Related Formula
By Dimensional Analysis or Scaling of Kepler's Third Law:
T ∝ m^x G^y a^z$$T \propto m^x G^y a^z$$
Core Logic
Let's perform a dimensional matching to express the collision time T$T$ in terms of physical scaling variables m$m$, G$G$, and a$a$:
[T] = [M]^x [M⁻¹L³T⁻²]^y [L]^z$$[T] = [M]^x [M^{-1}L^3T^{-2}]^y [L]^z$$
Equating dimensions on both sides:
- Mass (M$M$): x - y = 0 x = y$x - y = 0 \implies x = y$
- Length (L$L$): 3y + z = 0 z = -3y$3y + z = 0 \implies z = -3y$
- Time (T$T$): -2y = 1 y = -1/2$-2y = 1 \implies y = -1/2$
Solving these equations:
x = -1/2, y = -1/2, z = 3/2$$x = -1/2, \quad y = -1/2, \quad z = 3/2$$
Step 1: Scaling Formula of Time
Therefore, the scaling relationship for time T$T$ is:
T ∝ m-1/2 G-1/2 a3/2 T ∝ √((a³)/(m))$$T \propto m^{-1/2} G^{-1/2} a^{3/2} \implies T \propto \sqrt{\frac{a^3}{m}}$$
Let's write the ratio for two cases:
(T₂)/(T₁) = √(((a₂)/(a₁))³ · ((m₁)/(m₂)))$$\frac{T_2}{T_1} = \sqrt{\left(\frac{a_2}{a_1}\right)^3 \cdot \left(\frac{m_1}{m_2}\right)}$$
Step 2: Calculating Final Time
Given values:
- a₁ = a$a_1 = a$, a₂ = 2a$a_2 = 2a$
- m₁ = m$m_1 = m$, m₂ = 2m$m_2 = 2m$
- T₁ = 4~s$T_1 = 4\mathrm{~s}$
(T₂)/(4) = √(((2a)/(a))³ · ((m)/(2m))) = √(2³ · (1)/(2)) = √(4) = 2$$\frac{T_2}{4} = \sqrt{\left(\frac{2a}{a}\right)^3 \cdot \left(\frac{m}{2m}\right)} = \sqrt{2^3 \cdot \frac{1}{2}} = \sqrt{4} = 2$$
T₂ = 4 × 2 = 8~seconds$$T_2 = 4 \times 2 = 8\mathrm{~seconds}$$
Pattern Recognition
Kepler's Third Law / free-fall collapse scaling: whenever a orbit or a direct gravitational collapse scale is involved, the time scales as T ∝ √((R³)/(GM))$T \propto \sqrt{\frac{R^3}{GM}}$. Thus doubling R$R$ multiplies time by √(8)$\sqrt{8}$ and doubling M$M$ divides time by √(2)$\sqrt{2}$. The combination results in a clean doubling of time: √(8)/√(2) = 2$\sqrt{8}/\sqrt{2} = 2$.
Chapter Mix
Class 11 Physics: Gravitation
Class 11 Physics: Units and Measurements: Dimensional Analysis