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In the distant future, a 5.40xx10^(5)-kg...

In the distant future, a `5.40xx10^(5)-kg` intergalactic ship leaves Earth orbit and accelerates to a constant speed of 0.92c. Determine the difference, `p-p_(0)`, between the relativistic and classical momenta of the ship.

A

`3.9xx10^(14)kg*m//s`

B

`8.0xx10^(13)kg*m//s`

C

`2.3xx10^(14)kg*m//s`

D

`5.8xx10^(13)kg*m//s`

Text Solution

AI Generated Solution

The correct Answer is:
To determine the difference between the relativistic momentum \( p \) and the classical momentum \( p_0 \) of the intergalactic ship, we will follow these steps: ### Step 1: Calculate Classical Momentum \( p_0 \) The classical momentum \( p_0 \) is given by the formula: \[ p_0 = m_0 v \] where: - \( m_0 = 5.4 \times 10^5 \, \text{kg} \) (rest mass of the ship) - \( v = 0.92c \) (velocity of the ship, where \( c \) is the speed of light) Substituting the values: \[ p_0 = (5.4 \times 10^5 \, \text{kg}) \times (0.92 \times c) \] Using \( c \approx 3 \times 10^8 \, \text{m/s} \): \[ p_0 = (5.4 \times 10^5) \times (0.92 \times 3 \times 10^8) \] Calculating this gives: \[ p_0 = (5.4 \times 10^5) \times (2.76 \times 10^8) = 1.4904 \times 10^{14} \, \text{kg m/s} \] ### Step 2: Calculate Relativistic Momentum \( p \) The relativistic momentum \( p \) is given by the formula: \[ p = \frac{m_0 v}{\sqrt{1 - \frac{v^2}{c^2}}} \] First, we need to calculate \( \sqrt{1 - \frac{v^2}{c^2}} \): \[ \frac{v^2}{c^2} = (0.92)^2 = 0.8464 \] Thus, \[ 1 - \frac{v^2}{c^2} = 1 - 0.8464 = 0.1536 \] Now, taking the square root: \[ \sqrt{1 - \frac{v^2}{c^2}} = \sqrt{0.1536} \approx 0.39 \] Now substituting this back into the relativistic momentum formula: \[ p = \frac{(5.4 \times 10^5) \times (0.92 \times c)}{\sqrt{0.1536}} = \frac{(5.4 \times 10^5) \times (2.76 \times 10^8)}{0.39} \] Calculating this gives: \[ p \approx \frac{1.4904 \times 10^{14}}{0.39} \approx 3.8205 \times 10^{14} \, \text{kg m/s} \] ### Step 3: Calculate the Difference \( p - p_0 \) Now we can find the difference between the relativistic momentum and the classical momentum: \[ p - p_0 = 3.8205 \times 10^{14} - 1.4904 \times 10^{14} \] Calculating this gives: \[ p - p_0 \approx 2.3301 \times 10^{14} \, \text{kg m/s} \] ### Final Answer The difference between the relativistic and classical momenta of the ship is approximately: \[ \boxed{2.33 \times 10^{14} \, \text{kg m/s}} \]
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