Centripetal force exerted on Earth

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SUMMARY

The centripetal force exerted on Earth by the Sun is calculated using the formula F = MV²/R, where M is Earth's mass (6 × 1024 kg), V is the orbital velocity, and R is the average distance from the Sun (1.5 × 108 km). The correct calculation yields a centripetal force of 3.56775 × 1022 N, which was miscalculated as 3.56775 × 1019 N due to a unit conversion error from kilometers to meters. The period of revolution for Earth is 365.25 days, and the orbital velocity is approximately 29.86 m/s.

PREREQUISITES
  • Understanding of centripetal force calculations
  • Knowledge of unit conversions (km to m)
  • Familiarity with basic physics formulas (F = MV²/R)
  • Concept of orbital mechanics and Earth's revolution
NEXT STEPS
  • Review the derivation of centripetal force in circular motion
  • Learn about unit conversion techniques in physics
  • Study the implications of gravitational forces in orbital mechanics
  • Explore the impact of mass and distance on gravitational attraction
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Students of physics, educators teaching mechanics, and anyone interested in understanding the forces acting on celestial bodies.

electronicxco
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Here is the problem and the choices:
Calculate the centripetal force exerted on
the Earth by the Sun. Assume that the period
of revolution for the Earth is 365.25 days,
the average distance is 1.5 × 10^8 km and the
Earth’s mass is 6 × 10^24 kg.
The choices are:
1. 3.56775 × 10^22 N
2. 2.66331 × 10^32 N
3. 7.24562 × 10^22 N
4. 1.62932 × 10^21 N
5. None of these
6. 3.56775 × 10^19 N
7. 4.6238 × 10^29 N
8. 1.28439 × 10^26 N
9. 7.24562 × 10^20 N
__________________________________________________
Here is the attempted solution ( got choice # 6 but it is not correct)

2πr=D
(2)(π)(1.5 * 10^8) = 942477796.1 m=D

D = VT
V = D/T
V = (942477796.1) / ( 365.25 * 24 * 60 * 60)
V = 29.86 m/s


F = MV^2 / R
F = (6 * 10^24)(29.86)^2 / (1.5 * 10^8)
F = 3.56775 * 10^19
 
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electronicxco said:
Here is the problem and the choices:
Calculate the centripetal force exerted on
the Earth by the Sun. Assume that the period
of revolution for the Earth is 365.25 days,
the average distance is 1.5 × 10^8 km and the
Earth’s mass is 6 × 10^24 kg.
The choices are:
1. 3.56775 × 10^22 N
2. 2.66331 × 10^32 N
3. 7.24562 × 10^22 N
4. 1.62932 × 10^21 N
5. None of these
6. 3.56775 × 10^19 N
7. 4.6238 × 10^29 N
8. 1.28439 × 10^26 N
9. 7.24562 × 10^20 N
__________________________________________________
Here is the attempted solution ( got choice # 6 but it is not correct)

2πr=D
(2)(π)(1.5 * 10^8) = 942477796.1 m=D
that ditance is in km, not m
D = VT
V = D/T
V = (942477796.1) / ( 365.25 * 24 * 60 * 60)
V = 29.86 m/s


F = MV^2 / R
F = (6 * 10^24)(29.86)^2 / (1.5 * 10^8)
F = 3.56775 * 10^19
looks like your off by a factor of 1000. Simple units error.
 
wow..thanks for catching my mistake!
 

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