Earth had Saturn-like rings 466 million years ago, new study suggests
The temporary structure likely consisted of debris from a broken-up asteroid.
Earth may have sported a Saturn-like ring system 466 million years ago, after it captured and wrecked a passing asteroid, a new study suggests.
The debris ring, which likely lasted tens of millions of years, may have led to global cooling and even contributed to the coldest period on Earth in the past 500 million years.
That's according to a fresh analysis of 21 crater sites around the world that researchers suspect were all created by falling debris from a large asteroid between 488 million and 443 million years ago, an era in Earth's history known as the Ordovician during which our planet witnessed dramatically increased asteroid impacts.
A team led by Andy Tomkins, a professor of planetary science at Monash University in Australia, used computer models of how our planet's tectonic plates moved in the past to map out where the craters were when they first formed over 400 million years ago. The team found that all the craters had formed on continents that floated within 30 degrees of the equator, suggesting they were created by the falling debris of a single large asteroid that broke up after a near-miss with Earth.
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"Under normal circumstances, asteroids hitting Earth can hit at any latitude, at random, as we see in craters on the moon, Mars and Mercury," Tomkins wrote in The Conversation. "So it's extremely unlikely that all 21 craters from this period would form close to the equator if they were unrelated to one another."
The chain of crater locations all hugging the equator are consistent with a debris ring orbiting Earth, scientists say. That's because such rings typically form above planets' equators, as occurs with those circling Saturn, Jupiter, Uranus and Neptune. The chances that these impact sites were created by unrelated, random asteroid strikes is about 1 in 25 million, the new study found.
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The researchers estimate that the ring-spawning asteroid would be about 7.7 miles (12.5 kilometers) wide if it were a "rubble pile," or slightly smaller if it were a solid body. Once it shattered after nearing Earth's vicinity, its fragments would have "jostled around" before settling into a debris ring orbiting Earth's equator, Tomkins said.
"Over millions of years, material from this ring gradually fell to Earth, creating the spike in meteorite impacts observed in the geological record," Tomkins added in a university statement. "We also see that layers in sedimentary rocks from this period contain extraordinary amounts of meteorite debris."
The team found that this debris, which represented a specific type of meteorite and was found to be abundant in limestone deposits across Europe, Russia and China, had been exposed to a lot less space radiation than meteorites that fall today. Those deposits also reveal signatures of multiple tsunamis during the Ordovician period, all of which can be best explained by a large, passing asteroid capture-and-break-up scenario, the researchers argue.
The new study is a "new and creative idea that explains some observations," Birger Schmitz of Lund University in Sweden told New Scientist. "But the data are not yet sufficient to say that the Earth indeed had rings."
Searching for a common signature in specific asteroids grains across the newly studied impact craters would help test the hypothesis, Schmitz added.
If Earth did sport a Saturn-like ring around its equator, the ring would have significantly affected our planet's climate, according to the new study. Because Earth's axis is tilted relative to its orbit around the sun, the ring would have cast a shadow over parts of our planet's surface that may have caused global cooling. But the specifics are still murky, the researchers say.
The researchers speculate that such an event may have contributed to the dramatic cooling of our planet 465 million years ago, which led to the coldest period in the past half a billion years, known as the Hirnantian Ice Age.
"We don't know how the ring would have looked from Earth or how much light it would have cut out or how much debris there would have had to be in the ring to lower the temperature on Earth," Tomkins told New Scientist.
This research is described in a paper published Monday (Sept. 16) in the journal Earth and Planetary Science Letters.
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Sharmila Kuthunur is a Seattle-based science journalist covering astronomy, astrophysics and space exploration. Follow her on X @skuthunur.
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Classical Motion 466 million years is recent. And short. Could such structure exist with the tide of the moon? Was the tide any stronger at that time? Was the moon always locked?Reply
I’m guessing to be wrecked up and out there, the rock would have to be soft, or a sand pile. Not much to reach the surface. No large impacts.
There might be other factors and reasons for the locations of the studied impacts.
It might take 466 million years just to establish a ring.
Are rings caught and aligned, or are rings spewed out? -
Torbjorn Larsson Classical Motion said:Could such structure exist with the tide of the moon? Was the tide any stronger at that time?The Earth-Moon Roche limit, according to NASA, is about 19,900 km
Even at the closest point in its orbit, the Moon is 363,104 km
https://www.skyatnightmagazine.com/space-science/roche-limit
So the Moon is 20 times further out. Even Saturn have long term rings despite large moons et cetera, but these became just 30 million years old (see the paper). The rest of your questions should be covered by the paper's model. -
Unclear Engineer Why does it have to have been a "ring" of tiny particles? They don't leave impact craters, anyway. Another scenario would be that an asteroid broke into pieces when it came within the Roche limit, but those pieces orbited multiple times before individually impacting Earth. Jupiter did that to a comet not long ago.Reply
The "ice age" may or may not be related. If there was enough ejecta from the impacts, would we have had cooling effects from dust thrown into the atmosphere by the impacts? Could that have been a "tipping point" in Earth's climate balance, rather than a sustained cooling by the dust?
Finding a lot of craters 400,000,000 million years old suggests to me that they must have been substantial impacts to have produced evidence that survived Earth's weathering processes for that length of time. And, those are just the ones that hit the continents - how many hit the oceans?
For that matter, why would it have to be an "asteroid"? Why not a second, smaller moon that was created at the same time as the Moon we all know, love, and want to get back to? Maybe that second moon's orbit slowly lowered while the Moon of today's orbit slowly rose, as is currently happening with the 2 moons of Mars? When the smaller, lower moon finally got within the Roche limit, it broke apart and eventually led to multiple impacts, maybe with a ring.
Just because a theory might fit the sparse data does not make it a sure thing.