the orbiting planets does cause it to "wobble."
The effect of gravity does effect the planets. Gravity keeps the planets to the sun. Gravity works between any 2 objects. It's the attraction between planets and sun that keeps planets going around the sun otherwise they would keep going in a straight line.
Earth has gravity rather than other planets.
The motions of the planets are primarily controlled by gravity, which is the force of attraction between all masses in the universe. In our solar system, the Sun's gravitational pull governs the orbits and movements of the planets. The precise motions of the planets are also influenced by their initial velocities and the conservation of angular momentum.
First of all, gravity causes the orbital movement in the first place - due to the attraction by the Sun, the planets go around the Sun in ellipses. Because planets also attract each other, the orbits may gradually change over time.
The scientific explanation lies in Kepler's laws of planetary motions, which were discovered by Newton to be linked with the law of gravity. All the planets have elliptical orbits, and many of those are close being circular.
The balance between gravity (attraction to the Sun) and orbital energy (1/2 velocity2 times mass) gives the planets their order.
true
The primary force that determines the motions of planets and other objects in the solar system is gravity. This force, described by Newton's law of universal gravitation, causes celestial bodies to attract one another, leading to the orbits of planets around the Sun and the moons around their respective planets. Additionally, Einstein's theory of general relativity refines our understanding of gravity, illustrating how massive objects warp spacetime, further influencing these motions.
Planets with elliptical orbits are affected by the difference in the strength of the Sun's gravity as they move closer to, or farther away from, the Sun. The only other major effect on planets are the gravity of other planets, notably Jupiter and Neptune. Except for Mars, Ceres, Pluto, and trans-Neptunian planets, the effect is extremely small -- it has resulted in stable orbital resonances between several small outer planets and the planet Neptune.
There are two reasons. First, since they are farther from the sun they have longer orbital path. Second at a greater distance from the sun the sun's gravity is weaker, giving the outer planets a slower orbital speed.
Without gravity, each of the planets would continue straight ahead into space, and become dispersed. Gravity holds them in their orbital paths around the Sun. Of course, without gravity, the Sun would explode, and the planets would also disintegrate and their mass would scatter because of the centrifugal force of their spin and angular momentum.
Inertia and gravity are fundamental forces that govern the orbital motion of planets. Inertia, as described by Newton's first law of motion, causes planets to continue moving in a straight line unless acted upon by an external force. Meanwhile, gravity, the attractive force between masses, pulls planets toward the sun, creating a curved path. The balance between these two forces results in stable orbits, where planets continually fall toward the sun but also move forward, preventing them from crashing into it.
The orbital speed of the planets prevent this. The planet's ARE all failing towards the Sun but their horizontal speed means they always miss.
The orbital speed of the planets prevent this. The planet's ARE all failing towards the Sun but their horizontal speed means they always miss.