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Circumstellar disc

Imagine giant cosmic donuts spinning around baby stars, where planets might be born!

Images

Circumstellar disc

Circumstellar disc

wikipedia
File:Viewing the Vermin Galaxy.jpg
Rho Ophiuchi cloud complex (weic2316a)
Circumstellar Disks HD 141943 and HD 191089
A young star takes centre stage
Circumstellar disc IRAS 23077+6707 (opo2606)
PDS 70 closeup - eso2111a
HL Tau protoplanetary disk
Artist's rendering of the 2M1207 System
Potw1742a
Caught in a Dust Trap
Wide and close-up views of a moon-forming disc as seen with ALMA

Key Facts

What It Is
A flat, spinning ring of gas and dust around a young star.
How It Forms
From the leftover material when a star is born from a gas cloud.
What Happens There
Planets, moons, and asteroids are formed within the disc.
Size Comparison
Can be much larger than our entire solar system.

Meet the Cosmic Donut!

Around a brand new star, there's a giant, flat, spinning ring of dust and gas. It looks a bit like a giant donut or a frisbee! This is called a circumstellar disc.

It's made of tiny bits of rock and ice, like the stuff that makes up planets. These discs are super important because they are like nurseries for baby planets. They are often much bigger than our whole solar system, stretching out for billions of miles!

Where Do These Rings Come From?

When a star is born, it doesn't just pop into existence all by itself. It forms from a giant cloud of gas and dust in space. As this cloud collapses and gets smaller, it starts to spin faster, just like an ice skater pulling their arms in.

Most of the stuff spins into a flat disc around the new star. This disc is the birthplace of planets, moons, and even asteroids. It’s like the leftover ingredients from making a star!

Why Are They So Cool?

These cosmic donuts are super important because they are where planets are made! The dust and gas in the disc bump into each other and stick together. Over millions of years, these little clumps grow bigger and bigger, eventually becoming planets like Earth or Mars.

Scientists study these discs to understand how our own solar system got started. It’s like looking at a baby picture of our cosmic home!

Spinning into Planets!

Inside the disc, the tiny dust grains start to clump together. Imagine tiny snowflakes sticking to each other. These clumps get bigger, forming pebbles, then rocks, and then giant boulders.

Eventually, these grow into planetesimals, which are like baby planets. Gravity pulls these together, and if they get big enough, they become full-fledged planets! Some discs have rings and gaps, showing where planets are already forming and clearing out their paths.

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Based on content from Wikipedia · Licensed under CC BY-SA 4.0