Planets in "Snow Globe Theory"In "snow globe theory", the Poincare-Einstein principle of relativity states:According to Einstein, planets move faster around the central star due to relativity. But since time is dilated, shouldn't they move slower? As with STR, a section (interval) of the time measured by the observer is smaller locally.* The cone of view narrows. The planet is actually closer to the star. Does Newton's inverse square law apply? One mass has gravity a. Two masses have gravity 2a + ghost mass. . In "snow globe theory", it is always necessary to consider the scale at which a system is viewed. If the planet is viewed from a greater distance, it is assigned a numerically smaller distance than it has locally, since its gravity is measured to be weaker there. Einstein finds a greater gravity. However, based on the above considerations: Newton's law of gravity applies locally.*** The event horizon, with Newtonian acceleration, results in Rh=M•G/c². However, this can only be measured locally. Seen from the outside, it appears much larger. A mass falling into the hole, as well as the central mass, is m*(1+Rh/r) = 2m. The ghost mass of the central mass acts like a baryonic mass. And with the narrowing of the cone of view, the radius of a black hole, seen from the outside, increases to more than 2•Rh, known as the Schwarzschild radius. *Proper time, twin paradox **A fixed length, measured on a larger scale, is numerically smaller. ***With the local scales and the universal constants of nature. However, the ghost mass of the central star changes its presumed mass with the distance of an observer. These properties don't seem to be of much use, as they only apply to a spherical shell—except for two: 1.) The hollow sphere principle only applies to Newtonian gravity (K/R²). 2.) Gravitational collapse is impossible. Ludwig Resch |