The radius of the nth orbit in the Bohr model is given by the formula: (r_n = 0.529 \times n^2 / Z), where n is the principle quantum number and Z is the atomic number. For He+, Z = 2 and n = 3, so the radius of the third orbit of He+ would be (r_3 = 0.529 \times 3^2 / 2 = 2.117 Amstraum).
The radius of an orbit is directly related to the average speed of the orbiting body. As the radius of the orbit increases, the average speed of the orbiting body decreases. This is because at a larger distance from the center of mass, the gravitational force decreases, requiring a lower speed to maintain the orbit.
It depends on the radius of the orbit. Different orbit radii have different orbital periods. As an example, one of Mars's natural satellites, Phobos takes 7.66 hours to orbit Mars. It's orbital radius is around 9,400 km.
According to Kepler's Third Law of Planetary Motion, the orbital period of a planet increases with the radius of its orbit. Specifically, the square of the orbital period is proportional to the cube of the semi-major axis of its orbit. Therefore, if the radius of a planet's orbit increases, its orbital period will also increase, resulting in a longer time required to complete one full orbit around the sun or central body.
The answer depends on where the other end of the line segment is. If it is on the circumference the segment is a radius. Otherwise, it is indeterminate.
The radius of the nth orbit in the Bohr model is given by the formula: (r_n = 0.529 \times n^2 / Z), where n is the principle quantum number and Z is the atomic number. For He+, Z = 2 and n = 3, so the radius of the third orbit of He+ would be (r_3 = 0.529 \times 3^2 / 2 = 2.117 Amstraum).
The radius is the distance from the center of the circle to its edge. No matter how you draw this radius, it is one value of one length only, for any given circle.
A geostationary orbit around the Earth has a radius of approximately 42,164 kilometers.
The radius of a geosynchronous orbit around Earth is approximately 42,164 kilometers.
you cant: pi is the same for any circle - 3.1415... the diamter or the radius has to be given diameter divided by two equals the radius the radius times two equals the diameter
For any given circle, the circumference is equal to the radius multiplied by 2 x pi.
The radius of the Moon's orbit is about 60 times larger than the radius of Earth.
The orbit of the Earth has a radius of about 93 million miles.
To calculate the mass of an object in orbit, we can use the period and radius of its orbit by applying Newton's version of Kepler's third law. This formula states that the square of the period of an orbit is proportional to the cube of the semi-major axis of the orbit. By rearranging this formula and plugging in the known values of the period and radius, we can solve for the mass of the object.
152.98 (rounded to 2 d.p) I haven't included units as I haven't been given any but they would be the same units as the units given for the radius.
An orbit.
The radius of an orbit is directly related to the average speed of the orbiting body. As the radius of the orbit increases, the average speed of the orbiting body decreases. This is because at a larger distance from the center of mass, the gravitational force decreases, requiring a lower speed to maintain the orbit.