F= G (m1m2)/(r2)
F= the gravitational force
G= gravitational constant
m1= mass of the first object (the satellite)
m2= mass of the second object (earth)
r= the radius
Plug in the values and solve for r:
690 N= 6.67 X 10-11 ((124kg) X (5.98 X 1024)/(r2)
690r2= 6.67 X10-11 (7.41 X 1026)
690r2= 4.94 X 1016
r2= (4.94 X 1016)/(690)
r= square root of (7.16 x 1013)
r= 8.46 x 106 m, or 846,000 Km
Gravity is the force that allows satellites to orbit the Earth. The gravitational pull between the Earth and the satellite causes the satellite to continuously fall towards the Earth while moving forward at a speed that keeps it in orbit.
Not at all. The mutual gravitational force that attracts the satellite and the earth toward each other is exactly what keeps the satellite in orbit. Without it, the satellite would just take off in a straight line away from the vicinity of the earth.
Satellites A (APEX)
That's the mutual gravitational force of attraction between the satellite and the central body that it's orbiting.
Satellite Leo refers to low Earth orbit (LEO) satellites that orbit the Earth at an altitude of around 2,000 kilometers. These satellites are used for various purposes such as communication, Earth observation, and scientific research. LEO satellites have shorter orbital periods and are closer to Earth compared to other types of satellites, which can result in faster data transmission and lower latency.
gravitational force
Gravity is the force that allows satellites to orbit the Earth. The gravitational pull between the Earth and the satellite causes the satellite to continuously fall towards the Earth while moving forward at a speed that keeps it in orbit.
The satellite that is closer to the planet will experience a larger gravitational force. Gravitational force decreases with distance, following an inverse square law. Therefore, the satellite that is closer will experience a stronger gravitational pull compared to the satellite that is farther away.
A satellite in a higher orbit moves more slowly due to the weaker gravitational pull it experiences compared to satellites in lower orbits. According to Kepler's laws of planetary motion, the orbital period increases with distance from the central body; thus, satellites further from Earth take longer to complete an orbit. This slower speed is a result of the balance between gravitational force and the satellite's inertia, which diminishes with increased distance from the planet.
The reason that satellites stay in orbit around Earth is because of two factors. Velocity and the gravitational pull between the satellite and the Earth.
Not at all. The mutual gravitational force that attracts the satellite and the earth toward each other is exactly what keeps the satellite in orbit. Without it, the satellite would just take off in a straight line away from the vicinity of the earth.
No, satellites do not repel each other. The gravitational force between satellites is attractive, which means they are actually drawn towards each other. This force helps maintain their orbits around a planet.
Satellites A (APEX)
That's the mutual gravitational force of attraction between the satellite and the central body that it's orbiting.
That's the mutual gravitational force of attraction between the satellite and the central body that it's orbiting.
That's the mutual gravitational force of attraction between the satellite and the central body that it's orbiting.
The plural of satellite is satellites.