Displacement Gravity: Dark Matter

Unit 3

Displacement Gravity: Dark Matter

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Physics says that dark matter makes up approximately 27% of the universe’s total mass-energy content—far exceeding the ordinary matter that comprises stars, planets, and everything we can see.

Dark matter is the aether or space particles that are beyond a solar system.

On a galactic level, these are displaced by a galaxy’s vortex which is made up of large timespace particles, as aethereal information.

Examples of Dark Matter

  1. Galaxy Rotation Curves

Stars at the edges of spiral galaxies orbit just as quickly as those near the center, contrary to what Newtonian physics predicts based on visible matter alone.

  1. Gravitational Lensing

When light from distant objects passes near massive structures like galaxy clusters, it bends due to gravity. The amount of bending observed often exceeds what visible matter can account for, indicating substantial amounts of aether.

  1. The Bullet Cluster

This famous collision of two galaxy clusters provides some of the strongest evidence for the aether that opposes matter.

During the collision, hot gas (visible matter) slowed down due to friction, while the gravitational mass continued moving ahead, demonstrating that most of the mass is separate from ordinary matter.

  1. Cosmic Microwave Background

Patterns in the CMB reveal how matter was distributed in the early universe.

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