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Spiral Galaxy

(flat galaxy with spiraling arms)

A Spiral Galaxy is a flat galaxy with spiraling arms (Spiral Arms). One of three Galaxy classes described by Edwin Hubble along with elliptical galaxies and lenticular galaxies. The Galaxy Classification designations for spiral galaxies are SA or SB followed by a letter, a,b,c or d, indicating how tight are the arms. SB is for Barred, i.e., a Barred Galaxy, a spiral galaxy whose center appears like a Bar between two opposing arms rather than just a circular mass of stars.

Spiral galaxies are generally younger than elliptical galaxies with more interstellar gas and Dust, and are generally forming stars.

The dynamics that produces the galaxy's Spiral Structure (i.e., the spiral arms) is not immediately apparent: even given the unexplained "slow" orbits of stars, entire arms of orbiting stars would wrap far tighter than what is evident from populations. Theories are under study including the concept that the visible bright arms consist of young, bright stars resulting from rotating "fronts" of Star Formation.


The Large Magellanic Cloud and Small Magellanic Cloud were earlier considered irregular but are now sometimes cited as single-armed spiral galaxies.

(galaxy type)

Referenced by:
Comet Galaxy
Cosmic Distance Ladder
Dwarf Galaxy
Elliptical Galaxy
ESO 137-001
Freeman's Law
Galaxy Classification
Galaxy Formation
Galaxy Merger
Grand Design Spiral Galaxy
HII Region (HII)
IC 342
Lindblad Torque
Large Magellanic Cloud (LMC)
Messier 100 (M100)
Pinwheel Galaxy (M101)
Andromeda (M31)
Triangulum Galaxy (M33)
Whirlpool Galaxy (M51a)
Messier 74 (M74)
Milky Way
Morgan Classification
NGC 2770
NGC 3314
Scutum-Centaurus Arm
Synthetic Field Method (SFM)
Standard Candle
Tully-Fisher Relation (TFR)