Two particles of the same mass m are moving in circular orbits because of force, given by
`F(r)=(-16)/(r)-r^(3)`
The first particle is at a distance r =1 , and the second, at r = 4. The best estimate for the ratio of kinetic energies of the first and the second particle is closet to :
Two particles of the same mass m are moving in circular orbits because of force, given by
`F(r)=(-16)/(r)-r^(3)`
The first particle is at a distance r =1 , and the second, at r = 4. The best estimate for the ratio of kinetic energies of the first and the second particle is closet to :
`F(r)=(-16)/(r)-r^(3)`
The first particle is at a distance r =1 , and the second, at r = 4. The best estimate for the ratio of kinetic energies of the first and the second particle is closet to :
A
`3xx10^(-3)`
B
`6xx10^(2)`
C
`10^(-1)`
D
`6xx10^(-2)`
Text Solution
AI Generated Solution
The correct Answer is:
To solve the problem, we need to find the ratio of the kinetic energies of two particles moving in circular orbits under the influence of a given force. The force is defined as:
\[ F(r) = -\frac{16}{r} - r^3 \]
### Step 1: Understand the relationship between force and centripetal motion
For a particle moving in a circular orbit, the centripetal force required to keep it in that orbit is provided by the net force acting on it. The centripetal force \( F_c \) is given by:
\[ F_c = \frac{mv^2}{r} \]
where \( m \) is the mass of the particle, \( v \) is its tangential velocity, and \( r \) is the radius of the circular orbit.
### Step 2: Set up the equation for each particle
We can equate the given force to the centripetal force for each particle:
\[ F(r) = \frac{mv^2}{r} \]
Thus, we have:
\[ -\frac{16}{r} - r^3 = \frac{mv^2}{r} \]
Multiplying through by \( r \) to eliminate the denominator gives:
\[ -16 - r^4 = mv^2 \]
So, we can express \( mv^2 \) as:
\[ mv^2 = -16 - r^4 \]
### Step 3: Calculate \( mv^2 \) for both particles
1. **For the first particle at \( r = 1 \)**:
\[
mv^2 = -16 - (1)^4 = -16 - 1 = -17
\]
2. **For the second particle at \( r = 4 \)**:
\[
mv^2 = -16 - (4)^4 = -16 - 256 = -272
\]
### Step 4: Calculate the kinetic energy for both particles
The kinetic energy \( K \) of a particle is given by:
\[ K = \frac{1}{2} mv^2 \]
1. **Kinetic energy of the first particle**:
\[
K_1 = \frac{1}{2} mv^2 = \frac{1}{2} (-17) = -\frac{17}{2}
\]
2. **Kinetic energy of the second particle**:
\[
K_2 = \frac{1}{2} mv^2 = \frac{1}{2} (-272) = -136
\]
### Step 5: Find the ratio of the kinetic energies
Now, we can find the ratio of the kinetic energies of the first particle to the second particle:
\[
\text{Ratio} = \frac{K_1}{K_2} = \frac{-\frac{17}{2}}{-136} = \frac{17}{2 \times 136} = \frac{17}{272}
\]
### Step 6: Simplify the ratio
Calculating the ratio:
\[
\frac{17}{272} = \frac{1}{16} = 0.0625
\]
### Step 7: Convert to scientific notation
\[
0.0625 = 6.25 \times 10^{-2}
\]
### Conclusion
The best estimate for the ratio of kinetic energies of the first and the second particle is closest to:
\[
\boxed{6 \times 10^{-2}}
\]
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