The Trumpler Classification


1600x1200px with open cluster names


The Trumpler Type

The Trumpler classification system of open clusters was invented by R.J. Trumpler. The classification is based on three parameters:

Degree of concentration

I.

II.

III.

IV.

Detached clusters with strong central concentration.

Detached clusters with little central concentration.

Detached clusters with no noticeable concentration.

Not well detached from surrounding star field.

Range of brightness

1.

2.

3.

Most of the cluster stars are nearly the same apparent brightness.

Moderate range in brightness.

Cluster is composed of bright and faint stars.

Number of stars in cluster

p.

m.

r.

Poor (less than 50 stars).

Medium rich (50-100 stars).

Rich (more than 100 stars).

The letter 'n' following the Trumpler type means that there is nebulosity associated with the cluster.

Image Data

The above image shows twelve open clusters, sorted by the degree of concentration (horizontally) and sorted by the richness of stars (vertically). The range of brightness of all shown clusters is 2 or 3.

 

Source: WEBDA (Lynga catalogue)

 

The following links give detailed information about the cluster images.

  I II III IV
r NGC 6791 NGC 7789 NGC 6940 NGC 1817
m NGC 436 NGC 7790 NGC 129 DoDz 9
p NGC 7788 NGC 1807 NGC 7686 Stock 12
 
 

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