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Every star has its own life cycle, ranging from a few million to trillions of years, and its properties change as it ages. Overview the space between stars is dotted with twisting towers studded with stars, unblinking eyes, ethereal ribbons, and floating bubbles Scientists call a star that is fusing hydrogen to helium in its core a main sequence star

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Main sequence stars make up around 90% of the universe’s stellar population. Because most stars in our galaxy belong to binary systems, studying nebulae like this helps us understand how stellar pairs evolve and how they enrich the galaxy with the elements needed to form new stars and planets. All stars are born in clouds of dust and gas like the pillars of creation in the eagle nebula pictured below

In these stellar nurseries, clumps of gas form, pulling in more and more mass as time passes

As they grow, these clumps start to spin and heat up. Stars are the most basic building blocks of galaxies The age, distribution, and composition of stars trace the history, dynamics, and evolution of their galaxy. Groups of stars make up galaxies, while planets and ultimately life arise around stars

Although stars have been the main topic of astronomy for thousands of years, we have begun to understand them in detail only in recent times through the advent of powerful telescopes and computers. Stars form in large clouds of gas and dust called nebulae that scatter the visible wavelengths of light our eyes can see To explore the skymap, scroll, double click, or pinch/swipe to zoom in and out.