A nebula is a gigantic cloud of dust and gas found in space, often hundreds of light-years across. Some nebulae are where new stars are born, while others are the leftover remains of dead or dying stars. Nebulae come in amazing shapes and glowing colors, creating some of the most beautiful sights in the universe.
The word "nebula" comes from the Latin word for "cloud." When telescopes were first invented, anything fuzzy in the sky was called a nebula. Later, astronomers learned that some of those fuzzy objects were galaxies, while others were true clouds of gas and dust — the nebulae we study today.
Nebulae form in several ways:
These materials — hydrogen, helium, and tiny dust particles — eventually clump together to start forming new stars and planets.
There are several different types of nebulae, each with unique properties:
Nebulae are vital for the life cycle of stars. They act as "stellar nurseries," where gas and dust gather to form new stars and planets. In a way, every star, including our Sun, was born in a nebula. Even we are connected to them — the elements in our bodies were once created inside stars that formed inside nebulae!
Nebulae also help astronomers study how stars live and die. By observing different types of nebulae, scientists understand more about the birth of solar systems, the recycling of matter in space, and the evolution of galaxies.
Even though nebulae seem thick and cloudy, they are actually very empty! If you were inside a nebula, you wouldn't notice anything around you — they are much less dense than even the best vacuums we can create on Earth!