[Solution] Theoretical Question 1

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APHO II 2001 Theoretical Question 1 2020/04/12 12:45 PM p.

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[Solution] Theoretical Question 1

When will the Moon become a Synchronous Satellite?

(1) The total orbital angular momentum

L

L z

ˆ of the Earth-Moon system with respect to C can be calculated as follows.

Since all angular momenta are along the z -direction, only the z -component of each angular momentum will be calculated. The distance between the center of mass C and the center of the Earth O is r

CM

M

Mr

0

M

E

1

3 .

85

10

8

( 597 / 7 .

35 )

4 .

68

10

6 m

0 .

735 R

E

The angular speed of the Moon 's revolution is

0

2

27 .

322

86400

2 .

6617

10

6 rad / s (1a)

The orbital angular momentum of the Moon about C is

M

M ( r

0

 r

CM

)

2 

0

7 .

35

( 385

4 .

68 )

2 

2 .

6617

10

28 

2 .

83

10

34 kg

 m

2

/ s

The angular speed of the Moon's spinning or rotational motion is

M

 

0

2 .

6617

10

6 r a d / s

The spin angular momentum of the Moon is

S

M

2

5

MR

2

M

M

2

5

7 .

35

( 1 .

74 )

2

2 .

37

10

29 kg

 m

2

/ s

2 .

6617

10

28

8 .

40

10

6 

M

This is much smaller than the Moon's orbital angular momentum and can therefore be neglected .

The orbital angular momentum of the Earth about C is

E

M

E r

2

CM

0

M

M

M

E

7 .

35

597

2 .

83

10

34 

3 .

48

10

32 kg

 m

2

/ s

The angular speed of the Earth's spinning motion is

E

2

23 .

933

3600

7 .

2926

10

5 r a d / s

The moment of inertia of the Earth about its axis of rotation is

I

2

M

E

R

E

2

5

0 .

4

5 .

97

( 6 .

37 )

2 

10

36 

9 .

69

10

37

The spin angular momentum of the Earth is km

 m

2

/ s (1b)

S

E

2

5

M

E

R

2

E

E

7 .

07

10

33 kg

 m

2

/ s

20 .

3 

E

1

APHO II 2001 Theoretical Question 1 2020/04/12 12:45 PM p.

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[Solution] (continued) Theoretical Question 1

When will the Moon become a Synchronous Satellite?

Thus, the total angular momentum of the Earth-Moon system L is given by

L

( 

M

 

E

S

E

S

M

)

( 2 .

83

0 .

0348

0 .

707

0 .

0000237 )

10

34

(2)

3 .

57

10

34 kg

 m

2

/ s

Note that L

( 

M

 

E

S

E

) .

(2) According to Newton's form for Kepler's third law of planetary motions, the angular speed

of the revolution of the Moon about the Earth is related to the

Earth-Moon distance r by

 2 r

3 

G ( M

E

M ) (3)

Therefore, the orbital angular momentum of the Earth-Moon system with respect to C is

 

(

M

M

E

M

M

E

) r

2  

MM

E

(

( M

G

2

M

E

)

)

1 / 3

(4)

(Note: 

M

M (

M

M

E r

M

)

2 

, 

E

M

E

(

M

M

 r

M

E

)

2 

so that   

E

 

M

.)

E

When the angular speed

 of the Earth's rotation is equal to the angular speed

 of the orbiting Moon, the total angular momentum of the Earth-Moon system is, with the spin angular momentum of the Moon neglected , given by

( 

M

 

E

S

E

)

MM

E

{

( M

G

2

M

E

)

}

1 / 3 

2

5

M

E

R

E

2

7 .

35

5 .

97

66 .

726

{

( 5 .

97

66 .

726

0 .

0735 )

}

1 / 3 

10

30 

9 .

69

10

37 

(5a)

3 .

96

10

32  

1 / 3 

9 .

69

10

37  

3 .

57

10

34

The last equality follows from conservation of total angular momentum and Eq.(2).

For an initial estimate of

, the spin angular momentum of the Earth may be neglected in Eq.(5a) to give

  

1

(

3 .

96

357

)

3 

1 .

