THE MOST IMPORTANT THING EINSTEIN HAD FAILED

When taking observe for finding the angle of bending of star light in the sky, knowing the altitude of star is just as important as measuring the time of moving celestial bodies. We must know the altitude of star quite exactly if observations are to be of any use. The reason for this is that the angle calculations all depend on the altitude of star.

WHY DIDN'T THEY KNOW NONSENSE?

 Prediction at 2017 solar eclipse, August 21, in USA

The first calculation of the deflection of light by mass was published by the German astronomer Johann Georg von Soldner in 1801. Soldner showed that rays from a distant star skimming the Sun’s surface would be deflected through an angle of about 0.9 seconds of arc, or one quarter of a thousandth of a degree. This angle corresponds to the apparent diameter of a compact disc (CD) viewed from a distance of about 30 kilometers (nearly 20 miles). Soldner’s calculations were based on Newton’s laws of motion and gravitation, and the assumption that light behaves like very fast moving particles. As far as we know, neither Soldner nor later astronomers attempted to verify this prediction, and for good reason: Such an attempt would have been far beyond the capability of early 19th century astronomical instruments.
Light deflection in general relativity. Over a century later, in the early 20th century, Einstein developed his theory of general relativity. Einstein calculated that the deflection predicted by his theory would be twice the Newtonian value.The following image shows the deflection of light rays that pass close to a spherical mass. To make the effect visible, this mass was chosen to have the same value as the Sun’s but to have a diameter five thousand times smaller (i.e., a density 125 billion times larger) than the Sun’s.(www.einstein-online.info).

2017 SOLAR ECLIPSE PROVES EINSTEIN WRONG

".. for the stars observed being the closest to the Sun, their deviation was about 1.75 seconds of an arc." (Albert Einstein)

“….during totality on August 21, 2017 — although it will be close to midday — you’ll easily be able to see 4 planets with the unaided eye near the eclipsed sun!

In order of brightness, these planets will be Venus, Jupiter, Mars and Mercury. Mars is slightly brighter than Mercury, but so nearly the same in brightness that you probably won’t notice a difference.”(See 4 planets during 2017 solar eclipse).

At the 2017 solar eclipse, Monday, August 21, in USA, the bright star Regulus make a thrilling sight shinning near the Sun’s corona, this event is the best chance to test or re-examine Einstein’s general theory of relativity.