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M37

Salt and Pepper Cluster

Cúmulo Abierto Espectacular (78/100)
M37 OpenCluster Auriga Visible Nivel 2 Small telescope (4") - Wide field preferred
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Propiedades

Magnitud 6.2
Tamaño Angular 11.4′
Distancia 4400 ly
Open Cluster [Distance: 4400 ly]

Posición e Identificadores

RA 05h 52m 18.0s
Dec +32° 33' 02.0"
Constelación Auriga
Catálogo M37

Visibilidad

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Acerca de M37

Descripción

M37 is the richest and brightest of the three Auriga Messier clusters, about 4,500 light-years from Earth. It contains roughly 500 stars across about 25 light-years, with an age of 350-550 million years. The cluster is notable for containing at least a dozen red giant stars among its white and blue members, creating a subtle color contrast.

Consejos de Observación

Located about 3.5 degrees southeast of M36. The richest of the Auriga trio. Binoculars show a large, bright, granular patch. A telescope at 80-100x reveals a spectacular dense field of faint stars — often described as 'salt and pepper' due to the mix of faint white stars with brighter orange-red giants scattered throughout. One of the finest open clusters in the sky. Best observed from November through March.

Historia

Discovered by Giovanni Battista Hodierna before 1654 and independently found by Charles Messier in 1764. Its richness and beauty have made it one of the most observed open clusters by amateur astronomers.

Datos Curiosos

M37 contains about 150 white dwarf stars — the remnants of higher-mass stars that have already completed their evolution. The contrast between these dead stellar remnants, the red giants nearing the end of their lives, and the main-sequence stars still in their prime makes M37 a showcase of stellar evolution in a single object.

Fotos de la Comunidad (1)

Credit: Jim Mazur. License: CC BY-SA 4.0. (Wikimedia Commons)

Credit: Jim Mazur. License: CC BY-SA 4.0. (Wikimedia Commons)

Skybred Feb 28, 2026