-
A.
\( M^{–1}L^3 T^{–2} \)
-
B.
ML3T2
-
C.
ML3
-
D.
MLT-2
Correct Answer: Option A
Explanation
f α (MM ÷g
2)
F(GMM ÷ r
2) [G – gravitational constant]
GMM = Fr
2
G = F0
2 ÷ MM = m × aπr
2 ÷ MM (f = ma)
= (m × m5
-2 × r
2) ÷ MM
= (Kg.m5
2 × m
2) ÷ Kg.Kg
=1 ÷ kg.m
3.5
2
The dimension mathematically representation have a quantities of M, L AND T
M (Mass) = kg, L (Length) = M, T (Time) second
G = kg
-1 m
2.5
2(Using dimension rule)
M
-1.L
3.T
-2
∴ The universal gravitational constant (G) =\( M^{–1}L^3 T^{–2} \)
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