Dick Foster
Platinum Member
I thought it was settled science once the fact that light bends around a mass was proved by observations made during a total solar eclipse. For this reason we could not run sight lines in close proximity to massive structures or other large masses for precise 1st order geodetic surveys.
I'm not disputing that you were told not to do that, but it must have been for some other reason. Gravitational bending is insignificant for a mass smaller than a star. As an example, light skimming past the surface of the earth would be gravitationally bent by a total of 0.0006 arc-seconds. That would correspond to 3 inches deflection over 10,000 miles. Such gravitational bending is insignificant compared to distortion from the atmosphere, which may have been what you were trying to avoid.
I know that and you know that but try and tell that to a PHd geodesist sometime.
Atmospheric distortion is why most of our observations were done in the wee hours sometimes when it was as cold as a witches titty and a ballpoint pen would even freeze up. Yeah we had to do everything in ink, no cheating. We had to do a lot of crazy stuff.