Dark Matter
Our galaxy, the Milky Way, and other galaxies contain more matter than
expected from visual observations. This so called "dark matter"
is detected by the rapid rotation of matter in the outer regions of galaxies
as well as the motion of the galaxies within galactic clusters. The
gravity exerted by the dark matter holds the galaxies and clusters together
and allows faster rotations than would be possible if it did not exist.
It is estimated that 70% to 90% of the mass which should exist according
to the laws of gravity cannot be seen in visible light images of the galaxies.
Candidates for the dark matter include:
But when all the estimates of the masses of these different classes of
objects is joined together it still does not provide enough mass to explain
the gravitational effects observed in galaxies and clusters of galaxies.
Physicists have invented several possible catagories for the remaining
missing dark matter:
A variety of observational methods may be used to detect and differentiate
between the various dark matter candidates. These include:
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Neutrino Detectors
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Superkamiokande,
Kamioka-cho, Yoshiki-gun, Gifu-ken, Japan, 1,000 m underground.
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The Sudbury Neutrino Observatory
(SNO), Sudbury, Ontario, Canada, 2072 m underground.
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Gallex, Abruzzo
region of Italy, in the Gran Sasso Tunnel, ~1400 m underground.
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UK Dark Matter Calaboration,
Cleveland, UK, 1100 m underground.
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HOMESTAKE, Homestake mine, South Dakota, ~1478 m underground.
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See also: The Ultimate Neutrino
Page; Neutrion
Detection Experiments; Neutrion
Oscillation Industry ; History
of the Neutrinos and Neutrino Detectors
& Beams
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Gravity Wave Detectors
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X-ray Observatories
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Infrared Telescopes
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Dark Matter Searches
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Gravitational Microlensing
Studies
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Conferences:
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Microlensing 2000, 21-25 February
2000, Cape Town, South Africa
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4th International
Workshop on Gravitational Microlensing Surveys, 15-17 January 1998,
Paris, France
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3rd International
Workshop on Gravitational Microlensing Surveys, 6-8 March 1997, Notre
Dame, Indiana, USA
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2nd
International Workshop on Gravitational Microlensing Surveys, 29-31
January 1996, Orsay, France
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IAU Symposium 173, Astrophysical Applications of Gravitational Microlensing,
9-14 July 1995, Melbourne, Australia
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Telescopes:
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The Galactic Exoplanet Survey Telescope (GEST): A Proposed Space-Based
Microlensing Survey for Terrestrial Extra-Solar Planets (astro-ph/0003102).
Proposes to survey 108 stars to discover 1300-5000 planets over
a 2.5 year mission, including potentially 100 planets of ~ Earth mass.
Missing Mass Pages
Dark Matter Pages
MACHO Pages
WIMP Pages
superWIMP Pages
Gravitational Microlensing Pages
Brown Dwarf Pages
Red Dwarf Pages
White Dwarf Pages
Neutron Star Pages
Black Hole Pages
Neutrino Experiments
Interstellar Gas Clouds
Gravity Wave Detectors
Related Pages
Stellar Evolution
Observatories and Sky Surveys
Globular Cluster Distance & Ages
Astronomy Index
Created: February, 1998
Last Modified: July 9, 2003
HTML Editor: Robert Bradbury