Question #50287

Two spherical bodies of mass M and 5M and radii R and 2R respectively are released in free space with initial separation between their centres eual to 12R. If they attract each other due to gravitational force only , then the distance covered by the smaller body just before collision is
(1)2.5R
(2)4.5R
(3)7.5R
(4)1.5R
1

Expert's answer

2015-01-06T12:34:15-0500

Answer on Question#50287 - Physics - Mechanics | Kinematics | Dynamics

(3) 7.5R

Solution


Keep in mind that xaxisx - axis actually passes through bodies' centers. Grading in units of RR .

V1V_{1} and V2V_{2} denote velocities.

Due to Newton's 3rd3^{\mathrm{rd}} law:


Md2x1dt2=5Md2x2dt2M \frac {d ^ {2} x _ {1}}{d t ^ {2}} = - 5 M \frac {d ^ {2} x _ {2}}{d t ^ {2}}


Thus,


d2x1dt2=5d2x2dt2\frac {d ^ {2} x _ {1}}{d t ^ {2}} = - 5 \frac {d ^ {2} x _ {2}}{d t ^ {2}}


, where x1x_{1} and x2x_{2} positions of the 1st1^{\text{st}} and the 2nd2^{\text{nd}} bodies respectively.

Let us integrate both part with respect to time tt .


d2x1dt2dt=5d2x2dt2dt\int \frac {d ^ {2} x _ {1}}{d t ^ {2}} d t = - 5 \int \frac {d ^ {2} x _ {2}}{d t ^ {2}} d tdx1dt=V1(t);dx2dt=V2(t);\frac {d x _ {1}}{d t} = V _ {1} (t); \frac {d x _ {2}}{d t} = V _ {2} (t);dV1dtdt=5dV2dtdt\int \frac {d V _ {1}}{d t} d t = - 5 \int \frac {d V _ {2}}{d t} d tV1+C1=5V2+C2V _ {1} + C _ {1} = - 5 V _ {2} + C _ {2}


, where C1C_1 and C2C_2 - constants of integration.

At initial moment of time (t=0)(t = 0) both velocities equal to zero, hence C1=C2=0C_1 = C_2 = 0 .


V1=5V2V _ {1} = - 5 V _ {2}


Integrate with respect to time once more. Definite integral now. τ\tau - time at which collision happens.


0τV1dt=50τV2dt\int_{0}^{\tau} V_{1} dt = -5 \int_{0}^{\tau} V_{2} dt0τdx1dtdt=50τdx2dtdt\int_{0}^{\tau} \frac{dx_{1}}{dt} dt = -5 \int_{0}^{\tau} \frac{dx_{2}}{dt} dtx1(τ)x1(0)=5(x2(τ)x2(0))x_{1}(\tau) - x_{1}(0) = -5 \left(x_{2}(\tau) - x_{2}(0)\right)


Recall, that due to our choice: x1(0)=0x_{1}(0) = 0; x2(0)=12x_{2}(0) = 12;


x1(τ)0=5(x2(τ)12)x_{1}(\tau) - 0 = -5 (x_{2}(\tau) - 12)x1(τ)=605x2(τ)x_{1}(\tau) = 60 - 5 x_{2}(\tau)


Also, we know that minimal distance between spheres is nothing else, but the sum of its radii.

It means in our case: x2(τ)x1(τ)=1+2=3x_{2}(\tau) - x_{1}(\tau) = 1 + 2 = 3.

Thus, we can substitute x2(τ)=3+x1(τ)x_{2}(\tau) = 3 + x_{1}(\tau) into main equation above.


x1(τ)=605(3+x1(τ))x_{1}(\tau) = 60 - 5 \left(3 + x_{1}(\tau)\right)x1(τ)=60155x1(τ)x_{1}(\tau) = 60 - 15 - 5 x_{1}(\tau)6x1(τ)=456 x_{1}(\tau) = 45x1(τ)=7.5x_{1}(\tau) = 7.5


Recall that we get result in units of RR.

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