29:51 Are my eyes betraying me or is that the dopest 2-graviton function since the nineteen ninety eight when the Undertaker threw Mankind off Hеll in a Cell, and plummeted sixteen feet through an announcer's table?
@SoloNoobKingАй бұрын
Im only 13 years old and i already mastered math
@shawns0762Ай бұрын
Relativistic dilation explains dark matter/galaxy rotation curves. Mass that is dilated is smeared through spacetime relative to an outside observer. It's what our high school teachers were talking about when they said "mass becomes infinite at the speed of light". Time dilation is just one aspect of dilation. A graph illustrates its squared nature, it increases at an exponential rate the closer you get to the speed of light. It occurs wherever there is an astronomical quantity of mass. This includes the centers of very high mass stars and the overwhelming majority of galaxy centers. The mass at the center of our own galaxy is dilated. This means that there is no valid XYZ coordinate we can attribute to it, you can't point your finger at something that is smeared through spacetime. In other words that mass is all around us. It exists in a "non local" state from the vantage point of an Earthbound observer. Dilation does not occur in galaxies with low mass centers because they do not have enough mass to achieve relativistic velocities. It has been confirmed in 6 ultra diffuse galaxies including NGC 1052-DF2 and DF4 to have no dark matter, in other words they have normal rotation rates.
@friendlyone2706Ай бұрын
It is the anomalous that truly tests our understanding of reality. When doing experiments, it is the unexplained experimental errors that should grab our attention. In some ways, those few galaxies with "normal rotation rates" should be getting a lot more attention --- they are 2024's astronomy's "experimental errors".
@shawns0762Ай бұрын
@friendlyone2706 It can be inferred mathematically that dilation is not occurring in those galaxies. All galaxies with low mass centers have normal/near normal rotation rates.