| HotLiquidMagma.com A Practical Guide to Astronomy |
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Galaxies |
Our Own Galaxy: The Milky WayThe Milky Way contains about 250 billion stars, any of which may have orbitting planets like our solar system. Some solar systems in our galaxy are binary (two stars revolving around each other). Others consist of dying stars.Our galaxy is the spiral-shaped type with several arms. Our Sun is about two-thirds of the way out from the centre hub and is located on the arm called Orion Spur. The Sagittarius arm is located between us and the galactic center, the Perseus Arm wraps itself behind us. Some scientist believe there is a black hole at the centre of our Galaxy that may be slowly sucking in the surrounding light and gas. If we wanted to travel the diameter of our galaxy it would take about 100,000 years- travelling at the speed of light. Just as the moon rotates around the Earth, and the Earth rotates around the Sun, our Sun rotates around the Galaxy's center. It takes 225 million years to rotate around the galaxy. This is called a galactic year. Galactic Neighbours
The Milky Way is part of a cluster of about 20 other galaxies. This is a small cluster, since some clusters contain thousands of galaxies. Our group of 20 is part of a larger group known as the Virgo Supercluster. The largest galaxy in our group is called the Andromeda Spiral. It is about 2.3 million light years from Earth and contains about 400 billion stars. Andromeda can be seen from Earth with the naked eye.
The closest known neighbouring galaxy is the Magellanic Clouds, named after the famous explorer who first spotted them in 1521. In the 'clouds' are two irregular galaxies, one larger, containing about 10 billion stars, the other smaller and farther away. Other galaxies that are close enough to study from the Earth are: M81 (a spiral), M51 -the Whirlpool, another spiral, about 14 million light years away, reaches out to a smaller galaxy. Then there is M77 -another spiral, M87- which sends out strong radio waves and M104-a spiral nicknamed the Sombrero because of its shape.
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