Tilted Wonder
03 Септември 2020
This page isn't available in your language yet, if you'd like to provide a translation please contact us at info@unawe.org

Imagine a giant dinner plate that could fit our entire solar system. Almost all of the planets would be touching the plate because our solar system is very flat. But this is not always the case because some systems in the universe are tilted!

A Violent Series of Events

For a solar system to become tilted, something must have changed its shape. This can also happen long before planets form, when the system is still a large disc of gas and dust. 

An international team of astronomers have found the first direct evidence that groups of stars are strong enough to tear apart their planet-forming discs. This creates a warped and tilted disc!

The team studied a system called GW Orionis, which is 1300 light years away in the constellation Orion. This system has three stars and a large deformed, broken-apart disc surrounding them. 

A Home for Planets?

When a star is born, any leftover gas and dust forms a disc around it, similar to Saturn's rings. Within this disc, small dust grains made of rock or gas sometimes form. These grains can then collide and stick together, forming larger and larger objects. In these rings of dust and gas, called protoplanetary discs, is where planets are born.

No planets have formed in the peculiar tilted rings of GW Orionis... yet!

But, this new research suggests that planets may form in these tilted rings of gas and dust that encircle more than one star.


Image credit: ESO/Exeter/Kraus et al./L. Calçada

Интересно

Astronomers believe that around half of all planets live in star systems with at least two stars!

This Space Scoop is based on Press Releases from ESO, NAOJ, ALMA.
ESO NAOJ ALMA
Изображение
Версия за разпечатване
Още новини

Още си любопитен? Научи повече...

Какво е Space Scoop?

Открий още астрономически тайни

Вдъхновяваме ново поколение космически изследователи

Приятели на Space Scoop

Свържи се с нас

This website was produced by funding from the European Community's Horizon 2020 Programme under grant agreement n° 638653