What is the SI unit of universal gravitational constant ?
- AOption (a)
- BOption (b)
- COption (c)
- DOption (d)
View answer & explanationHide answer & explanation
Correct answer
Why this answer is correct
The correct answer is Nm²/kg².
Key Points
- The Universal Gravitational Constant (G) is a physical constant involved in the calculation of gravitational effects in Sir Isaac Newton's Law of Universal Gravitation.
- According to the law, the gravitational force (F) between two bodies is directly proportional to the product of their masses (m1 and m2) and inversely proportional to the square of the distance (r) between them: F = G(m1m2/r²).
- To find the SI unit of G, we rearrange the formula: G = (F × r²) / (m1 × m2).
- In the SI system, the unit of force (F) is the Newton (N), the unit of distance (r) is the meter (m), and the unit of mass (m) is the kilogram (kg).
- Substituting these units into the rearranged formula gives: Newton × meter² / (kilogram × kilogram), which simplifies to Nm²/kg² (or Nm²kg⁻²). Hence, the correct option is Nm²/kg².
Additional Information
- Value of G: The accepted value of the Universal Gravitational Constant is approximately 6.674 × 10⁻¹¹ Nm²/kg². This value is extremely small, which explains why gravitational forces between everyday objects are not easily noticeable.
- Henry Cavendish: The first person to accurately measure the value of G in a laboratory setting was the English scientist Henry Cavendish in the year 1798 using a torsion balance experiment.
- Universal Nature: Unlike the acceleration due to gravity (g), G is a scalar quantity and is a universal constant. This means its value remains the same everywhere in the universe, regardless of the medium or the bodies involved.
- Dimensional Formula: The dimensional formula for the universal gravitational constant G is [M⁻¹ L³ T⁻²].
Important Points
- Difference between G and g: It is important to distinguish between G (Universal Gravitational Constant) and g (Acceleration due to gravity).
- G is constant throughout the universe, while g varies from place to place (e.g., g is approximately 9.8 m/s² on Earth but about 1.6 m/s² on the Moon).
- The relationship between them is given by the formula g = GM/R², where M is the mass of the celestial body and R is its radius.
- Newton's Principia: The concepts of universal gravitation were first published by Isaac Newton in his work Philosophiæ Naturalis Principia Mathematica in 1687.
- Weak Force: Gravity is considered the weakest of the four fundamental forces of nature (the others being electromagnetism, the strong nuclear force, and the weak nuclear force), yet it dominates the large-scale structure of the universe.