The solar system may have passed through dense interstellar clouds 2 million years ago, altering Earth's climate (2024)

Around two million years ago, Earth was a very different place, with our early human ancestors living alongside saber-toothed tigers, mastodons, and enormous rodents. And, depending on where they were, they may have been cold: Earth had fallen into a deep freeze, with multiple ice ages coming and going until about 12,000 years ago. Scientists theorize that ice ages occur for a number of reasons, including the planet's tilt and rotation, shifting plate tectonics, volcanic eruptions, and carbon dioxide levels in the atmosphere. But what if drastic changes like these are not only a result of Earth's environment, but also the sun's location in the galaxy?

In a new paper published in Nature Astronomy, lead authorand astrophysicist Merav Opher -- an astronomy professor at Boston University and fellow at Harvard Radcliffe Institute -- found evidence that some two million years ago, the solar system encountered an interstellar cloud so dense that it could have interfered with the sun's solar wind. Opher and her co-authors believe this shows that the sun's location in space might shape Earth's history more than previously considered.

Our whole solar system is swathed in a protective plasma shield that emanates from the sun, known as the heliosphere. It's made from a constant flow of charged particles, called solar wind, that stretch well past Pluto, wrapping the planets in what NASA calls a "a giant bubble." It protects us from radiation and galactic rays that could alter DNA, and scientists believe it's part of the reason life evolved on Earth as it did. According to the latest paper, the cold cloud compressed the heliosphere in such a way that it briefly placed Earth and the other planets in the solar system outside of the heliosphere's influence.

"This paper is the first to quantitatively show there was an encounter between the sun and something outside of the solar system that would have affected Earth's climate," says Opher, who is an expert on the heliosphere. Her models have quite literally shaped our scientific understanding of the heliosphere, and how the bubble is structured by the solar wind pushing up against the interstellar medium -- which is the space in between stars and beyond the heliosphere in our galaxy. Her theory is that the heliosphere is shaped like a puffy croissant, an idea that shook the space physics community. Now, she's shedding new light on how the heliosphere, and where the sun moves through space, could affect Earth's atmospheric chemistry.

"Stars move, and now this paper is showing not only that they move, but they encounter drastic changes," says Opher. She first discovered and began working on this study during a yearlong fellowship at Harvard Radcliffe Institute.

To study this phenomenon, Opher and her collaborators essentially looked back in time, using sophisticated computer models to visualize where the sun was positioned two million years in the past -- and, with it, the heliosphere, and the rest of the solar system. They also mapped the path of the Local Ribbon of Cold Clouds system, a string of large, dense, very cold clouds mostly made of hydrogen atoms. Their simulations showed that one of the clouds close to the end of that ribbon, named the Local Lynx of Cold Cloud, could have collided with the heliosphere.

If that had happened, says Opher, Earth would have been fully exposed to the interstellar medium, where gas and dust mix with the leftover atomic elements of exploded stars, including iron and plutonium. Normally, the heliosphere filters out most of these radioactive particles. But without protection, they can easily reach Earth. According to the paper, this aligns with geological evidence that shows increased 60Fe (iron 60) and 244Pu (plutonium 244) isotopes in the ocean, on the moon, Antarctic snow, and ice cores from the same time period. The timing also matches with temperature records that indicate a cooling period.

"Only rarely does our cosmic neighborhood beyond the solar system affect life on Earth," says Avi Loeb, director of Harvard University's Institute for Theory and Computation and coauthor on the paper. "It is exciting to discover that our passage through dense clouds a few million years ago could have exposed the Earth to a much larger flux of cosmic rays and hydrogen atoms. Our results open a new window into the relationship between the evolution of life on Earth and our cosmic neighborhood."

The outside pressure from the Local Lynx of Cold Cloud could have continually blocked out the heliosphere for a couple of hundred years to a million years, Opher says -- depending on the size of the cloud. "But as soon as the Earth was away from the cold cloud, the heliosphere engulfed all the planets, including Earth," she says. And that's how it is today.

It's impossible to know the exact effect the cold clouds had on Earth -- like if it could have spurred an ice age. But there are a couple of other cold clouds in the interstellar medium that the sun has likely encountered in the billions of years since it was born, Opher says. And it will likely stumble across more in another million years or so. Opher and her collaborators are now working to trace where the sun was seven million years ago, and even further back. Pinpointing the location of the sun millions of years in the past, as well as the cold cloud system, is possible with data collected by the European Space Agency's Gaia mission, which is building the largest 3D map of the galaxy and giving an unprecedented look at the speed stars move.

"This cloud was indeed in our past, and if we crossed something that massive, we were exposed to the interstellar medium," Opher says. The effect of crossing paths with so much hydrogen and radioactive material is unclear, so Opher and her team at BU's NASA-funded SHIELD (Solar wind with Hydrogen Ion Exchange and Large-scale Dynamics) DRIVE Science Center are now exploring the effect it could have had on Earth's radiation, as well as the atmosphere and climate.

"This is only the beginning," Opher says. She hopes that this paper will open the door to much more exploration of how the solar system was influenced by outside forces in the deep past and how these forces have in turn shaped life on our planet.

This research was supported by NASA.

