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16 time 1 equals 16 16 times 2 equal 32 16 times 3 equal 48 16 times 4 equal 64 16 times 5 equal 80 16 times 6 equal 96 16 times 7 equal 112 16 times 8 equal 128 16 times 9 equal 144 16 times 10 equal 160
8 times 15 times 50 is equal to 6,000.
12 times 12 times 12 is equal to 1,728.
It is: 4.21875 times 32 = 135
What does ten times eighty equal? well, it equals 800.
In equal times, a line segment between the planet and the sun sweeps out equal areas. This concept is known as Kepler's second law of planetary motion. It implies that planets move faster when they are closer to the sun and slower when they are farther away, maintaining a balance between gravitational force and orbital speed.
He thought that the planet went around the sun over 40,000 times faster than in reality. He was a very imaginative person.Really he thought that the closer it was to the sun in its orbit the faster it had to go.
According to Kepler's 2nd Law, as a planet moves around its orbit, it sweeps out equal areas in equal times. This means that a planet will move faster when it is closer to the sun (perihelion) and slower when it is farther away (aphelion) to ensure this law is followed.
Kepler's Laws of Planetary Motion:1] Each planet moves in an elliptical orbit with the sun at one focus2] The line form the sun to any planet sweeps out equal areas of space in equal time intervals3] The squares of the times of revolution (days, months or years) of the planets are proportional to the cubes of their average distances from the sun.
Kepler's Laws of Planetary Motion:1] Each planet moves in an elliptical orbit with the sun at one focus2] The line form the sun to any planet sweeps out equal areas of space in equal time intervals3] The squares of the times of revolution (days, months or years) of the planets are proportional to the cubes of their average distances from the sun.
Kepler's Laws of Planetary Motion:1] Each planet moves in an elliptical orbit with the sun at one focus2] The line form the sun to any planet sweeps out equal areas of space in equal time intervals3] The squares of the times of revolution (days, months or years) of the planets are proportional to the cubes of their average distances from the sun.
Kepler's Laws of Planetary Motion:1] Each planet moves in an elliptical orbit with the sun at one focus2] The line form the sun to any planet sweeps out equal areas of space in equal time intervals3] The squares of the times of revolution (days, months or years) of the planets are proportional to the cubes of their average distances from the sun.
Kepler's Laws of Planetary Motion:1] Each planet moves in an elliptical orbit with the sun at one focus2] The line form the sun to any planet sweeps out equal areas of space in equal time intervals3] The squares of the times of revolution (days, months or years) of the planets are proportional to the cubes of their average distances from the sun.
Kepler's Laws of Planetary Motion:1] Each planet moves in an elliptical orbit with the sun at one focus2] The line form the sun to any planet sweeps out equal areas of space in equal time intervals3] The squares of the times of revolution (days, months or years) of the planets are proportional to the cubes of their average distances from the sun.
Kepler's laws are three principles that describe the motion of planets around the Sun. They state that planets move in elliptical orbits with the Sun at one focus, that a line segment joining a planet and the Sun sweeps out equal areas in equal intervals of time, and that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun.
Kepler's law of ellipses states that a planet orbits the Sun in an elliptical path with the Sun located at one of the two foci of the ellipse. This means that a planet does not move in a perfect circle around the Sun, but rather in an elongated oval shape.
A planet closer to the sun moves faster because the gravitational pull from the sun is stronger at that distance, causing the planet to accelerate. This is described by Kepler's second law of planetary motion, which states that a planet will sweep out equal areas in equal times as it orbits the sun.