Its properties were unique due to the special smelting and reworking of the steel creating networks of iron carbides described as a globular cementite in a matrix of pearlite.

globular cluster

Globular clusters

Globular Clusters

Globular Cluster

Globular Cluster M107 (also known as Messier Object 107 or NGC 6171) is the last globular cluster in the Messier Catalogue.

And that's the shell around that globular fat.

Messier 62 (also known as M62 or NGC 6266) is a globular cluster in the constellation Ophiuchus.

Messier 54 (also known as M54 or NGC 6715) is a globular cluster in the constellation Sagittarius.

The estimated mass of the cluster is 450,000 solar masses, suggesting it may become a globular cluster in the future.

Messier 30 (also known as M30 or NGC 7099) is a globular cluster of stars in the southern constellation of Capricornus.

The estimated mass of the cluster is 450,000 solar masses, suggesting it will likely become a globular cluster in the future.

Messier 55 (also known as M55 or NGC 6809 or The Summer Rose Star ) is a globular cluster in the constellation Sagittarius.

Stars can be much closer to each other in the centres of galaxies and in globular clusters, or much farther apart in galactic halos.

He had globular eyes starting out of his head with a fishy glitter, bumps on his forehead, and wore his long hair brushed back without a parting.

This issue was partially resolved in the late 1990s when new computer simulations, which included the effects of mass loss due to stellar winds, indicated a much younger age for globular clusters.

Computer simulations that matched the observations of the stellar populations of globular clusters suggested that they were about 15 billion years old, which conflicted with the 13.8 billion year age of the universe.