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It depends on the galaxy and how far you are from it

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16y ago

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What is the type of our galaxy?

Our galaxy is a spiral galaxy because it is spiral in shape.


What shape does an spiral galaxy have?

First of all, it's a spiral galaxy, not an spiral galaxy. Second, a spiral galaxy would have a spiral shape, obviously.


Is an Sab galaxy a type of spiral galaxy?

Yes, a SBC galaxy is a type of a spiral galaxy. The have loosely bounded arms.


The Milky Way is one?

The Milky way is a galaxy. A spiral galaxy, to be more precise.The Milky way is a galaxy. A spiral galaxy, to be more precise.The Milky way is a galaxy. A spiral galaxy, to be more precise.The Milky way is a galaxy. A spiral galaxy, to be more precise.


Which is not part of a spiral galaxy?

A galaxy orbiting outside spiral galaxy


What type of galaxy has a nuclear region of more or less uniform brightness from which long lines of stars curve outward?

Spiral galaxies.


The Milky Way Galaxy is a member of the?

The Milky Way Galaxy is a member of the Local Group, a collection of galaxies that includes around 54 members. Within the Local Group, the Milky Way is one of the largest galaxies and is gravitationally bound to other galaxies such as Andromeda.


How are elliptical galaxies different from spiral galaxy's?

An elliptical galaxy is round. A spiral galaxy is shaped like a spiral.


Which galaxy is thick in the center and has flattened arms?

A spiral galaxy or barred spiral.


Is Andromeda a spiral galaxy?

Yes, the Andromeda Galaxy is a spiral.


What type of a galaxy is the milky way galaxy?

The milky way is classified as a galaxy... A barred spiral galaxy.


Why does the dark matter theory explain the decrease in brightness of spiral galaxies?

The dark matter theory explains the decrease in brightness of spiral galaxies because dark matter does not emit, absorb, or reflect electromagnetic radiation, making it invisible to telescopes that rely on detecting light. The presence of dark matter provides extra mass in the galaxy, which affects the gravitational interactions within the galaxy and with other galaxies in a way that accounts for the observed decrease in brightness at large distances from the center.