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Astronomers find potential Solution into how Planets Form

This image shows V1247 Orionis, a young, hot star surrounded by a dynamic ring of gas and dust, known as a circumstellar disc. The disc can be seen in two parts: a clearly defined central ring of matter and a more delicate crescent structure located further out. Credit: Stefan Kraus

This image shows V1247 Orionis, a young, hot star surrounded by a dynamic ring of gas and dust, known as a circumstellar disc. The disc can be seen in two parts: a clearly defined central ring of matter and a more delicate crescent structure located further out. Credit: Stefan Kraus

The quest to discover how planets found in the far reaches of the universe are born has taken a new, crucial twist. A new study by an international team of scientists, led by Stefan Kraus from the University of Exeter, has given a fascinating new insight into one of the most respected theories of how planets are formed. Young stars start out with a massive disk of gas and dust that over time, astronomers think, either diffuses away or coalesces into planets and asteroids.

However, scientists are still searching...

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