The North Star points towards the compass point North.
The latitude and longitude of that point is known as the celestial body's geographic ... (Two other common methods for determining one's position using celestial ... The sextant and octant are most accurate because they measure angles.
the north star ,polaris
The Moon The north Star or The Sun
No sun doesn't revolve to any celestial body, but the celestial body revolve around the sun.
satellite
To determine the period of orbit for a celestial body, one can use Kepler's Third Law of Planetary Motion, which states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit. By measuring the semi-major axis of the orbit and the gravitational force acting on the celestial body, one can calculate the period of its orbit.
The moonMoon is the closet celestial body.
To derive the escape velocity of an object from a celestial body, you can use the formula: escape velocity (2 gravitational constant mass of celestial body / distance from the center of the celestial body). This formula takes into account the gravitational pull of the celestial body and the distance of the object from its center. By calculating this value, you can determine the minimum velocity needed for an object to escape the gravitational pull of the celestial body.
Latitude is not based on any celestial observation, but rather the geographical location - how far north or south the place is - with respect to the equatorial circle. You could say it is based on terrestrial observation, if you like.
To use a sextant at sea, you measure the angle between a celestial body (like the sun or a star) and the horizon. By comparing this angle with the known position of the celestial body at a specific time, you can calculate your position on the Earth's surface. This method is known as celestial navigation and has been used by sailors for centuries to determine their location on the open sea.
A celestial body is any physical body beyond the earth's atmosphere.
To calculate the Lagrange points in a celestial system, one can use mathematical equations that consider the gravitational forces between the celestial bodies involved. These points are where the gravitational forces of two large bodies, such as a planet and a moon, balance out the centrifugal force of a smaller body, like a spacecraft. There are five Lagrange points in a celestial system, labeled L1 to L5, each with specific calculations based on the masses and distances of the bodies in the system.