While there are many fascinating objects in the night sky to turn a telescope towards, star clusters are bountiful starscapes – glittering clumps of hundreds to millions of stars bound together by their collective gravity and travelling through space as one. As the stars that make up a cluster were born from the same cloud of gas and dust, they have similar ages and chemical compositions. This makes star clusters useful in the study of stellar evolution, as their member stars can be compared to see how stars of different sizes and masses change over time.
Star clusters fall into two categories: open and globular. Globular clusters are older – many over 10 billion years old – with an abundance of yellow and red giant stars. They possess thousands of individual stars and are particularly dense nearer their cores, with immense gravitational forces pulling them into roughly symmetrical spherical shapes. These sparkling stellar collections are most likely to be found in the halos of galaxies, orbiting far from the centre above and below the galactic plane. The Milky Way has around 150 globular clusters in orbit, but the giant elliptical galaxy Messier 87 is known to possess over 1,000 of these starstudded objects, revealing that they’re common across the cosmos.
Open clusters are much less dense, at most made up of a few thousand stars, with the less intense gravity meaning they’re loosely bound together and don’t take on a distinct shape. The stars that make up open clusters are younger, hotter blue stars, and some of these clusters possess enough leftover stellar material that star formation can still take place. Open clusters are found in the discs of galaxies, particularly near spiral arms. Unlike more stable globulars, open clusters are short-lived, with the members likely to drift apart naturally over millions of years or be affected by gravitational perturbations that break up the group.
1 THE PLEIADES
This story is from the Issue 161 edition of All About Space UK.
Start your 7-day Magzter GOLD free trial to access thousands of curated premium stories, and 9,000+ magazines and newspapers.
Already a subscriber ? Sign In
This story is from the Issue 161 edition of All About Space UK.
Start your 7-day Magzter GOLD free trial to access thousands of curated premium stories, and 9,000+ magazines and newspapers.
Already a subscriber? Sign In
MYSTERIES OF THE UNI WHERE ARE ALL THE SPIRAL GALAXIES?
There are far fewer spiral galaxies than elliptical ones in the Supergalactic Plane, and scientists are keen to discover why
ZOMBIE STARS
+10 OTHER TERRIFYING SPACE OBJECTS
HOW TO BEAT LIGHT POLLUTION
Thought it was impossible to observe the wonders of the night sky from towns and cities? Think again. Follow our tips and tricks on successfully observing through sky glow
15 STUNNING STAR CLUSTERS
These beautiful stellar groupings are spattered across the cosmos
Eileen Collins "It was a difficult mission...we were the first to see Mir"
Having served as both the first female pilot and first female commander of NASA's Space Shuttle, Collins boosted the involvement of women in space exploration to a whole new level
MARS LEAKS FASTER WHEN IT'S CLOSER TO THE SUN
The Red Planet has lost enough water to space to form a global ocean hundreds of kilometres deep
FUTURE TECH KANKOH-MARU
This ambitious reusable spacecraft will be capable of taking 50 people to and from orbit
THE FINAL FRONTIER
Beyond the reach of the Sun is a fascinating region of the cosmos that were only just beginning to explore
A long-lost moon could explain Mars' weird shape and extreme terrain
A long-lost moon could explain why Mars is so different from the other rocky planets in the Solar System. Today Mars has two tiny moons.
A sprinkling of cosmic dust may have helped kick-start life on Earth
Cosmic dust may have helped kick-start life on Earth. New findings challenge a widely held assumption that this wasn't a plausible explanation.