36

10

6 rad / s (first iteration)

An improved estimate may be obtained by using the above estimated value

1

to compute the spin angular momentum of the Earth and use Eq.(5a) again to solve for

. The result is

2

APHO II 2001 Theoretical Question 1 2020/04/12 12:45 PM p.

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[Solution] (continued) Theoretical Question 1

When will the Moon become a Synchronous Satellite?

   f

(

3 .

96

358

)

3 

1 .

35

10

6 rad / s (second iteration) (5b)

Further iterations of the same procedure lead to the same value just given. Thus, the period of rotation of the Earth will be

T f

2

 f

6 .

2832

1 .

35

10

6 

86400

53 .

9 d a y s

(3) Since the total torque

 is proportional to 1 / r

6

, we conclude r

6   constant (6)

F x

( x

0 )

Fig.1e r

ˆ



Moon

O

( x

0 )

Earth

F x

Let the current values of r and



be, respectively, r

0

and

0

. From Eq.(6), we then have

The torque

 is equal to the

 

( r r

0

)

6 

0

(7) rate of change of spin angular momentum I

of the Earth so that

I d

 

(8) dt

By Newton's law of action and reaction or by the law of conservation of the total angular momentum,

 

is equal to the rate of change of the total orbital angular momentum  of the Earth-Moon system so that d  dt

  

(9)

But according to Eq.(3), we have

 2 r

3 

G ( M

E

M ) and Eq.(4) may be written as

3

APHO II 2001 Theoretical Question 1 2020/04/12 12:45 PM p.

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 

(

M

MM

E

E

M

)

 r

2 

MM

E

(

M

E

G

M

)

1 / 2 r

1 / 2

(10)

MM

E

(

M

E

G

2

M

)

1 / 3  

1 / 3

This implies

The value of

0 d  dt

MM

1

3

E

(

MM

M

E

(

E

G

M

E

M

G

2

)

1 /

M

2

2

)

1 / r

3

1

1 /

2

1

4 / dr dt

3 d

 dt

  

can be determined from Eq. (11a) as follows:

(11a)

 

0

( d  dt

)

0

1

2

MM

E

1

2

7 .

35

5 .

97

( M

E

G

M ) r

0

( dr dt

)

0

10

46 

66 .

7

10

44

( 0 .

0735

5 .

97 )

( 3 .

85 )

3 .

8

10

8

3 .

65

8 .

64

(13)

4 .

5

10

16

N

 m

Starting with Eq.(11a) in the following form d  dt

 

1

3

MM

E

(

( M

E

G

2

M )

)

1 / 3

1

4 / 3 d

 dt

 

( r

0 r

)

6 

0 we may use Eq.(3) to express r in terms of

 and obtain the following equations

1

3

MM

E

(

( M

E

G

2

M )

)

1 / 3

( d

) dt

{ G

( r

0

)

6

( M

E

0

M )}

2

 16 / 3

[Solution] (continued) Theoretical Question 1

When will the Moon become a Synchronous Satellite? d

 dt

3 ( r

0

)

6

[

GM

E

M { G ( M

E

0

M )}

5 / 3

]

 16 / 3  b

 16 / 3 where the constant b stands for the expression in the square brackets. The last equation leads to the solution where t f

(

 f

)

13 / 3 

(

0

)

13 / 3 

13 b

( t f

3

0 )

is the length of time needed for the angular speed of the rotation of the

Earth to be equal to that of the Moon's revolution about the Earth.

Using the values of

 f and

0 obtained in Eqs.(1a) and (5b) and the value of

0

in Eq.(13), we have

3

13 b

GM

E

M { G ( M

13 ( r

0

)

6

E

(

 

0

M

)

)}

5 / 3

3 .

4

10

8

4

APHO II 2001 Theoretical Question 1 2020/04/12 12:45 PM p.

5 / 5 t f

3

13 b

(

 

13 f

/ 3   

13 /

0

3

)

3 .

4

{( 1 .

35 )

13 / 3

3 .

4

10

18 

( 0 .

254

0 .

014376 )

( 2 .

6617 )

13 / 3

}

10

18

8 .

1

10

17 sec onds

2 .

6

10

10 years

5

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