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Emendatio ex 18:21, 15 Decembris 2011

Diagramma Hertzsprung-Russell anno 1913 ab Henrico Norris Russell scriptum est, qui cogitationibus astronomi Ejnari Hertzsprung usus est.

Hoc in diagrammate altera axi color altera luminositas absoluta stellarum inscriptae sunt. Omnes stellae in regionibus certe divisis in diagrammate videntur. Plurimae stellae in serie principali sitae sunt, etiam Sol. Stellae huius seriei classem spectralem V fingunt generum O, B, A, F, G, K, M, R, N, S, T (magnitudinum 6–16). Unicuique harum classium sunt decem subclasses (0–9). Gigantes, ingentissimae, subgigantes, pumiliones albae, alias classes fingunt.

Diagramma Hertzsprung-Russell

Vide etiam

Haec stipula ad astronomiam spectat. Amplifica, si potes!