| 10.11 |
Galaxy properties
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Like all form in the Universe, the vast
majority of galaxies into a few common shape patterns, that then vary according
to size and general features such as rate of change of position, rotation rate,
distance, general attraction or repulsion to or from other galaxies.
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The most common shape varieties of
galaxies |
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The four main classes of galactic shapes
are: |
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(1) Spiral |
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These galaxies resemble pin wheels, with
spiral arms trailing out from a brighter centre. The largest galaxies appear to
be Spiral in shape and almost always have companion smaller galaxies (
sometimes called pygmy galaxies). |
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(2) Barred spiral |
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Here the spiral arms trail from the ends
of a central bar around 30% of galaxies are spirals or barred spirals. All
barrel spiral galaxies are in pairs, with the barrel effect being created from
the gravitation pull of the second galaxy. |
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(3) Elliptical |
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These galaxies do not have spiral arms.
About 60% of galaxies are elliptical, varying in shape from almost spherical
(like a soccer ball) to very flattened (like a football). Elliptical galaxies
are usually very small, and most often the "pygmy" type galaxies that cluster
around much larger galaxies. |
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(4) Irregular |
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About 10% of galaxies are irregular with
no definite shape.
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