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A star of mass 7×1030kg is located at <5×1012,2×1012,0>m.A planet of mass 3×1024kg and is located at <3×1012,4×1012,0>m and is moving with a velocity of <0.3×104,1.5×104,0>m/s (a) At a time 1×106s later what is the new velocity of the planet? (b) Where is the planet at this later time? (c) Explain briefly why the procedures you followed in parts (a) and (b) were able to produce usable results but wouldn’t work if the later time had been 1×109s instead of 1×106s after the initial time. Explain briefly how you could use a computer to get around this difficulty.

Short Answer

Expert verified
  1. The velocity of the planet is 0.26×104,1.54×104,0m/s

  2. The position of the planet is 3.0029×1012,4.015×1012,0m


  3. The values obtained for the velocity and the location of the planet will change very rapidly (due to the larger values). Therefore, these results will not be useful.

Step by step solution

01

Identification of given data

The mass of the star is mstar=7×1030kg

The location of the star is rstar=5×1012,2×1012,0m

The mass of the planet is mplanet=3×1024kg

The location of the planet is rplanet=3×1012,4×1012,0m

The initial velocity of the planet isu=0.3×104,1.5×104,0m/s

02

Concept Introduction

The gravitational attraction between two massive bodies of masses m1and m2 having a separation of r can be expressed as,

F=Gm1m2|r|2r^.........................(1)

03

Calculate the net gravitational force and acceleration of the planet

Distance between the star and the planet can be given as,

r=rplanet-rstar=3×1012,4×1012,0m-5×1012,2×1012,2×1012,0m=-2×1012,2×1012,0m

Thus the magnitude of the distance is,

r=-2×1012m2+2×1012m2+0=2.83×1012m

The unit vector of the distance is,

r^=rr=-2×1012,2×1012,0m2.83×1012m=-0.707,0.707,0

Thus the net gravitational force on the planet due to the star can be given using equation (1) such that,

FPlanet=GmstarmPlanetr2=6.67×10-11N·m2/kg2×7×1030kg×3×1024kg2.83×1012m2=1.75×1020N

Thus the acceleration of the planet due to this attractive gravitational force will be,

aplanet=FPlanetmplanetr^=1.75×1020N3×1024kgr^=5.84×10-5m/s2r^

04

Calculation of the velocity (a)

According to Newton’s first law of motion, the velocity can be calculated as,

v=u+at=0.3×104,1.5×104,0m/s+10-5m/s2×1×106s×-0.707,0.707,0=0.3×104,1.5×104,0m/s+-0.04×104,0.04×104,0m/s=0.26×104,1.54×104,0m/s

Thus the velocity of the planet is 0.26×104,1.54×104,0m/s

05

Calculation of the position (b)

According to Newton’s second law of motion, the velocity can be calculated as,

s=s0+ut+12at2=3×1012,4×1012,0m+0.3×104,1.5×104,0m/s×1×106s+12×5.84×10-5m/s2×1×106s2×-0.707,0.707,0=3×1012,4×1012,0m+3×109,1.5×1010,0m+-2.06×107,2.06×107,0m=3.0029×1012,4.015×1012,0m

Thus the position of the planet is3.0029×1012,4.015×1012,0m

06

Calculation of the position (c)

If the later time is 1×109 instead of 1×106 after the initial time then we can see from the calculations done in parts (a) and (b) that the values obtained for the velocity and the location of the planet will change very rapidly (due to the larger values). Therefore, these results will not be useful.

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