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Consider a spacecraft in an elliptical orbit around the earth. At the low point, or perigee, of its orbit, it is 400 km above the earth’s surface; at the high point, or apogee, it is 4000 km above the earth’s surface. (a) What is the period of the spacecraft’s orbit? (b) Using conservation of angular momentum, find the ratio of the spacecraft’s speed at perigee to its speed at apogee. (c) Using conservation of energy, find the speed at perigee and the speed at apogee. (d) It is necessary to have the spacecraft escape from the earth completely. If the spacecraft’s rockets are fired at perigee, by how much would the speed have to be increased to achieve this? What if the rockets were fired at apogee? Which point in the orbit is more efficient to use?.

Short Answer

Expert verified
  1. The time period of spacecraft orbit is,7.9×103 s .
  2. The ratio of the spacecraft’s speed at perigee to its speed at apogee is, 1.53.
  3. Thespeed of apogee and speed of perigee are5.52×103″¾/s and8.4×103″¾/s
  4. The increase speed of perigee and apogee are2.4×103″¾/s and3.24×103″¾/s.

Step by step solution

01

Identification of the given data

The given data can be listed below as,

  • The distance of perigee from the earth’s surface is,hp=400 k³¾.
  • The distance of apogee from the earth’s surface is,role="math" localid="1655735322547" ha=4000 k³¾.
02

Significance of conservation of energy

The total amount of energy of an isolated system remains stable, even though internal changes occur when energy disappears in one form and appears in another.

03

Determination of the period of the spacecraft’s orbit

a)

The spacecraft moving in an elliptical orbit, the relation between the time period, the mass of earth, and the semi-major axis is expressed as,

T=2Ï€a3/2GME ...(i)

Here Tis the time period, role="math" localid="1655735444026" ais the semi-major axis of an elliptical orbit, Gis the gravitational constant, and MEis the mass of the sun.

The major axis of an elliptical orbit is expressed as,

2a=ra+rp ...(ii)

Hererole="math" localid="1655735530960" 2ais the major axis of an elliptical orbit,role="math" localid="1655735628136" rais the radius of apogee andrpis the radius of perigee. The radius of apogee and the radius of perigee are expressed as,

ra=ha+RE

And

rp=hp+RE

HereREis the radius of the earth.

Substitute the value of raand rpin equation (ii)

2a=ha+RE+hp+RE=2RE+ha+hpa=RE+(ha+hp)2

Substitute6.37×106″¾ forRE ,400×103″¾ forhp , and4000×103″¾ forha in the above equation.

a=6.37×106″¾+(400×103″¾+4000×103″¾)2=8.57×106″¾

Substitute6.673×10−11 N³¾2/kg2 for G,8.57×106″¾ fora , and5.97×1024 k²µ forME in the equation (i).

T=2π×(8.57×106″¾)326.673×10−11 N³¾2/kg2×5.97×1024 k²µ=7.9×103 s

Hence the time period of spacecraft orbit is,7.9×103 s .

04

Determination of the ratio of the spacecraft’s speed at perigee to its speed at apogee

b)

The conservation of angular momentum between apogee and perigee is expressed as,

rava=rpvpvpva=rarp

HereVP is the speed of perigee andVa is the speed of apogee.

Substitute the value of rpandra in the above equation.

vpva=ha+REhp+RE

Substitute6.37×106″¾ for RE,400×103″¾ for hp, and 4000×103″¾forha in the above equation.

vpva=4000×103″¾+6.37×106″¾400×103″¾+6.37×106″¾=1.53

Hence the ratio of the spacecraft’s speed at perigee to its speed at apogee is, 1.53.

05

Determination of the acceleration due to Miranda’s gravity at the surface of Miranda

c)

The conservation of energy to apogee and perigee is expressed as

Ka+Ua=Kp+Up ...(iii)

HereKaand KPare the kinetic energy of apogee and perigee androle="math" localid="1655736678099" UaandUPare the gravitational potential energy of apogee and perigee.

The kinetic and potential energy of apogee is expressed as,

Ka=12mva2

And

Ua=GMEmra

The kinetic and potential energy of perigee is expressed as,

Kp=12mvp2

And

Up=GMEmrp

Substitute the value of Ka, Kp,role="math" localid="1655736829112" UaandUPin the equation (iii).

12mva2+GMEmra=12mvp2+GMEmrpvp2−va2=2GME1rp−1ra=2GMEra−rprarp

Substitute the value of Vpin the above equation.

(1.53va)2−va2=2GMEra−rprarp1.341va2=2GMEra−rprarp

Substitute the value of rpand rain the above equation.

1.341va2=2GMEha+RE−hp−RE(ha+RE)(hp−RE)1.341va2=2GMEha−hp(ha+RE)(hp+RE)

Substitute 6.673×10−11 N³¾2/kg2for G, 6.37×106″¾for RE, 400×103″¾for hp, 4000×103″¾for ha, and 5.97×1024 k²µ for MEin the above equation.

1.341va2=2×6.673×10−11 N³¾2/kg2×5.97×1024 k²µÃ—4000×103″¾âˆ’400×103″¾(4000×103″¾+6.37×106″¾)(400×103″¾+6.37×106″¾)va=5.52×103″¾/s

And

vpva=1.53vp=1.53va

Substitute the value of vain the above equation.

vp=1.53×5.52×103″¾/s=8.4×103″¾/s

Hence the speed of apogee and speed of perigee are5.52×103″¾/s and8.4×103″¾/s .

06

Determination of the speed of apogee and perigee to escape the spacecraft from the earths

d)

The spacecraft escape from earths then the total energy is expressed as,

E=K+U

HereK andUare the kinetic and gravitational potential energy. For determine speed,E=0. Then the total energy expressed as,

K+U=0 ...(iv)

At perigee, kinetic and gravitational potential energy is expressed as,

Kp=12mvp2

And

Up=−GMEmrp

Substitute the value of rp,in the above equation.

Up=−GMEmhp+RE

Substitute the value of Kp, and Upin the equation (iv).

12mvp2−GMEmhp+RE=0vp=2GMEhp+RE

Substitute 6.673×10−11 N³¾2/kg2for G, 6.37×106″¾for RE, 400×103″¾for hPand 5.97×1024 k²µfor MEin the above equation.

vp=2×6.673×10−11 N³¾2/kg2×5.97×1024 k²µ400×103″¾+6.37×106″¾=1.085×104″¾/s

Hence the increase of speed of is,(1.085×104″¾/s−8.4×103″¾/s)=2.4×103″¾/s

At apogee, kinetic and gravitational potential energy is expressed as,

Ka=12mva2

And

Ua=−GMEmra

Substitute the value of ra,in the above equation.

Ua=−GMEmha+RE

Substitute the value of Ka, andUa in the equation (iv).

12mva2−GMEmha+RE=0va=2GMEha+RE

Substitute6.673×10−11 N³¾2/kg2 for G,6.37×106″¾ forRE ,4000×103″¾ forha and5.97×1024 k²µ forME in the above equation.

vp=2×6.673×10−11 N³¾2/kg2×5.97×1024 k²µ4000×103″¾+6.37×106″¾=8.76×103″¾/s

Hence the increase of speed of is,(8.76×103″¾/s−5.52×103″¾/s)=3.24×103″¾/s

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