Dark Matter Project Overview
Dark matter is currently
estimated to make up approximately 90% of the universe's total mass (Rubin
73). There presently exist two distinct theoretical candidates to
explain the presence of dark matter: massive dark bodies, ordinary matter
that does not emit light, or minute particles present throughout the universe.
Massive bodies could be brown dwarfs, black holes, neutron stars or gasses
and dust (Rubin 106). The minute particle most likely to account
for dark matter is the neutrino, which is said to be nearly weightless
and extremely abundant (Hawley 389-393).
Long ago, Aristotle held the belief that
an invisible force propelled objects through space (Hawley 26). This
belief held sway until it was gradually replaced with the more modern notion
of inertia. Concepts of invisible forces have played important roles throughout
the history of scientific understanding of the cosmos. Our plan is
to study Greek notions of invisible force that affects observable reality.
For the observation aspect of this project,
we will select a galaxy to observe through the 8" Orion telescope from
Lab Stores and determine the basic shape of that galaxy. We will
then gather data from scientific sources on the velocities of rotating
bodies within that galaxy relative to their distance from the apparent
center. This data will be applied to Kepler's third law, p2=r3
where p is the length of time a complete orbit takes to make around its
foci and r is the size of the semi-major axis of the orbit. We will
then compare this data with similar data on our own solar system.
The presence of extra gravitational force, in the form of dark matter,
can be confirmed or denied by using Kepler's third law to predict the periods
of orbit relative to the semi-major axis.
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