‘Great Divide’ in our solar system between rocky inner planets and outer gas giants was caused by pressure changes in a ring of dust and gas around the early Sun
- Protoplanetary discs form around early stars and lead to planetary systems
- This disc had bands of high and low pressure that split material off into two areas
- One side formed the inner rocky planets and the other the outer gas planets
The ‘great divide’ in the Solar System that splits inner rocky planets from outer gas giants was caused by a ‘ring around the Sun’, scientists claim.
The ring, known as a protoplanetary disc, was made up of dust and gas particles which combined to form the planets and moons we have today.
Researchers from Japan and the USA say this disc would have had bands of high and low pressure that split off to create the two distinct regions in the solar system.
One led to Jupiter, Saturn and the other outer planets with high levels of carbon molecules, while the other led to the creation of Earth and Mars.
Some of those high carbon elements likely crossed the divide and may have led to organic molecules, water and then life on Earth, the researchers claim.
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Researchers from Japan and the USA say this disc would have had bands of high and low pressure that split off to create the two distinct regions. To the sunside there were rocky planets low in organic molecules and to the Jupiter side gas giants high in carbon
The team, led by Ramon Brasser from the Tokyo Institute with Stephen Mojzsis from the University of Boulder created computer models of the early solar system.
They also examined other young systems in the universe that have active protoplanetary discs surrounding the host star.
Dr Brasser compared the divide in the solar system to the Rocky Mountain range in the USA that splits the country east and west.
In the mountains, ‘the Great Divide causes water to drain one way or another,’ Mojzsis said. ‘It’s similar to how this pressure bump would have divided material’ in the solar system.
The solar system ‘Great Divide’ does not look like much today, according to Dr Mojzsis, who said it is now a relatively empty stretch of space.
‘You can still detect its presence throughout the solar system. Move sunward from that line, and most planets and asteroids tend to carry relatively low abundances of organic molecules.
‘Go the other direction toward Jupiter and beyond, however, and a different picture emerges: Almost everything in this distant part of the solar system is made up of materials that are rich in carbon’, he said.
This dichotomy ‘was really a surprise when it was first found,’ Dr Mojzsis added.
In the Rocky mountains, ‘the Great Divide causes water to drain one way or another,’ Mojzsis said. ‘It’s similar to how this pressure bump would have divided material’ in the solar system
However, he said the barrier in space was not perfect as some outer system material may have climbed across the divide.
He said that material is what would have been important to the evolution of Earth.
‘Those materials that might go to the Earth would be those volatile, carbon-rich materials,’ Dr Mojzsis said. ‘And that gives you water. It gives you organics.’
He said those lead to water and ‘the rest is Earth history’.
Many scientists assumed that Jupiter was responsible for the higher carbon levels found in the outer solar system, according to Dr Mojzsis.
The ‘great divide’ in the Solar System that splits inner rocky planets from outer gas giants was caused by a ‘ring around the Sun’, scientists claim
The thinking went that the planet is so massive that it may have acted as a gravitational barrier, preventing pebbles and dust from the outer solar system from spiraling toward the sun, he said.
They were able to dispute this theory using computer simulations that explored Jupiter’s role in the evolving solar system.
They found that while Jupiter is big, it was probably never big enough early in its formation to entirely block the flow of rocky material from moving sunward.
This led to their discovery of the ‘Great Barrier’ likely formed alongside the rest of the solar system out of that early protoplanetary disc.
The research has been published in the journal Nature Astronomy.
WHAT ARE PROTOPLANETARY DISCS?
A protoplanetary disc is a ring of gas and dust surrounding an early star and likely formed around the Sun in the earliest years of the solar system.
Dust grains collide and stick together, growing in size, and eventually forming rocky ‘planet embryos’ that may later accumulate the gas around them
The rings around a star are the early stages in the creation of planetary systems – something that happens around most stars, astronomers say.
Dust grains collide and stick together, growing in size, and eventually forming rocky ‘planet embryos’ that may later accumulate the gas around them.
New research suggests those discs also left behind a barrier in the solar system marking a divide between planetary types.
The divide was likely caused by bands of high and low pressure within the disc splitting material into two distinct camps, one forming Jupiter and the outer planets, the other Earth and the inner planets.
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