M5


m5hst950Messier 5 (M5) is  a globular star cluster of 100,000 or more stars bound by gravity into a region around 165 light-years in diameter. It’s about 25,000 light-years away.  M5 is one of the oldest globulars in our galaxy, with stars estimated to be nearly 13 billion years old. The beautiful star cluster is a popular target for Earthbound telescopes. This closeup  that spans about 20 light-years near the central region of M5 was taken by the Hubble Space Telescope. The cluster’s aging red and blue giant stars and rejuvenated blue stragglers stand out in yellow and blue hues.

Image Credit: NASA

M80


M80No, not the firecracker, the star cluster.

M80 is in the constellation Scorpius between the stars α Scorpii (Antares) and β Scorpii in a part of the Milky Way rich in nebulae. When viewed with a modest amateur telescope (like mine), it appears as a mottled ball of light. This Hubble image shows more detail. M80 is roughly 95 light-years in diameter. It contains several hundred thousand stars, making it one of the more densely populated globular clusters in the galaxy.

M80 contains a fair number of blue stragglers, stars that appear to be much younger than the cluster itself. Astronomers believe that these stars lost part of their outer layers during close encounters with other cluster members or as the result of collisions between stars in the tightly packed cluster. Images from Hubble show regions with very high blue straggler densities which suggests that the center of the cluster probably has a very high capture and collision rate.

Image Credit: NASA / ESA

An Old Star Cluster


An ancient globuleThis is NGC 6535, a globular cluster 22,000 light-years away in the constellation of Serpens (The Serpent). It’s about one light-year across.

Globular clusters are tightly bound groups of stars which orbit galaxies. The Latin word globulus, from which these clusters take their name, means a small sphere.  A large mass in the rich stellar centre of a globular cluster pulls the stars inward to form a ball of stars.

Globular clusters are generally very ancient objects that form around the same time as their host galaxy. Thus far, no new star formation has been observed within any globular cluster. The lack of young stars explains the abundance of aging yellow stars in this image, most of them containing very few heavy elements.

Image Credit: NASA

Messier 69


This is an image of the core fo the globular star cluster Messier 69. It is made up of visible light and infrared data taken by the Hubble Space Telescope. The cluster was discovered by Charles Messier in 1780. It’s located 29,700 light-years from Earth in the constellation Sagittarius. It’s too dim to be seen with the naked eye, but it can be viewed with a pair of binoculars, especially during August.

The stars in M69 have over ten times more iron than stars in other globular clusters of the same age. Iron is the heaviest element created by fusion in a star unless it explodes as a supernova.

Image Credit: NASA / ESA

Messier 2


Messier 2 or M2 (aka NGC 7089) is a globular cluster in the constellation Aquarius. It’s one of the larger globular clusters known—rich, compact, and significantly elliptical—containing over 150,000 stars. It’s one of the oldest globulars in our galaxy, around 13 billion years old. This Hubble image shows the core of the cluster.

Image Credits: NASA, ESA, STScI, and A. Sarajedini (University of Florida)

Messier 70


Messier 70 (aka M70 or NGC 6681) is a globular cluster of stars in the southern constellation of Sagittarius. It’s about 29,400 light-years away from Earth and roughly 6,500 light-years from the Galactic Center. M70 has undergone core collapse, so it has a very small core radius of 0.22 light-years.

Image Credit: NASA / ESA