The path that planets take around the sun is called it's orbit. The gravitation pull of the sun keeps each planet in it's orbit. Each planets orbit varies in the time it takes to make one trip around the sun.
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∙ 9y agoA planet's speed changes as it moves along its elliptical orbit around the sun. It moves fastest at the point closest to the sun (perihelion) and slowest at the point farthest from the sun (aphelion) due to Kepler's second law of planetary motion. Thus, the speed of a planet in its elliptical orbit is not constant but varies depending on its position in the orbit.
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∙ 10y agoA planet is slowest when farthest from the Sun.
A planet moves fastest when closest to the Sun
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∙ 14y agoWhen a planet makes one complete rotation around the sun is called a revolution, and an orbit. When it spins on it's axis then it is called a rotation.
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∙ 12y agoIt depends on their mass and their distance from the sun
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∙ 11y agoOrbital velocity
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∙ 14y agoAn elliptical orbit.
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∙ 7y agoIt is called its orbit.
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∙ 15y agoAn "orbit"
Anonymous
mars
The speed of a satellite in an elliptical orbit around Earth varies depending on its distance from the planet. The satellite moves fastest at the point in its orbit closest to the Earth (perigee) and slowest at the point farthest from the Earth (apogee). The average speed of the satellite can be calculated using the vis-viva equation.
A planet is slowest when it is farthest from the Sun in its elliptical orbit, at its aphelion point.
Each planet in our solar system revolves around the sun in an elliptical orbit. The time it takes for a planet to complete one revolution around the sun is known as its orbital period. This period varies for each planet based on its distance from the sun.
A planet's movement around the sun is due to the gravitational pull of the sun, which keeps the planet in orbit. The planet moves along its path (orbit) at a constant speed, following an elliptical trajectory due to the balance of gravitational force and the planet's inertia. This movement repeats in a predictable pattern, forming the planet's year.
The gravitational pull exerted by the Sun, which acts as the central force keeping planets in orbit, causes them to move along elliptical paths. The conservation of angular momentum ensures that planets travel in elliptical orbits, with their speed varying at different points along the orbit to maintain this balance.
A satellite in a closed orbit has the greatest speed when it's closest to the planet, and the lowest speed when it's farthest from the planet.
I'll assume you mean: "... as opposed to a circular orbit". That is caused by the fact that for a circular orbit, a planet needs a VERY PRECISE SPEED. Change the speed slightly (at a particular point in the orbit), and the orbit immediately becomes elliptical.
in the orbit of a planet there is a point called perihelion which is closest point to the sun and aphelion which is furthest from the sun . Moment of a planet in it's elliptical orbit reaches it's maximum in perihelion
The speed of a satellite in an elliptical orbit around Earth varies depending on its distance from the planet. The satellite moves fastest at the point in its orbit closest to the Earth (perigee) and slowest at the point farthest from the Earth (apogee). The average speed of the satellite can be calculated using the vis-viva equation.
A planet is slowest when it is farthest from the Sun in its elliptical orbit, at its aphelion point.
Dwarf planet Eris has an average orbital speed of about 3.4 km/s or 7,600 mph while orbiting around the Sun. It completes one orbit around the Sun in about 557 Earth years due to its highly elliptical orbit.
A planet's speed in an elliptical orbit around the Sun varies. It moves fastest at the point closest to the Sun (perihelion) and slowest at the point farthest from the Sun (aphelion). This variation is due to conservation of angular momentum in the solar system.
Kepler's Second Law: The planet moves faster when it is closer to the Sun.
The speed of a planet revolving around the Sun is slowest at the aphelion, which is the point in its orbit farthest from the Sun.
Each planet in our solar system revolves around the sun in an elliptical orbit. The time it takes for a planet to complete one revolution around the sun is known as its orbital period. This period varies for each planet based on its distance from the sun.
A planet's movement around the sun is due to the gravitational pull of the sun, which keeps the planet in orbit. The planet moves along its path (orbit) at a constant speed, following an elliptical trajectory due to the balance of gravitational force and the planet's inertia. This movement repeats in a predictable pattern, forming the planet's year.
The gravitational pull exerted by the Sun, which acts as the central force keeping planets in orbit, causes them to move along elliptical paths. The conservation of angular momentum ensures that planets travel in elliptical orbits, with their speed varying at different points along the orbit to maintain this balance.