PRECALCULUS:GRAPHICAL,...-NASTA ED.
PRECALCULUS:GRAPHICAL,...-NASTA ED.
10th Edition
ISBN: 9780134672090
Author: Demana
Publisher: PEARSON
Expert Solution & Answer
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Chapter 8.5, Problem 51E
Solution

a)

To prove:that the perihelion distance of any planet is a1e and the aphelion distance is a1+e using the fact that 1cosθ1 .

It is proved that the perihelion distance of any planet is a1e and the aphelion distance is a1+e .

Given information:

The polar equation: r=a1e21+ecosθ

Formula used:

  a2b2=aba+b

Calculation:

The perihelion distance is defined as the closest distance of any planet to the sun.

So, given the fact that 1cosθ1 , substitute 1 for cosθ in the polar equation.

Therefore

  r=a1e21+e1

Factorize the numerator using the identity a2b2=aba+b and cancel out the common factors.

  r=a1e1+e1+e=a1e

Hence the perihelion distance is a1e .

The aphelion distance is defined as the furthest distance of any planet to the sun.

So, given the fact that 1cosθ1 , substitute 1 for cosθ in the polar equation.

Therefore

  r=a1e21+e1

Factorize the numerator using the identity a2b2=aba+b and cancel out the common factors.

  r=a1e1+e1e=a1+e

Hence the aphelion distance is a1+e .

Therefore, it is proved that the perihelion distance of any planet is a1e and the aphelion distance is a1+e .

b)

To prove: that a1e=ac and a1+e=a+c .

Given information:

The polar equation: r=a1e21+ecosθ

Formula used:

  e=ca

Calculation:

Substitute ca for e in a1e .

  a1ca=aaca=ac

Hence it is proved that a1e=ac .

Substitute ca for e in a1+e .

  a1+ca=a+aca=a+c

Hence it is proved that a1+e=a+c .

c)

To compute:the perihelion and aphelion distances of each planet listed in the table.

The perihelion and aphelion distances are tabulated as follows:

    PlanetSemi major Axis (AU)EccentricityPerihelionAphelion
    Mercury0.38710.2060.3070.467
    Venus0.72330.0070.7180.728
    Earth1.00000.0170.9831.017
    Mars1.52370.0931.3821.665
    Jupiter5.20260.0484.9535.452
    Saturn9.55470.0569.0210.09

Given information:

The semimajor axes and eccentricities of the six innermost planets.

    PlanetSemimajor Axis (AU)Eccentricity
    Mercury0.38710.206
    Venus0.72330.007
    Earth1.00000.017
    Mars1.52370.093
    Jupiter5.20260.048
    Saturn9.55470.056

Source: Encrenaz and Bibring The Solar System (2nd ed.) New York: Springer, p-5.

Formula used:

Formula to compute perihelion distance: a1e

Formula to computer aphelion distance: a1+e

Calculation:

To find the perihelion and aphelion distances of Mercury:

Substitute 0.3871 for a and 0.206 for b in perihelion formula.

  0.387110.206=0.38710.7940.307

Substitute 0.3871 for a and 0.206 for b in aphelion formula.

  0.38711+0.206=0.38711.2060.467

Therefore, the perihelion and aphelion distances for Mercury are 0.307 and 0.467 respectively.

To find the perihelion and aphelion distances of Venus:

Substitute 0.3871 for a and 0.206 for b in perihelion formula.

  0.723310.007=0.72330.9930.718

Substitute 0.3871 for a and 0.206 for b in aphelion formula.

  0.72331+0.007=0.72331.0070.728

Therefore, the perihelion and aphelion distances for Venus are 0.718 and 0.728 respectively.

To find the perihelion and aphelion distances of Earth:

Substitute 1.0000 for a and 0.017 for b in perihelion formula.

  1.000010.017=1.00000.9830.983

Substitute 0.3871 for a and 0.206 for b in aphelion formula.

  1.00001+0.017=1.00001.0171.017

Therefore, the perihelion and aphelion distances for Earth are 0.983 and 1.017 respectively.

To find the perihelion and aphelion distances of Mars:

Substitute 1.5237 for a and 0.093 for b in perihelion formula.

  1.523710.093=1.52370.9071.382

Substitute 0.3871 for a and 0.206 for b in aphelion formula.

  1.52371+0.093=1.52371.0931.665

Therefore, the perihelion and aphelion distances for Mars are 1.382 and 1.665 respectively.

