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Marketing hype aside, which also would have been nice, just a simple stationary view up of the rocket getting smaller and smaller would have been GREAT if not for the cloud cover.
But then again it *was* Christmas so I channeled my inner Ralphie as they switched to the animations.
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thanks for sharing.This is a great read and brings back memories of advanced physics classes in college …
Very innovative solution to maintaining a stable orbital position without having to burn lots of fuel. They sent @JamesW up there with a good amount of canned beans with which to do course corrections but even his ability to supply the fuel for those burns will be limited … the bean & cheese burritos are for “emergency burns” only ….
He has legit been gone since Christams Eve. Could it really be JamesW(ebb) ?Goodbye @JamesW … it was nice knowing you![]()
He has legit been gone since Christams Eve. Could it really be JamesW(ebb) ?
Same issue with LIGO.They are literally attempting to reduce the vibrations of the ATOMS that make up the materials inside the detector so that their images are as perfect as possible
The change in distance between LIGO's mirrors when a gravitational wave passes is on the order of 10-19 m.
The suspensions then take over, reducing this noise level nearly a million times more to help achieve LIGO's desired detection sensitivity of 10-19 m (the amount which gravitational waves expand and contract spacetime between the test masses).
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Vibration Isolation
The Laser Interferometer Gravitational-Wave Observatory (LIGO) consists of two widely separated installations within the United States — one in Hanford Washington and the other in Livingston, Louisiana — operated in unison as a single observatory. LIGO is operated by the LIGO Laboratory, a...www.ligo.caltech.edu
Same issue with LIGO.
The change in distance between LIGO's mirrors when a gravitational wave passes is on the order of 10-19 m.
Or not.so much detail to look out! Astronomers will be at this for decades.