Shapley–Sawyer Concentration Class

The Shapley–Sawyer Concentration Class is a classification system on a scale of one to twelve using Roman numerals for globular clusters according to their concentration. The most highly concentrated clusters such as M75 are classified as Class I, with successively diminishing concentrations ranging to Class XII, such as Palomar 12. (The class is sometimes given with numbers [Class 1–12] rather than with Roman numerals.)

History

From 1927–1929, Harlow Shapley and Helen Sawyer Hogg began categorizing clusters according to the degree of concentration the system has toward the core using this scale. This became known as the Shapley–Sawyer Concentration Class.^[1]

Classes

Class	Description	Example
01 !I	High concentration toward the center
02 !II	Dense central concentration	Messier 2
03 !III	Strong inner core of stars	Messier 54
04 !IV	Intermediate rich concentrations	Messier 15
05 !V	Intermediate concentrations	Messier 30
06 !VI	Intermediate	Messier 3
07 !VII	Intermediate	Messier 22
08 !VIII	Rather loosely concentrated towards the center	Messier 14
09 !IX	Loose towards the center	Messier 12
10 !X	Loose	Messier 68
11 !XI	Very loose towards the center	Messier 55
12 !XII	Almost no concentration towards the center	Palomar 12

^[2]

References