17.28 Satellites

Before you read this, I suggest you read posts 16.16 and 17.13

satelitt-1820106_640

Why does a satellite stay in orbit around the earth? If we think of something going round in a circle (like the hammer in post 17. 13 before it is thrown), it appears that something must be pulling it towards the earth. What can this “something” be? The only possibility is the force exerted by the earth’s gravitational field (post 16.16) that has a magnitude of GMm/r2 where G is the universal gravitational constant, M is the mass of the earth, m is the mass of the satellite and r is the distance of the satellite from the centre of the earth.

This gravitational force provides the centripetal force (post 17.13) to keep the satellite moving in a circle. The magnitude of the centripetal force for an object of mass m and angular speed (post 17.12) ω is mω2r where r is the radius of the circle (post 17.13). Since this force is provided by the earth’s gravitational field, we can write the equation

mω2r = GMm/r2.

If we divide both sides of this equation by m and then divide each side by r, we get the result that

ω2 = GM/r3.               (1)

Dividing both sides of equation 1 by ω2 and multiplying both sides by r3 gives the result that

r3 = (GM/ω2).               (2)

To find r, we take the cube root of both sides of equation 2. The cube root of a number is the number that we need to multiply by itself three times to get the original number. So, the cube root of 8 is 2 because 2 × 2 × 2 = 8. We could write this as 81/3 = 2. Taking the cube root of both sides of equation 3 gives

r = (GM/ω2)1/3.               (3)

Equation 3 relates the angular speed of the satellite to the radius of its orbit.

As an example, let’s find the radius for the orbit of a geostationary satellite. Let’s suppose that we always want the satellite to appear in the same place when viewed from a fixed point on the equator. The satellite must have an angular speed of 2π/(24 × 60 × 60) = 7.272 × 10-5 rad.s-1 (post 17.12) because it rotates through 2π radians (1 complete revolution, see post 17.11) every 24 hours or 24 × 60 × 60 seconds. (If you’re not sure about the way I’ve written the result for the angular speed, see post 16.7)

G has a value of 6.674 ×10-11 m3.kg-1.s-2 and M has a value of 5.972 ×1024 kg. Putting these values and the required value for ω into equation 3 gives the result that r = 4.2 × 107 m which equals 4.2 × 104 km. (If you want to repeat the calculation and aren’t sure how to work out the cube root, see the appendix).

Since the radius of the earth is 0.6 × 104 km, the height of the satellite above the surface of the earth is (4.2 – 0.6) × 104 = 3.6 × 104 km.

16.28 Diagram cropped

To get the satellite into orbit it is first launched into space using a rocket (see posts 17.26 and 17.27). When it has reached the required height, it is released and propelled at right angles to the direction of the rocket with a speed v = ωr (see post 17.12), where ω and r have the values we have already calculated, in the direction of the earth’s rotation (see diagram above).

Why doesn’t a satellite fall? It does! It is in orbit because it is being attracted by the earth’s gravitational field – which is another way of saying that it’s falling (posts 16.16 and 17.20) If it didn’t fall (because the gravitational field suddenly ceased to exist) it would fly off at a tangent to its orbit – just like the hammer of post 17.13 when the thrower stops pulling the cable.

But sometimes satellites do fall closer to earth. When they meet the earth’s atmosphere, the drag forces lead to loss of a lot of energy (post 17.17). This energy is lost as heat (post 16.35) and the satellite debris burns – the result can sometimes be seen in the night sky. Why do they fall closer to earth? One reason is because of collisions with other objects.

But the important point is that a satellite in stable orbit is always falling. The gravitational force that makes it fall provides the centripetal force to keep it in orbit.

 

Related posts

17.27 Getting into space
17.26 Rockets
17.16 Why do planes fly?

 

Appendix

It is easy to calculate that r3 = 7.537 × 1022 m3, using equation 2. But how do we calculate r from this result?

Type = log10(7.537*10^22) into a cell in the Excel spreadsheet. You will get the answer 22.877198. This answer means that 1022.877198 = 7.537 × 1022.

So, the cube root of 7.537 × 1022 is equal to 1022.877198/3 = 107.6257328.

Now type = 10^7.6257328 into another cell in Excel to obtain the value of r, written in the usual way, in m.

 

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