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Massa Solis

E Vicipaedia

Massa Solis (M, ubi ☉ est vexillum astronomicum pro Sole) est unitas astronomica massae aequalis circiter 2×1030 kg. Solet saepe eligi ad massam aliarum stellarum atque nebularum, galaxiarum, foraminum nigrorum et cumulorum stellarum mensurandam. Massa Solis est circiter 2000 quettagrammatum, vel 2000 Qg:[1]

Id est fere 333 000 massarum Telluris (M), vel 1047 massarum Iovis (M).

Nexus interni

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