Orbits Pg. 297 - 303.

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Presentation transcript:

Orbits Pg. 297 - 303

Satellites A satellite is an object or body that revolves around another body that usually has much more mass than the satellite For example, the planets are natural satellites of the Sun and the planetary moons are natural satellites of the planets

Satellites Artificial satellites, on the other hand, are human- made objects that orbit Earth or other bodies in the solar system RADARSAT-1 and RADARSAT-2 as well as the International Space Station (ISS) are examples of artificial satellites

Satellites Another well-known example of artificial satellites is the network of 24 satellites that make up the Global Positioning System (GPS) The data from one satellite will show that the object is somewhere along the circumference of the circle Two satellites consulted simultaneously will refine the location to one of two intersection spots With three satellites, the intersection of the three circles will give the location of the object to within 15 km of its actual position

Satellites in Circular Orbits When Newton developed the idea of universal gravitation, he also theorized that the same force that pulls objects to Earth also keeps the Moon in its orbit One difference, of course, is that the Moon does not hit the Earth’s surface The moon orbits Earth at a distance from Earth’s centre – called the orbital radius

Satellites in Circular Orbits The moon’s orbit, similar to the orbits of the planets around the Sun, is actually elliptical However, for most problem-solving purposes, we can closely approximate the orbits by assuming that they are circular

Satellites in Circular Orbits To analyze the motion of a satellite in uniform circular motion about Earth:

Orbital Speed The speed needed by a satellite to remain in orbit

Practice 1. Determine the speeds of Venus and Earth as they orbit the Sun. Venus has an orbital radius of 1.08 x 1011 m while Earth has an orbital radius of 1.49 x 1011 m. The mass of the Sun is 1.99 x 1030 kg. 2. Material has been observed in a circular orbit around a black hole some five thousand light-years away from Earth. Spectroscopic analysis of the material indicates that it is orbiting with a speed of 3.1 x 107 m/s. If the radius of the orbit is 9.8 x 105 m, determine the mass of the black hole, assuming the matter being observed moves in a circular orbit around it.

3. What is the difference between a geosynchronous orbit and a geostationary orbit?

4. The International Space Station orbits Earth at an altitude of ~ 350 km above Earth’s surface. If the mass of the Earth is ~ 5.98 x 1024 kg and the radius of Earth is ~ 6.38 x 106 m, determine the speed needed by the ISS to maintain its orbit (hint: rISS = rEarth + raltitude) Textbook: Pg. 303, #6, 7, 9 Pg. 307, # 1- 4 (PJ: General Relativity)  you will need to read!!