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.
The sun's gravity keeps the planets in orbit around it, preventing them from moving off into space. The strength of the sun's gravity decreases with distance, so planets closer to the sun experience a greater gravitational pull than those farther away. This gravitational force is what keeps the planets in their elliptical paths around the sun.
Gravity is the force that pulls objects toward each other.
Gravity on the outer planets, such as Jupiter and Saturn, is stronger than on Earth due to their larger mass. This strong gravity affects the size and composition of these planets, influencing their gaseous atmospheres and formation of rings and moons. The gravitational pull also helps to shape their orbits and interactions with other celestial bodies in the solar system.
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.
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The balance between gravity (attraction to the Sun) and orbital energy (1/2 velocity2 times mass) gives the planets their order.
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.
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.
If the force of gravity suddenly stopped acting on the planets, they would continue moving in a straight line at a constant speed, following Newton's first law of motion. Without the force of gravity to pull them towards the Sun, the planets would travel in a tangential direction away from their current orbital paths.
Planets that are farther from the sun have longer orbital periods due to the influence of gravity. The gravitational force between the sun and a planet decreases with distance, so planets farther out experience weaker gravitational pulls, resulting in slower orbital speeds. This explains why outer planets like Neptune have longer orbital periods compared to inner planets like Mercury.