Dale
As an example of what Brent just wrote, if you go to Patrick's web site http://planet.state.ut.us and scroll down to International Space Station Data and the select Salt Lake City you will see that the Space Station like the Shuttle comes over Utah on different orbits.
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Thr Feb 06/07:44 PM |
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10 above NNW | 13 above NNW |
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Fri Feb 07/06:46 PM |
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10 above NNW | 11 above NE |
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Sat Feb 08/07:23 PM |
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11 above NNW | 22 above N |
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Sun Feb 09/06:25 PM |
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10 above NNW | 10 above ENE |
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Mon Feb 10/07:03 PM |
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10 above NW | 30 above ENE |
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Tue Feb 11/07:45 PM |
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39 above W | 51 above SW |
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Wed Feb 12/06:49 PM |
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23 above NW | 13 above ESE |
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Thr Feb 13/07:32 PM |
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23 above SW | 10 above S |
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Fri Feb 14/06:37 PM |
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49 above SW | 11 above SE |
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Which, by the way, the space station will be visible tonight for 5 minutes.
Jim
Brent Watson <brentjwatson@yahoo.com> wrote:
I don't think the re-entry path was atypical. The
shuttle has passed over s. Utah several times for
landing at Kennedy. This was the second time I have
seen it, and I believe Patrick has seen it three times
now. (Patrick?) The path is whatever it is depending
on where in the earth/orbit relation the orbiter is
when it de-orbits. I have looked at many re-entry
tracks, and they are not the same.
Brent
--- Dale Hooperwrote:
> There is something that I have been really curious
> about that I haven't seen mentioned (please forgive
> me if I somehow just missed it). We know that the
> shuttle was following an atypical reentry track -
> because we were able to observe it over southern
> Utah. I'm wondering if this reentry profile
> presents times when there are greater stresses on
> the orbiter than a typical reentry profile? I.e.,
> more severe banking that might overly stress an
> already somewhat damaged wing; which wouldn't have
> caused a failure in a more typical reentry profile.
>
> Certainly, this wouldn't be a root cause - but might
> be a contributing factor. Obviously, I've entered
> into second tier speculation.
>
>
> _______________________________________________
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> Utah-Astronomy@mailman.xmission.com
>
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