Explaining Dramatic Planetwide Changes After The Last Snowball Earth Event
Some of the most dramatic climatic events in our planet’s history are “Snowball Earth” events that happened hundreds of millions of years ago, when almost the entire planet was encased in ice up to 0.6 miles (1 kilometer) thick.
These “Snowball Earth” events have happened only a handful of times and do not occur on regular cycles. Each lasts for millions of years or tens of millions of years and is followed by dramatic warming, but the details of these transitions are poorly understood.
New research from the University of Washington provides a more complete picture for how the last Snowball Earth ended, and suggests why it preceded a dramatic expansion of life on Earth, including the emergence of the first animals.
The study recently published in Nature Communications focuses on ancient rocks known as “cap carbonates,” thought to have formed as the glacial ice thawed. These rocks preserve clues to Earth’s atmosphere and oceans about 640 million years ago, far earlier than what ice cores or tree rings can record.
These panels show the new theory for the three phases that ended the Snowball Earth event. In the first stage, thick ice sheets separate most of the atmosphere and ocean. In the second stage, freshwater flows into the ocean to join meltwater floating on the ocean’s surface. In the final stage, ocean mixing resumes, allowing exchanges between the atmosphere, upper ocean and deep ocean.Thomas et al./Nature Communications
“Cap carbonates contain information about key properties of Earth’s atmosphere and ocean, such as changing levels of carbon dioxide in the air, or the acidity of the ocean,” said lead author Trent Thomas, a UW doctoral student in Earth and space sciences. “Our theory now shows how these properties changed during and after Snowball Earth.”
Cap carbonates are layered limestone or dolomite rocks that have a distinct chemical makeup and today are found in over 50 global locations, including Death Valley, Namibia, Siberia, Ireland and Australia. These rocks are thought to have formed as the Earth-encircling ice sheets melted, causing dramatic changes in atmospheric and ocean chemistry and depositing this unique type of sediment onto the ocean floor.
They are called “caps” because they are the caps above glacial deposits left after Snowball Earth, and “carbonates” because both limestone and dolomite are carbon-containing rocks. Understanding their formation helps explain the carbon cycle during periods of dramatic climate change. The new study, which models the environmental changes, also provides hints about the evolution of life on Earth and why more complex lifeforms followed the last Snowball Earth.
“Life on Earth was simple — in the form of microbes, algae or other tiny aquatic organisms — for over 2 billion years leading up to Snowball Earth,” said senior author David Catling, a UW professor of Earth and space sciences. “In fact, the billion years leading up to Snowball Earth are called the ‘boring billion’ because so little happened. Then two Snowball Earth events occurred. And soon after, animals appear in the fossil record.”
A Measured 87Sr/86Sr offsets upsection in 5 cap carbonates. The red lines are the roughly inferred heights in the cap carbonate at which ocean stratification ends according to the mixing models of those who obtained and analyzed the data: Liu et al.28,29 (Mongolia), Liu et al.27 (Australia), and Wei et al.56 (Namibia, South China, and North China). Below the red lines, the cap carbonates were precipitated out of mostly glacial meltwater with elevated, continentally influenced 87Sr/86Sr. Above these lines, the cap carbonates were precipitated out of mostly ocean water with lower, hydrothermally influenced 87Sr/86Sr. B Model predictions for the height at which ocean stratification ends in the baseline scenario. These are effectively predictions for where the red lines should be. Results assuming tstrat = 104 years are on the left in blue, and assuming tstrat = 105 years are on the right in green. The filled squares are the median model predictions and the error bars are the 95% confidence interval corresponding to Fig. 5. — Computational simulation/modeling
The new paper provides a framework for how the last two facts may be connected.
The study modeled chemistry and geology during three phases of Snowball Earth. First, during Snowball Earth’s peak, thick ice encircling the planet reflected sunlight, but some areas of open water allowed exchange between the ocean and atmosphere. Meanwhile frigid seawater continued to react with the ocean floor.
Eventually, carbon dioxide built up in the atmosphere to the point where it trapped enough solar energy to raise global temperatures and melt the ice. This let rainfall reach the Earth, and let freshwater flow into the ocean to join a layer of glacial meltwater that floated over the denser, salty ocean water. This layered ocean slowed down ocean circulation. Later, ocean churning picked up, and mixing between the atmosphere, upper ocean, and deep ocean resumed.
“We predict important changes in the environment as Earth recovered from the Snowball period, some of which affected the temperature, acidity and circulation of the ocean. Now that we know these changes, we can more confidently figure out how they affected Earth’s life,” Thomas said.
Future research will explore how pockets of life that may have survived the tumult of the Snowball Earth and its aftermath could have evolved into the more complex lifeforms that followed soon after.
The research was funded by the National Science Foundation and NASA, in part by a NASA Astrobiology Program grant to the UW’s Virtual Planetary Laboratory.
Three-stage formation of cap carbonates after Marinoan snowball glaciation consistent with depositional timescales and geochemistry, Computational simulation/modeling (open access)
Astrobiology
