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No known globular clusters display active star formation, which is consistent with the view that globular clusters are typically the oldest objects in the Galaxy, and were among the first collections of stars to form.
From the location of the Main Sequence Turn-Off, you can see that NGC 2362 is the youngest, then h & Versa, and M67 is the oldest of the clusters.
Open cluster ages are predominantly young, and they are often associated with interstellar material by virtue of this youth. The youngest of these clusters have bright main sequence stars, blue super giants, and sometimes a few variables, either young Cepheid's or even younger T Lauri stars.
As time passes the most massive stars at the top of the main sequence evolve into red giants. Therefore, the older the cluster, the fewer stars to be found at the top of the main sequence, and an obvious grouping of red giants will be seen at the top right of the HR diagram.
Stars emit colors of many wavelengths, but the wavelength of light where a star's emission is concentrated is related to the star's temperature — the hotter the star, the more blue it is; the cooler the star, the more red it is. ... So that is one way in which older stars are redder than young stars.
As a cluster ages, the mass of the main-sequence turnoff stars decreases. By determining the mass of the main-sequence turnoff stars, we get the age of the cluster. The cluster age equals the main-sequence lifetime of the turnoff stars.
Typical results for globular clusters are that they may be as old as 12.7 billion years. This is in contrast to open clusters which are only tens of millions of years old. The ages of globular clusters place a bound on the age limit of the entire universe.
As a cluster ages, the mass of the main-sequence turnoff stars decreases. By determining the mass of the main-sequence turnoff stars, we get the age of the cluster. The cluster age equals the main-sequence lifetime of the turnoff stars.
Globular clusters formed from giant molecular clouds, or huge masses of gas that form stars as they collapse. ... However, there is a globular cluster forming in a galaxy near to the Milky Way called the Large Magellanic Cloud.
Globular clusters were given this name because they are nearly symmetrical round systems of, typically, hundreds of thousands of stars. The most massive globular cluster in our own Galaxy is Omega Centaur, which is about 16,000 light-years away and contains several million stars (Figure 1).
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