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Re: Asteroid Problem (2)



Ahh, but we are told that tides are generated by the difference
between lunar and solar forces, so that the force equivalent to that of
the moon is generated by a satellite having 10^{-3} moon masses at a
distance (1/r_{moon})^{2} =10^{-3)/r^{2}, or
r = 10^{-3/2}r_{moon} = .03x60 earth radii or about 1.8 earth
radii.

Regards,
Jack
On Wed, 29 Aug 2001, brian whatcott wrote:

[Presentation in reverse time order...]

Hmmmm,
supposing the tidal force due to the Moon mass (Mm) at 60 earth r away
is proportional to the rate of change of Gravity force at the Earth
F = G.m1.m2.r^-2
i.e
Ftidal = -2.G.m1.m2.r^-3

and wishing the planetaid's close encounter to no more than equal this
tidal force, we have
-2G m1 m2 r^-3 = -2 G m1/1000 m2 x^-3
r^-3 = x^-3/1000
so x = 6 Earth radii for r = 60 Re

So Rick's estimate (4 Re) was evidently in the ball park.
Brian W


At 14:09 8/28/01 -0500, Jack Uretsky added helpfully:
Well, that's about 10^{-3} times the lunar mass, and the moon
is about 60 earth radii away. Does that help?
--
Franz Kafka...


On Tue, 28 Aug 2001, Ludwik Kowalski responded:

This begs for a question. How far should the m=10^19 kg
asteroid pass to avoid undesirable tides and earthquakes?
Ludwik Kowalski

Earlier, Rick Tarara wrote:

With the earth moving at 30 km/s along its orbital path,
15 minutes will move the earth 2 diameters [from the
trajectory of the asteroid].


--
Franz Kafka's novels and novella's are so Kafkaesque that one has to
wonder at the enormity of coincidence required to have produced a writer
named Kafka to write them.
Greg Nagan from "The Metamorphosis" in
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