Shapley–Sawyer Concentration Class
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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.)
From 1927 to 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.
Classes
| Class | Description | Example |
|---|---|---|
| I | High concentration toward the center | Messier 75 |
| II | Dense central concentration | Messier 2 |
| III | Strong inner core of stars | Messier 54 |
| IV | Intermediate rich concentrations | Messier 15 |
| V | Intermediate concentrations | Messier 30 |
| VI | Intermediate mild concentration | Messier 3 |
| VII | Intermediate loose concentration | Messier 22 |
| VIII | Rather loosely concentrated towards the center | Messier 14 |
| IX | Loose towards the center | Messier 12 |
| X | Loose | Messier 68 |
| XI | Very loose towards the center | Messier 55 |
| XII | Almost no concentration towards the center | Palomar 12 |