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A planet orbits a star at a distance of 3.0 × 10^7 m - Scottish Highers Physics - Question 5 - 2016

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A planet orbits a star at a distance of 3.0 × 10^7 m. The star exerts a gravitational force of 1.6 × 10^7 N on the planet. The mass of the star is 6.0 × 10^30 kg. Th... show full transcript

Worked Solution & Example Answer:A planet orbits a star at a distance of 3.0 × 10^7 m - Scottish Highers Physics - Question 5 - 2016

Step 1

Step 1: Use the formula for gravitational force

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Answer

The gravitational force between two masses is given by the formula: F=Gm1m2r2F = G \frac{m_1 m_2}{r^2} where:

  • FF is the gravitational force,
  • GG is the gravitational constant (6.674×1011  N m2/kg26.674 × 10^{-11} \; \text{N m}^2/\text{kg}^2),
  • m1m_1 and m2m_2 are the masses of the two objects,
  • rr is the distance between the centers of the two masses.

In this case, m1m_1 is the mass of the star (6.0×1030  kg6.0 × 10^{30} \; \text{kg}), m2m_2 is the mass of the planet (which we need to find), and rr is the distance (3.0×107  m3.0 × 10^{7} \; \text{m}).

Step 2

Step 2: Rearrange the formula to find the mass of the planet

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Answer

Rearranging the formula gives: m2=Fr2Gm1m_2 = \frac{F r^2}{G m_1} Substituting in the known values:

  • F=1.6×107  NF = 1.6 × 10^{7} \; \text{N},
  • r=3.0×107  mr = 3.0 × 10^{7} \; \text{m},
  • G=6.674×1011  N m2/kg2G = 6.674 × 10^{-11} \; \text{N m}^2/\text{kg}^2,
  • m1=6.0×1030  kgm_1 = 6.0 × 10^{30} \; \text{kg}.

Step 3

Step 3: Calculate the mass of the planet

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Answer

Plugging in the values:

m2=(1.6×107)(3.0×107)2(6.674×1011)(6.0×1030)m_2 = \frac{(1.6 × 10^{7}) (3.0 × 10^{7})^2}{(6.674 × 10^{-11}) (6.0 × 10^{30})}

Calculating (3.0×107)2=9.0×1014  m2(3.0 × 10^{7})^2 = 9.0 × 10^{14} \; \text{m}^2, we have:

m2=(1.6×107)(9.0×1014)(6.674×1011)(6.0×1030)m_2 = \frac{(1.6 × 10^{7})(9.0 × 10^{14})}{(6.674 × 10^{-11})(6.0 × 10^{30})}

Carrying out the calculations, we ultimately find: m2=3.6×1010  kgm_2 = 3.6 × 10^{10} \; \text{kg} So, the answer is C. 3.6 × 10^{10} kg.

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