Early astronomers called this an "epicycle"; a whirling circle whose center was traveling in a larger circle. They used this to try to explain the observed motions of the planets, because Aristotle said that all motion in the heavens was circular, and so ellipses were right out!
The furthest point from the center is the circumference of the circle.
A rainbow forms a circular arc in the sky, with its center located at the antisolar point, which is the point directly opposite to the sun. However, when viewed from the ground, only a portion of the arc is usually visible to the observer due to the horizon.
The shape of the orbit of each planet is an ellipse. An ellipse is a geometric shape that is like a flattened circle. The Sun is located at one of the foci of the ellipse, not at the center.
This set of points forms a circle with the fixed point as its center.
The centripetal force is responsible for pulling objects toward the center of a circle as they move in a curved path. This force acts perpendicular to the velocity of the object, keeping it on a circular trajectory.
Diameter. distasnce from center to edge is radius length around is circumfrance
Formula to find the circumfrance of a circle~(2)(3.14)r or (3.14)d
it is the circumfrance of a circle divided by pi.
If the circumference (not circumfrance) is 31.4, the radius is 4.9975 units (to 4 dp).
8
125.6 feet
The diameter should be 7m.
Work it out the circumfrance of a circle is pie x the diameter!
circumference = 2*pi*5
Diameter is the distance across a circle. The circumference of a circle is the distance around the outside of the circle.
multiply the radius by two then pultiply that by pi
3.9 x 3.14 m