Messiers Globular Clusters 12 to 15
Messier seems to have a thing for Globular clusters, at least at the start of his catalogue, although to be fair to him, his comments on these objects explains this somewhat.
This Messier described M12 as "A nebula without stars!"
It's easy to forget in a time of Hubble and JWST that Messier was dealing with instruments not that much better than a good pair of binoculars, and to him the object looked like a giant fuzzy patch, with no individual stars showing.
Messier 12 is odd in that it has a surprisingly low amount of the longest lived low mass stars (red dwarfs, K and G type stars), and with an age of 13.8 billion years old (pretty much the age of the universe itself), it's clearly passed through the milky way so many times, many of the lower mass stars have been ejected or found themselves pulled away, and likely now still live on in the central bulge.
M13 - The Great Hercules Cluster
The brightest of the stars in this cluster are the red giants, one in particular V1554 Hercules has an apparent mag 11.95 from 23,000 light years.
Interestingly, there's some blue stars here, but they are not young hot B or O type stars you find in Open Clusters, they are what are known as blue stragglers. Stars are so compressed in the heart of globular clusters that they do regularly merge, and when that happens, a blue straggler can be the product.
M14
Some 30,000 light years away from us in the constellation of Ophiuchus, it's 100 light years across and in total, 400,000 times the mass of our star, 10 times less than the supermassive black hole Sag A*.
M15 - The Great Pegasus Cluster
One of the most densely packed globular clusters known, so much so, the core (central region) has begin to contract in what is known as core collapse, where the mass of stars is so intense, it begins to pull in mass from around it, and most likely forming a intermediate black-hole, although none has ever been confirmed as such.
It is also the only globular cluster to ever be found to have a planetary nebula, Pease 1












