How Large Can a Pulsar Be Before Its Surface Exceeds Light Speed?

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A pulsar emits light in bursts due to its rotation, with the Crab Nebula pulsar flashing at 30 times per second. The discussion revolves around calculating the maximum radius of a pulsar, ensuring no part of its surface exceeds the speed of light (3.00 x 10^8 m/s). Key to solving this is understanding the relationship between surface speed and angular velocity, expressed as v = ωr. Participants share hints and guidance, ultimately leading to a clearer understanding of the problem. The collaborative effort helps resolve the initial confusion regarding the calculations needed.
akane
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ok, here we go. I got this problem and i can't figure out how to solve it.

A pulsar is a celestial object that emits light in short bursts. A pulsar in the Crab Nebula flashes at a rate of 30 time/s. Suppose the light pulses are caused by the rotation of a spherical object that emits light from a pair of diametrically opposed "flashlights" on it equator. What is the maximum radius of the pulsar if no part of its surface can move faster than the speed of light
(3.00 x 10 to the 8th m/s)?

Thanks a lot! I appreciate your help-

Akane
 
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please help me...i really need to figure out how to do this
 
anyone?> i tried solving it myself but no luck
 
What have you tried?

Here are a few hints:

Since there are two light sources, what rotation rate must the object have? What angular velocity?
What's the relationship between surface speed and angular velocity?
 
i am sorry but i still don't understand this chapter. If you could give me some more hints i would really appreciate it
 
The relationship between the surface speed at the equator and the angular velocity \omega (which is measured in radians/sec) is v = \omega r.
 
thank you very much! it helped me figure out the problem. :cry: it was not that bad-
 
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