Table of Contents
- 1 Does an orbit exist where a satellite can stay above the same spot on the earth?
- 2 How far above earth do satellites need to be to stay in orbit?
- 3 How do satellites stay in place?
- 4 How far can satellites travel?
- 5 Why do geostationary satellites stay in orbit?
- 6 What is the size of Mount Olympus Mons?
- 7 What is the orbital radius of the International Space Station?
Does an orbit exist where a satellite can stay above the same spot on the earth?
A geostationary orbit is extremely valuable for weather monitoring because satellites in this orbit provide a constant view of the same surface area. Satellites in geostationary orbit rotate with the Earth directly above the equator, continuously staying above the same spot.
How long does a geostationary satellite stay in orbit?
1,436 minutes
A geostationary orbit can be achieved only at an altitude very close to 35,786 kilometres (22,236 miles) and directly above the equator. This equates to an orbital speed of 3.07 kilometres per second (1.91 miles per second) and an orbital period of 1,436 minutes, one sidereal day.
How far above earth do satellites need to be to stay in orbit?
The aptly titled geosynchronous orbit is described in detail: “At an altitude of 124 miles (200 kilometers), the required orbital velocity is just over 17,000 mph (about 27,400 kph). To maintain an orbit that is 22,223 miles (35,786 km) above Earth, the satellite must orbit at a speed of about 7,000 mph (11,300 kph).
Do geostationary satellites have to be above the equator?
Most commercial and military communications satellites and broadcast satellites operate at GEO. A geostationary transfer orbit is used to move a satellite from low Earth orbit (LEO) into a GEO. Satellites in geostationary orbit must all occupy a single ring above the Equator.
How do satellites stay in place?
Satellites are able to orbit around the planet because they are locked into speeds that are fast enough to defeat the downward pull of gravity. A satellite maintains its orbit by balancing two factors: its velocity (the speed it takes to travel in a straight line) and the gravitational pull that Earth has on it.
Which force keeps the satellite in orbit around the Earth?
gravity
The Short Answer: Even when satellites are thousands of miles away, Earth’s gravity still tugs on them. Gravity—combined with the satellite’s momentum from its launch into space—cause the satellite to go into orbit above Earth, instead of falling back down to the ground.
How far can satellites travel?
It can get pretty crowded. Medium-Earth orbits (MEO) — These satellites park in between the low and high flyers, so from about 1,243 miles (2,000 kilometers) to 22,223 miles (36,000 kilometers). Navigation satellites, like the kind used by your car’s GPS, work well at this altitude.
Why is a geostationary orbit above equator?
Originally Answered: Why is the geostationary orbit necessarily above the equator? Because satellites orbit the center of mass of the planet which is in the center of the planet, more or less. So to orbit the Earth and stay above one place they need to orbit the equator.
Why do geostationary satellites stay in orbit?
So, How Do Satellites Stay in Orbit? A satellite maintains its orbit by balancing two factors: its velocity (the speed it takes to travel in a straight line) and the gravitational pull that Earth has on it. A satellite orbiting closer to the Earth requires more velocity to resist the stronger gravitational pull.
What is a geosynchronous orbit?
A geosynchronous orbit is one in which the satellite remains “in place” above the same spot on the Earth’s surface. Geosynchronous means that the satellite has same period as the earth, back to the same place in 24 hours. h = height of the satellite from the surface of the earth.
What is the size of Mount Olympus Mons?
Olympus Mons is a shield volcano 624 km (374 mi) in diameter (approximately the same size as the state of Arizona), 25 km (16 mi) high, and is rimmed by a 6 km (4 mi) high scarp.
How do you find the mass of a satellite in orbit?
Consider a satellite of mass m in a circular orbit about Earth at distance r from the center of Earth ( Figure ). It has centripetal acceleration directed toward the center of Earth. Earth’s gravity is the only force acting, so Newton’s second law gives GmM E r2 =mac = mv2 orbit r. G m M E r 2 = m a c = m v orbit 2 r.
What is the orbital radius of the International Space Station?
Since the ISS orbits 4.00× 102km 4.00 × 10 2 km above Earth’s surface, the radius at which it orbits is RE +4.00 ×102km R E + 4.00 × 10 2 km. We use Figure and Figure to find the orbital speed and period, respectively.