- 3,580
- 107
Polestar101 said:But even attempting to use the diurnal and annual aberrations as the main calibration tools shows the experimenters did not plan on accounting for any solar system motion relative to the guide star – meaning they essentially used a static solar system model.
The guide star IM Pegasi, chosen because it was also a radio star that could be tracked by the VLBI radio facility, was itself referenced to a distant quasar 3C454.3, which is at a distance of 12 billion light-years.
As the measurements were angular in nature the quasar's Proper Motion across the sky is negligible (see my post 323) and the solar system is therefore effectively 'static' relative to this distant reference point (see my post 329).
The suitability of quasar 3C454.3 as a stable reference point was itself carefully examined as you can see here: The “Core” of the Quasar 3C 454.3 as the Extragalactic Reference for the Proper Motion of the Gravity Probe B Guide Star, its conclusion:
The core of 3C 454.3 provides a sufficiently stable reference with which to measure the proper motion of the Gravity Probe B guide star, IM Pegasi, relative to the distant universe.
I hope this helps,
Garth
Last edited: