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Antigravity Matter

Interstellar and intergalactic space contains a thin atmosphere of antigravity matter

 

Antigravity matter has many effects within the universe including:-

·        Dark matter (and MOND).  These gravitational effects are caused by a local reduction in the density of antigravity matter, not by a presence of dark matter.

·        The densities of Bok globules, elliptical galaxies and globular clusters.

·        The shapes of galaxies - discs, cores, bars, spirals and reverse spirals, globular clusters, molecular clouds, elliptical galaxies and star forming regions.

·        Pulsar kicks and the behaviour of supernova remnants.

 

 

Antigravity matter cannot be observed directly and the closest significant density of antigravity matter is well away from the earth.  The Evidence page contains a list of observations that are indirect effects of antigravity matter.  To understand how these observations are evidence the reader is encouraged to first read the Behaviour page.

 Try these videos that form an Antigravity Matter Overview Course

 

AGM 000 - Why do we need Antigravity Matter?

AGM 001 - Basics

AGM 002 - Elliptical Galaxies and Galaxy Clusters

AGM 003 - AGM Drag and Bok Globules

AGM 004 - Supernovae and Remnants

AGM 005 - Spiral Galaxies (1 of 3)

AGM 006 - Spiral Galaxies (2 of 3)

AGM 007 - Spiral Galaxies (3 of 3)

AGM 008 - Globular Clusters

AGM 009 - The Galaxy Lifecycle

AGM 010 - The Milky Way

AGM 011 - The Large Scale AGM Exclusion Density

Other Videos:-

AGM and NGC 1277

Does the Milky Way have an Antihalo?

 

The latest paper is available at Antigravity_Matter.pdf

 

Email to:- timesimmons@blueyonder.co.uk

© Copyright Tim E Simmons 2006 to 2024.

Originally published in February 2006 at www.preston.u-net.com/AGMatter/Index.htm

Last updated 17th February 2024.  Major changes are logged in AGM Change Log.