A Galaxy is a massive conglomeration of stars and gas that is bound together by the collective gravity of all the objects, It has a center of mass so strong that it can preside over thousands, millions, billions, or even trillions of stars.
Our home galaxy the Milky Way is a barred spiral galaxy, about 100,000 light-years across. If you could look down on it from the top, you would see a central bulge surrounded by four large spiral arms that wrap around it. Spiral galaxies make up about two-third of the galaxies in the universe.
The Milky Way does not sit still, but is constantly rotating. As such, the arms are moving through space. The sun and the solar system travel with them. The solar system travels at an average speed of 515,000 mph (828,000 km/h). Even at this rapid speed, the solar system would take about 230 million years to travel all the way around the Milky Way.
There are different types of galaxies
1. Spiral galaxies:
They have a flat disc structure with extended spiral arms extending around a central bulge.
A spiral galaxy is said to be edge-on when it is highly tilted with respect to our line of sight and is therefore seen "sideways".
Our Milky Way
A special case of a galaxy that appears edge-on is our Milky Way. Due to Earth's position close to the galactic plane, the galaxy appears as a bright band in side view. Since the earth is part of our Milky Way, this band also extends across the entire firmament.
2. Elliptical galaxies:
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These galaxies are elliptical, spherical, or lenticular in shape and do not have a pronounced spiral structure. They mostly contain older stars.
3. Irregular galaxies:
Irregular galaxies do not have a uniform shape and structure. They can appear chaotic and erratic, and may have been created by galactic interactions or other disturbances.
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