# data[].attributes.headline
 Spiral Galaxy the path of a point in a plane moving around a central point while continuously receding from or approaching it. b : a three-dimensional curve (such as a helix) with one or more turns about an axis. 2  a single turn or coil in a spiral object.

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 Spiral Galaxy the path of a point in a plane moving around a central point while continuously receding from or approaching it. b : a three-dimensional curve (such as a helix) with one or more turns about an axis. 2  a single turn or coil in a spiral object.

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An elliptical galaxy is a type of galaxy with an approximately ellipsoidal shape and a smooth, nearly featureless image. They are one of the three main classes of galaxy described by Edwin Hubble in his Hubble sequence and 1936 work The Realm of the Nebulae, along with spiral and lenticular galaxies.

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An irregular galaxy is the catchall name given to any galaxy that does not neatly fit into one of the categories of the Hubble classification scheme. They have no defined shape nor structure and may have formed from collisions, close encounters with other galaxies or violent internal activity.

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An example of Spirals. A spiral is a curved pattern that focuses on a center point and a series of circular shapes that revolve around it. Examples of spirals are pine cones, pineapples, hurricanes. The reason for why plants use a spiral form like the leaf picture above is because they are constantly trying to grow but stay secure.

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An example of Spirals. A spiral is a curved pattern that focuses on a center point and a series of circular shapes that revolve around it. Examples of spirals are pine cones, pineapples, hurricanes. The reason for why plants use a spiral form like the leaf picture above is because they are constantly trying to grow but stay secure.

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An Example of elliptical Examples.  , whose supermassive black hole is the first black hole to be imaged by the Event Horizon Telescope.  one of the largest galaxies in the observable universe. Maffei 1, the closest giant elliptical galaxy.

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An Example of elliptical Examples.  , whose supermassive black hole is the first black hole to be imaged by the Event Horizon Telescope.  one of the largest galaxies in the observable universe. Maffei 1, the closest giant elliptical galaxy.

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 An example of Irregular Magellanic cloudsThe best known examples of irregular galaxies are the Small and Large Magellanic clouds. These are companion galaxies to our own Milky Way, and can be easily seen at dark sites in the Southern Hemisphere. The Large (left) and Small (right) Magellanic clouds are prime examples of irregular galaxies.

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 An example of Irregular Magellanic cloudsThe best known examples of irregular galaxies are the Small and Large Magellanic clouds. These are companion galaxies to our own Milky Way, and can be easily seen at dark sites in the Southern Hemisphere. The Large (left) and Small (right) Magellanic clouds are prime examples of irregular galaxies.

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The definition of spiral Spiral galaxies are twisted collections of stars and gas that often have beautiful shapes and are made up of hot young stars. ... Most spiral galaxies contain a central bulge surrounded by a flat, rotating disk of stars.

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The definition of spiral Spiral galaxies are twisted collections of stars and gas that often have beautiful shapes and are made up of hot young stars. ... Most spiral galaxies contain a central bulge surrounded by a flat, rotating disk of stars.

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: a galaxy that has a generally elliptical shape and that has no apparent internal structure or spiral arms. — called also elliptical. — compare spiral galaxy.

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the definition of Irregular An irregular galaxy is the catchall name given to any galaxy that does not neatly fit into one of the categories of the Hubble classification scheme. They have no defined shape nor structure and may have formed from collisions, close encounters with other galaxies or violent internal activity.

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the definition of Irregular An irregular galaxy is the catchall name given to any galaxy that does not neatly fit into one of the categories of the Hubble classification scheme. They have no defined shape nor structure and may have formed from collisions, close encounters with other galaxies or violent internal activity.