Star clusters

Deep space objects > Star clusters

Star clusters are a group of stars with a common origin and a gravitational link for a specific time. It is a useful tool for astronomers as it helps study and model stellar evolution. There are two main types of star clusters: open clusters (open) and globular clusters. Learn more about the galaxy s star clusters in an interesting video.

Types of star clusters

Open star clusters are so named because individual stars can be resolved easily. For example, the Pleiades and Hyades are so close that individual stars can be easily seen with the naked eye. They are sometimes called galactic clusters because they are located in dusty spiral arms. Stars in an open cluster have a common origin (the same initial molecular cloud was formed). Usually, the cluster contains several hundred stars (can reach several thousand).

The stars are bound by gravity, but it s pretty weak. The cluster revolves around the galaxy and finally dissipates due to gravitational contact with stronger objects. It is believed that the Sun appeared in an open cluster, which no longer exists. Therefore, these are always young objects. A nebula is still visible in the Pleiades, hinting at recent formation.

The open clusters are filled with Population I stars — young and highly metallic. In width, cover from 2 to 20 parsecs.

Messier open star clusters

M6

M7

M11

M18

M21

M23

M25

M26

M29

M34

M35

M36

M37

M38

M39

M41

M44

M45

M46

M47

M48

M50

M52

M67

M93

M103

Other notable open star clusters

The Perseus Cluster

Hyades star cluster

Jewelry box

Christmas tree

Snowflakes

Globular clusters of galaxies contain from a couple of thousand to a million stars located in a spherical gravitational system. They are in a halo and represent the most ancient stars – population II (developed, but low metallicity). The clusters are so old that any star (above the G or F class) has already stepped over the main sequence. The globular cluster has little dust and gas because new stars do not form there. The density in the interior is much higher than in areas near the Sun.

In globular clusters, stars also share a common origin. But this type holds objects firmly by gravity (stars do not scatter). There are approximately 200 globular clusters in the Milky Way. Among them, you can recall 47 Toucan, M4 and Omega Centauri. Although about the latter, there are suggestions that it may be a dwarf spheroidal galaxy.

Messier globular star clusters

M2

M3

М4

M5

M9

M10

M12

M13

M14

M15

M19

M22

M28

M30

M53

M54

M55

M56

M62

M68

M69

M70

M71

M72

M75

M79

M80

M92

M107

Other notable globular star clusters

Omega Centauri

Age of star clusters

Star clusters are incredibly valuable to astronomers because they can help determine the age of a star and track its evolution.

The stars of open clusters have a common origin, so their metallicity levels converge, which means that all members will pass through the evolutionary stages in the same way. In addition, they are located at the same distance, which also allows you to display the absolute value. If you see bright stars that stand out, then they are much lighter than their weaker neighbors.

With this information, scientists create digital charts for the clusters. They display the apparent value of V on the vertical axis relative to the digital index B – V horizontally. With spectrographic parallax, you can calibrate the chart to display the absolute value.

If we build diagrams for them, we get the bottom graph. Since they are at different distances, it is calibrated to absolute values.

A new scale is visible on the right vertical axis. “Years” is the age of the cluster. The pair in Perseus is so young that most of the stars are in the main sequence stage. The Pleiades are slightly older and do not have stars exceeding color index 0 (spectral type A0). More massive objects have already stepped over to the giant branches. M67 does not have a star hotter than a color index of 0.4. Most significant is the pivot point in the diagram, where the cluster turns off the main sequence. The lower the main sequence, the older the cluster.

Globulars are usually much older than open ones, so the color magnitude in the diagram shows more developed stars. They are also devoid of objects with a large mass. This point is illustrated below for example M55.

There is a cluster of hot stars in the main sequence above the shutdown point. They are called blue stragglers. Scientists believe that due to the high stellar densities in globular clusters, some are capable of merging. The combined mass makes the star hotter and brighter than the main mass. Star clusters are not eternal structures and they are destroyed. Examine this process in the video. Also, use the online star map to find the clusters yourself. If you can t buy a telescope, then visit our page with a virtual model of the Milky Way galaxy or view a photo from the list of clusters.