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Latest June Mission Update from the GP-B team.
Nothing new to report on the results.
1. GP-B SUCCEEDED IN COLLECTING THE DATA TO TEST EINSTEIN'S PREDICTIONS ABOUT GRAVITY
2. THE EFFECTS OF GENERAL RELATIVITY ARE CLEARLY VISIBLE
3. FIRST PEEK AT RESULTS PRESENTED AT APRIL APS MEETING; FINAL RESULTS IN DECEMBER
(geodetic precession = GR to 1% - however present estimate ("hint") of result ~30 mas too high but error is still ~100 mas)
4. THE TWO SURPRISES & THEIR IMPACT ON THE EXPERIMENT
5. NEXT STEPS-MOVING TOWARDS A FINAL RESULT
i. Fine calibration of the gyroscope/telescope scale factor
ii. Refining the analysis of the misalignment torques
iii. Extremely precise VLBI measurement data will be substituted for the current 1997 Hipparcos [star] Catalogue values for the proper motion of IM Pegasi.
We continue to wait and see!
Garth
Nothing new to report on the results.
This GP-B update is essentially a revised and expanded version of the GP-B press release that we posted in April that tells a more readable and complete story about the goals of GP-B, what we've accomplished to date, the surprises we've encountered and how we're addressing them, and the steps we are taking towards a final results announcement at the end of the year.
1. GP-B SUCCEEDED IN COLLECTING THE DATA TO TEST EINSTEIN'S PREDICTIONS ABOUT GRAVITY
2. THE EFFECTS OF GENERAL RELATIVITY ARE CLEARLY VISIBLE
3. FIRST PEEK AT RESULTS PRESENTED AT APRIL APS MEETING; FINAL RESULTS IN DECEMBER
(geodetic precession = GR to 1% - however present estimate ("hint") of result ~30 mas too high but error is still ~100 mas)
4. THE TWO SURPRISES & THEIR IMPACT ON THE EXPERIMENT
(Italics my text)i. Shortly after the gyros were spun up in August 2004, we discovered that the polhode motion of the gyro rotors, which was expected to exhibit a constant pattern throughout the experimental period, was changing over time, significantly complicating the calibration of the gyroscope readout angles.
ii. During the post-experiment instrument calibration testing in August-September 2005, the spin axes of the gyroscopes were found to be affected by certain class of small classical torques, known as "misalignment torques," whose effects must be rigorously separated from the relativity measurements. (Due to electrostatic patches on the rotors and their housing.)
5. NEXT STEPS-MOVING TOWARDS A FINAL RESULT
i. Fine calibration of the gyroscope/telescope scale factor
ii. Refining the analysis of the misalignment torques
iii. Extremely precise VLBI measurement data will be substituted for the current 1997 Hipparcos [star] Catalogue values for the proper motion of IM Pegasi.
We continue to wait and see!
Garth
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