MadSci Network: Astronomy |
If a planet rotates at its critical speed, or escape velocity, the centrifugal force will balance the gravitational force. For Earth, the critical speed is slightly greater than 11 km per second. Earth rotates at about 0.5 km per second; planets which rotate at less than about one-tenth of their critical speed can retain atmospheres for billions of years. If a planet were rotating at critical speed, it would lose its atmosphere eventually. Still, this does NOT mean that the solid planet would break up. Solids are held together by electomagnetic forces, in addition to their gravity. Tidal forces wouldn't directly affect a planet rotating at critical speed, as long as the planet were roughly spherical and its crust and core roughly evenly layered. The electromagnetic force is almost forty orders of magnitude stronger than gravity. We see examples in our own solar system, of this general principle at work. The planet Saturn is quite oblate - that is, its equatorial diameter is considerably larger than its polar diameter - due to its relatively rapid rotation. Faster rotating planets would have equatorial bulges which would gradually break away and form gaseous disks and rings. An astronaut on the surface of a planet gradually increasing in its speed of rotation would feel lighter and lighter. As the rotation passed the critical mark, she would no longer be able to stand on the surface, and would begin to float away. Landing a spaceship on such a planet would therefore be difficult. The spaceship could fire its rockets away from the surface to propel it downward, and could implant long arms into the surface which would resist shears and strains caused by the rotation of the planet. In the real universe, planets like this would not likely form, nor become supercritically rotating. A collision with another massive body might pass enough angular momentum to a planet to make it rotate supercritically, but such a collision would probably shatter the planet as well!
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