The solar system may have passed through dense interstellar clouds 2 million years ago, altering Earth's climate (2024)

FAQs

The solar system may have passed through dense interstellar clouds 2 million years ago, altering Earth's climate? ›

Researchers have found evidence suggesting we have traversed denser regions in the past, the study revealed. "In the ISM that the Sun has traversed for the last couple of million years, there are cold, compact clouds that could have drastically affected the heliosphere," the team explained in the study.

What is the interstellar cloud theory of the solar system? ›

This team thinks that it is possible a cold cloud of interstellar material could have once stymied the solar wind in such a way that the heliosphere was compressed. This might have, for a short period (in cosmic terms), removed Earth and other solar system planets from the protection offered by the heliosphere.

What may have caused the cloud that became our solar system to collapse? ›

Our solar system formed about 4.5 billion years ago from a dense cloud of interstellar gas and dust. The cloud collapsed, possibly due to the shockwave of a nearby exploding star, called a supernova.

Did the solar system form from an interstellar cloud of dust and gas or nebula about 4.6 billion years ago? ›

The Sun and the planets formed together, 4.6 billion years ago, from a cloud of gas and dust called the solar nebula. A shock wave from a nearby supernova explosion probably initiated the collapse of the solar nebula. The Sun formed in the center, and the planets formed in a thin disk orbiting around it.

What if the solar system passed through a cloud of gas and dust? ›

Our solar system would stay in place as it passed through a cloud of the density typical for interstellar dust clouds, but the passage of the Sun would, to a high degree of probability, set up eddies in the cloud which would then condense into new stars.

What happens when an interstellar cloud collapses? ›

A Star is BornA Star is Born. Summary: Stars form in cold, dense regions of space called molecular clouds. When the force of gravity pulling in on the cloud is greater than the strength of internal pressure pushing out, the cloud collapses into a protostar.

How long do interstellar clouds last? ›

Interstellar clouds can be large, up to 106 solar masses, and are often said to be the most massive entities in the galaxy. In this form, they may have a lifetime of more than 108 years. They are presumably dissipated as a result of pressure from stars formed within the clouds.

How will our solar system likely be destroyed? ›

Our planet will be swallowed by our expanding sun, according to researchers from the University of Warwick. Meanwhile, other planets in the solar system will be 'crushed and ground to dust'. Thankfully, there's no need to panic just yet, as the scientists say this will likely happen in around six billion years.

What will happen to Earth when the Sun collapses? ›

It'll swell into a red giant, whose outer layers will engulf Mercury and Venus and likely reach the Earth. Life on Earth will end. If the sun were more massive – estimates vary, but at least several times more massive – it would explode as a supernova.

What event can lead to the gravitational collapse of an interstellar cloud? ›

Helping factors: The main one is gravity; Collapse can possibly be triggered by shock waves from events like supernova explosions (or galaxy collisions, and possibly large "objects" such as globular clusters passing by), which can start a chain reaction.

What is the theory that the solar system developed from a cloud of dust and gas? ›

The nebular hypothesis is the idea that a spinning cloud of dust made of mostly light elements, called a nebula, flattened into a protoplanetary disk, and became a solar system consisting of a star with orbiting planets [ 12 ].

What two things started Earth? ›

The Earth formed over 4.6 billion years ago out of a mixture of dust and gas around the young sun. It grew larger thanks to countless collisions between dust particles, asteroids, and other growing planets, including one last giant impact that threw enough rock, gas, and dust into space to form the moon.

Where did the dense cloud of interstellar gas and dust come from? ›

An interstellar cloud is formed by the gas and dust particles from a red giant in its later life. A small part of the emission nebula NGC 6357.

What does an interstellar cloud have to do with our solar system? ›

But between two million and three million years ago, the researchers posit that an interstellar cloud compressed the heliosphere, temporarily leaving much of the solar system, including Earth, vulnerable.

What caused the sun to form an interstellar gas and dust cloud? ›

Gravitational collapse

This was possibly because of a nearby supernova - an exploding star - sending shock waves rippling through space. Gravity then caused dust and gas to be continually tugged to the centre of the cloud, making its core very hot and dense.

What theory is interstellar based on? ›

Compared to Earth, space-time on Miller's planet has been warped, hence why the crew say they must “think of time as a resource, just like food or oxygen”. Einstein's theory of relativity is key to all this. His revolutionary 1915 theory proposed that the larger the object, the more spacetime is warped and twisted.

What is the solar cloud theory? ›

Currently the best theory is the Nebular Theory . This states that the solar system developed out of an interstellar cloud of dust and gas, called a nebula . This theory best accounts for the objects we currently find in the Solar System and the distribution of these objects.

What is the cloud in interstellar space? ›

An interstellar cloud is formed by the gas and dust particles from a red giant in its later life. A small part of the emission nebula NGC 6357. It glows with the characteristic red of an H II region.

What is an interstellar object in our solar system? ›

'Oumuamua is the first confirmed object from another star to visit our solar system. This interstellar interloper appears to be a rocky, cigar-shaped object with a somewhat reddish hue. The object was named 'Oumuamua by its discoverers. It means "a messenger from afar arriving first" in Hawaiian.

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