Menu

M37

Salt and Pepper Cluster

Open Cluster Showpiece (78/100)
M37 OpenCluster Auriga Visible Level 2 Small telescope (4") - Wide field preferred
Star Map Add to List Add to Plan
Back to Catalog

Properties

Magnitude 6.2
Angular Size 11.4′
Distance 4400 ly
Open Cluster [Distance: 4400 ly]

Position & Identifiers

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

Visibility

Set a location in User Settings to see visibility data.

Survey Image

Loading survey image…

About M37

Description

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.

Observing Tips

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.

History

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.

Fun Facts

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.

Community Photos (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