Welcome
In astronomy, dark matter is a form of matter that is undetectable, but whose presence can be inferred from effects on visible matter. According to present observations of structures larger then galaxies, as well as Big Bang cosmology, dark matter could account for the vast majority of the mass in the observable universe. Dark Matter is believed to play a central role in structure formation and galaxy evolution, and has measurable effects on the anisotropy of the cosmic microwave background. All these lines of evidence suggest that galaxies, clusters of galaxies, and the universe as a whole contain far more matter than that which interacts with electromagnetic radiation: the remainder is frequently called the "dark matter component:. The largest part of dark matter, which does not interact with electromagnetic radiation, is not only "dark" but also, by definition, utterly transparent.
In Development
Dark Matter films has a few projects being investigated, however we are always looking for new scripts, if you have a screenplay you would like us to review please contact us.
Casting Call
If you are in the Mid-Atlantic area and would like to find out about working with us please use the contact form above.
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