LANS
- 24
- 0
Note: this is one of the suggested practice problems for my second-year classical mechanics course.
Homework Statement
A spherical asteroid of mass m_{0} and radius R, initially moving at speed v_{0}, encounters a stationary cloud of dust. As the asteroid moves through the cloud, it collects all the dust that it hits, and slows down as a result. Ignore the increase in radius of the asteroid, and its gravitational effect on distant dust grains. Asume a uniform average density D (mass per unit volume) in the dust cloud.
a)show that \frac{dv}{dt} = -kv^{3} and evaluate k.
b) find v(t)
The attempt at a solution
Let A_{c} = 2*\pi*R be the cross-sectional area of the asteroid.
Conservation of momentum:
m_{0}v_{0} = m(t) v(t)
dm = (\pi R^2)*(v(t)dt)*D
dm is from mass of dust which the asteroid hits in time dt. Cross-sectional area * distance traveled in time dt * dust density.
I'm not sure where to go from here. Any help is greatly appreciated.
Thanks
Homework Statement
A spherical asteroid of mass m_{0} and radius R, initially moving at speed v_{0}, encounters a stationary cloud of dust. As the asteroid moves through the cloud, it collects all the dust that it hits, and slows down as a result. Ignore the increase in radius of the asteroid, and its gravitational effect on distant dust grains. Asume a uniform average density D (mass per unit volume) in the dust cloud.
a)show that \frac{dv}{dt} = -kv^{3} and evaluate k.
b) find v(t)
The attempt at a solution
Let A_{c} = 2*\pi*R be the cross-sectional area of the asteroid.
Conservation of momentum:
m_{0}v_{0} = m(t) v(t)
dm = (\pi R^2)*(v(t)dt)*D
dm is from mass of dust which the asteroid hits in time dt. Cross-sectional area * distance traveled in time dt * dust density.
I'm not sure where to go from here. Any help is greatly appreciated.
Thanks
Last edited: