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
12 times 12 times 12 is equal to 1,728.
8 times 15 times 50 is equal to 6,000.
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.
Kepler's second law, also known as the law of equal areas, states that a planet sweeps out equal areas in equal times as it moves around the Sun. This means that a planet travels faster when it is closer to the Sun in its orbit and slower when it is farther away.
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.
Yes, the distance from the sun affects the speed of a planet's orbit. According to Kepler's laws of planetary motion, a planet moves faster when it is closer to the sun and slower when it is farther away. This relationship is known as the law of equal areas, which states that a planet sweeps out equal areas in equal times as it orbits the sun.
Kepler discovered that planets move faster when they are closer to the sun in their elliptical orbits. This relationship is described by Kepler's second law of planetary motion, which states that a planet sweeps out equal areas in equal times as it orbits the sun.
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 describe the motion of planets around the sun. They state that planets move in elliptical orbits with the sun at one of the foci (First law), that a line between a planet and the sun sweeps out equal areas in equal times (Second law), and that the square of a planet's orbital period is proportional to the cube of its average distance from the sun (Third law).