Richer, Harvey BHeyl, JeremyAnderson, JayKalirai, Jason SShara, Michael MDotter, AaronFahlman, Gregory GRich, R M2015-12-132041-8205http://hdl.handle.net/1885/74538Based on the width of its main sequence, and an actual observed split when viewed through particular filters, it is widely accepted that 47 Tucanae contains multiple stellar populations. In this contribution, we divide the main sequence of 47 Tuc into fouKeywords: globular clusters: individual (47 Tuc); Hertzsprung Russell and diagrams; stars: kinematics and dynamics; stars: Population II201310.1088/2041-8205/771/1/L152016-02-24