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A Barred Spiral Galaxy is a galaxy with a central bar-shape, composed of stars.
An Elliptical Galaxy is a type of galaxy with an ellipsoidal shape.
These four classes are used to classify common galaxies,
Also known as, "The Hubble Sequence".
An Irregular Galaxy is a galaxy that does not have a distinct regular shape.
A Spiral Galaxy has a rotating disc with spiral ‘arms’ that curve out from a dense central region.
A Barred Spiral Galaxy is a galaxy with a central bar-shape, composed of stars.
NGC 1073 ~ Credits ~ NASA, ESA, and The Hubble Heritage Team (STScI/AURA)
An Elliptical Galaxy is a type of galaxy with an ellipsoidal shape.
NGC 4150 ~ Credits ~ NASA, ESA, and The Hubble Heritage Team (STScI/AURA)
Astronomer Edwin Hubble 🔭
These four classes are used to classify common galaxies,
Also known as, "The Hubble Sequence".
An Irregular Galaxy is a galaxy that does not have a distinct regular shape.
NGC 1427a ~ Credits ~ NASA, ESA, and The Hubble Heritage Team (STScI/AURA)
A Spiral Galaxy has a rotating disc with spiral ‘arms’ that curve out from a dense central region.
Andromeda Galaxy ~ Credits ~ NASA, ESA, and The Hubble Heritage Team (STScI/AURA)
Some galaxies have a ring-like structure of stars and interstellar medium surrounding a bare core.
A Lenticular Galaxy has qualities of both Elliptical Galaxies and Spiral Galaxies, sometimes called an Armless Spiral.
A Peculiar Galaxy is a galaxy of unusual size, shape, or composition.
Starburst Galaxies that are characterized by dusty concentrations of gas.
Some galaxies have a ring-like structure of stars and interstellar medium surrounding a bare core.
Hoag's Object ~ Credits ~ NASA, ESA, and The Hubble Heritage Team
A Lenticular Galaxy has qualities of both Elliptical Galaxies and Spiral Galaxies, sometimes called an Armless Spiral.
NGC 6861 ~ NASA, ESA and The Hubble Heritage Team
A Peculiar Galaxy is a galaxy of unusual size, shape, or composition.
ARP-MADORE0002-503 ~ Credits ~ NASA, ESA, STScI, Julianne Dalcanton (UW)
Starburst Galaxies that are characterized by dusty concentrations of gas.
M83 ~ Credits ~ NASA, ESA, and The Hubble Heritage Team
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