Not exact matches
The most plausible answer was the galaxies also contained
clouds of what they dubbed «
dark matter» that could not be seen
by conventional means, but which exerts a gravitational tug.
By measuring the velocity of the gas and its distance from the
dark cloud where it originated, estimating its age was a simple
matter.
The case for
dark matter began in the 1930s with a pair of papers
by two very different kinds of geniuses, the buttoned - down Dutch astronomer Jan Oort (who also hypothesized the Oort
Cloud of comets) and the explosive Swiss - American cosmologist Fritz Zwicky.
Perhaps just as incredible, the
clouds of hot interstellar gas formerly contained
by the galaxies — and superheated
by the collision so they glow in x-ray light — seem to have been grabbed
by the
dark matter instead of being flung into space.
Observations of the orbits of stars around galaxies suggest that all galaxies, including the Milky Way, are surrounded
by a spherical
cloud of
dark matter (see diagram).
The Milky Way (like other spiral galaxies) is surrounded
by a large halo region which contains globular clusters, large
clouds of hydrogen gas, and a huge mass of the mysterious
dark matter.
Some are found in globular clusters, but most move in a huge
cloud around the disk called the galactic halo, which has a luminous inner component defined
by globular star clusters and other easily observable stars (with coronae of hot gas possibly expelled
by supernovae and of high - velocity neutron stars) and an outer
dark -
matter component inferred from its gravitational impact on the Milky Way's spiral disk.
In 2007, a similar collision with the Milky Way was projected for Smith's
Cloud within 20 to 40 million years, which is now believed to be surrounded
by a massive halo of
dark matter so that the entire incoming object has a «tidal mass» of some 300 million Solar - masses.
Comerón's scenario, however, was considered to be unlikely for a tenuous gas
cloud until astronomers came to realize that such
clouds could be held together
by a massive clump of
dark matter.
SDSS studies have probed the
dark matter environments of quasars through clustering measurements, revealed populations of quasars whose central engines are hidden
by obscuring dust, captured changes in quasar spectra that show
clouds moving in the gravitational grip of the central black hole, and allowed a comprehensive census of the much fainter accreting black holes (active galactic nuclei, or AGN) in present - day galaxies.
Brown
clouds contain
dark aerosols such as soot that are released into the atmosphere
by burning organic
matter.