Edwin Hubble originally identified an evolutionary sequence for the galaxies (from early-type to late-type) as one moved from left to right across the diagram. Although this is now known to be a false interpretation, the terms 'early-type' and 'late-type' are still used regularly by astronomers in the manner described below, and when discussing broad galaxy types.
E = 10 x (1 - b/a)
where a = semi-major axis and b = semi-minor axis of the ellipse. Observed values range from E0 (circular cross section - a spherical galaxy) to E7 (the most flattened). E0 are considered 'early-type' ellipticals and E7 are 'late-type' ellipticals.
Spiral galaxies are classed from 'early-type' to 'late-type' according to the ratio of the luminosity of the bulge compared with the disk, and the amount of winding of the spiral arms. Type Sa (early) spiral galaxies have prominent bulges (bulge to disk luminosity ~0.3), tightly wound arms (pitch angle ~ 0.6), and the stars in the spiral arms are distributed very smoothly. Type Sc (late) spirals have the least prominent bulges (bulge-to-disk luminosity ~ 0.05), and loosely wound arms (pitch angle ~ 0.18) that are resolved into clumps of stars and HII regions.
In bars, the spiral arms do not start directly from the bulge, but from an extended bar of stars that passes through the bulge. They share the same range of classifications as non-barred spirals - from Type SBa (early) to SBc (late) - according to the prominence of the bulge and the winding of the spiral arms.
|Class||Absolute magnitude (B-band)||Mass (solar masses)||Diameter (kiloparsec)|
|Ellipticals||-8 to -23||107 to 1012||~0.3 to 100s||Spirals||-16 to -23||109 to 1012||5 to 100||Irregulars||-13 to -20||108 to 1010||1 to 10|