To find the perihelion and aphelion distances of Jupiter:

Substitute 5.2026 for a and 0.048 for b in perihelion formula.

  5.202610.048=5.20260.9524.953

Substitute 0.3871 for a and 0.206 for b in aphelion formula.

  5.20261+0.048=5.20261.0485.452

Therefore, the perihelion and aphelion distances for Jupiter are 4.953 and 5.452 respectively.

To find the perihelion and aphelion distances of Saturn:

Substitute 9.5547 for a and 0.056 for b in perihelion formula.

  9.554710.056=9.55470.9449.020

Substitute 0.3871 for a and 0.206 for b in aphelion formula.

  9.55471+0.056=9.55471.05610.090

Therefore, the perihelion and aphelion distances for Saturn are 9.02 and 10.09 respectively.

The perihelion and aphelion distances are tabulated as follows:

    PlanetSemimajor Axis (AU)EccentricityPerihelionAphelion
    Mercury0.38710.2060.3070.467
    Venus0.72330.0070.7180.728
    Earth1.00000.0170.9831.017
    Mars1.52370.0931.3821.665
    Jupiter5.20260.0484.9535.452
    Saturn9.55470.0569.0210.09

d)

To find:the greatest perihelion and aphelion distances.

The planet Saturn has the greatest difference between the perihelion and aphelion and the difference is 1.07 .

Given information:

The polar equation: r=a1e21+ecosθ

Formula used:

Formula to compute perihelion distance: a1e

Formula to computer aphelion distance: a1+e

Calculation:

The difference between perihelion and aphelion distances are tabulated as follows:

    PlanetPerihelionAphelionDifference between Perihelion and Aphelion
    Mercury0.3070.4670.4670.307=0.16
    Venus0.7180.7280.7280.718=0.01
    Earth0.9831.0171.0170.983=0.034
    Mars1.3821.6651.6651.382=0.283
    Jupiter4.9535.4525.4524.953=0.499
    Saturn9.0210.0910.099.02=1.07

The greatest difference between the perihelion and aphelion is the least value in the last column.

Therefore, the planet Saturn has the greatest difference between the perihelion and aphelion and the difference is 1.07 .

Chapter 8 Solutions

PRECALCULUS:GRAPHICAL,...-NASTA ED.

Ch. 8.1 - Prob. 1ECh. 8.1 - Prob. 2ECh. 8.1 - Prob. 3ECh. 8.1 - Prob. 4ECh. 8.1 - Prob. 5ECh. 8.1 - Prob. 6ECh. 8.1 - Prob. 7ECh. 8.1 - Prob. 8ECh. 8.1 - Prob. 9ECh. 8.1 - Prob. 10ECh. 8.1 - Prob. 11ECh. 8.1 - Prob. 12ECh. 8.1 - Prob. 13ECh. 8.1 - Prob. 14ECh. 8.1 - Prob. 15ECh. 8.1 - Prob. 16ECh. 8.1 - Prob. 17ECh. 8.1 - Prob. 18ECh. 8.1 - Prob. 19ECh. 8.1 - Prob. 20ECh. 8.1 - Prob. 21ECh. 8.1 - Prob. 22ECh. 8.1 - Prob. 23ECh. 8.1 - Prob. 24ECh. 8.1 - Prob. 25ECh. 8.1 - Prob. 26ECh. 8.1 - Prob. 27ECh. 8.1 - Prob. 28ECh. 8.1 - Prob. 29ECh. 8.1 - Prob. 30ECh. 8.1 - Prob. 31ECh. 8.1 - Prob. 32ECh. 8.1 - Prob. 33ECh. 8.1 - Prob. 34ECh. 8.1 - Prob. 35ECh. 8.1 - Prob. 36ECh. 8.1 - Prob. 37ECh. 8.1 - Prob. 38ECh. 8.1 - Prob. 39ECh. 8.1 - Prob. 40ECh. 8.1 - Prob. 41ECh. 8.1 - Prob. 42ECh. 8.1 - Prob. 43ECh. 8.1 - Prob. 44ECh. 8.1 - Prob. 45ECh. 8.1 - Prob. 46ECh. 8.1 - Prob. 47ECh. 8.1 - Prob. 48ECh. 8.1 - Prob. 49ECh. 8.1 - Prob. 50ECh. 8.1 - Prob. 51ECh. 8.1 - Prob. 52ECh. 8.1 - Prob. 53ECh. 8.1 - 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