radiation pressure

Radiation pressure from the hot young stars will eventually drive most of the gas away.

Eventually the radiation pressure will be greater than the weight of the atmosphere above him.

In the final stages, that implies movement against radiation pressure.

His star is too cool for radiation pressure to be much of a factor in its stability.

This means that the change in frequency of the light is equal to the work done on the wall by the radiation pressure.

The effects of the solar wind and radiation pressure are similar, but directed away from the Sun.

In the Sun, radiation pressure is still quite small when compared to the gas pressure.

This is referred to as a radiation pressure force.

Finally, other forces such as radiation pressure and collisions also result in drifts.

This is the principle behind the solar sail, which uses light radiation pressure to move through space.

For certain types of spacecraft the use of radiation pressure certainly makes both physical and economic sense.

The envelope will expand further, seeking a new balance between gravity and radiation pressure.

Based on this, he argued that the collapse must be slowed to a near halt by radiation pressure.

Otherwise, radiation pressure would disperse the cloud in a matter of weeks."

The radiation pressure from a focused laser beam is able to trap small particles.

"Check the radiation pressure on your aft shields," Spock said.

See also Over time, radiation pressure from the cluster will disperse the molecular cloud.

The force ejecting the gas at the high velocities observed is radiation pressure.

The radiation pressure then slowly rockets the pulsar away.

He knows that some very hot stars exist on the verge of being blown apart because of radiation pressure.

He was the first to take account of the influence of radiation pressure on stellar equilibrium.

This implies that the sodium atoms are driven away from the comet's head by radiation pressure.

One may distinguish between the cases of small and large stellar masses by deriving the above results using radiation pressure.

The gradual restoration to normal brightness results from the dust being dispersed by radiation pressure.

These solid fragments of matter, are then injected into the interstellar medium by radiation pressure.