In
the early 1960s, Brian Harland, a geologist at Cambridge University, observed
that rocks on several continents, dating from the Neoproterozoic era
(approximately 800–680 million years ago), contain glacial debris. Some of the
glacial debris included carbonate rocks, which are known to form in the tropics
(e.g., in the presentday Bahama Banks). This conclusion later gained additional
support from paleomagnetic data. One potential explanation is that the entire
Earth was covered by ice and snow during the Neoproterozoic. This is known as
the “snowball Earth” hypothesis.
One
early problem was understanding how a global ice age could have commenced.
During the 1960s, the Russian climate scientist Mikhail Budyko used a computer
simulation to establish that a runaway ice-albedo feedback effect could lead to
global glaciation. The term albedo refers to the amount of
the sun’s energy that is reflected by the Earth’s surface. As glaciers grow in
extent, they reflect more of the sun’s energy, which causes the atmosphere to
cool. This in turn causes the glaciers to grow. Budyko showed that if the
glaciers extended beyond a certain critical point, this ice-albedo feedback
could lead to a global ice age.
A
second obstacle was understanding how a global ice age could ever end once it
began. In the early 1990s, Joseph Kirschvink of the California Institute of
Technology observed that during a global ice age, the carbon cycle would shut
down. Volcanoes sticking up through the ice cover would continue to add carbon
dioxide to the atmosphere. Having nowhere else to go, the carbon dioxide would
then accumulate over millions of years until a runaway greenhouse effect caused
the ice to melt. One important rival to the snowball Earth hypothesis is the
high obliquity hypothesis. If the tilt of the Earth’s axis had been much
different during the Neoproterozoic, the poles could have received more solar
energy than the tropics. If so, it would be possible to explain the evidence
for glaciers in the tropics, without supposing that the entire planet had
frozen over.
In
his widely cited 1992 paper, Kirschvink also proposed an explanation for banded
iron deposits observed
in Neoproterozoic glacial debris. Iron is not soluble in seawater in the
presence of oxygen. During
a true snowball Earth episode, the oceans would have become deoxygenated over
time. Iron from
thermal vents would build up in the seawater. Then, when the ice finally melted
and oxygen was
once again exchanged between the oceans and atmosphere, oxidized iron would
have been left
along with the debris from the retreating glaciers.
During
the 1990s, two Harvard scientists, Paul Hoffman and Daniel Shrag, gathered
additional, highly suggestive evidence that seemed to favor the snowball Earth
theory. They found that in many places, the Neoproterozoic glacial debris
occurs right below thick layers of carbonate rock (which are known as “cap
carbonates”), and they showed how Kirschvink’s proposal could account for this.
During a snowball Earth episode, very large amounts of carbon dioxide would
have built up in the atmosphere. As the ice receded and the carbon cycle
resumed, large amounts of carbon would have been washed out of the atmosphere
during storms and ended up in the form of carbonate rock on the ocean floor.
More controversially, Hoffman and Shrag also studied the ratio of carbon-12 to
carbon-13 isotopes in the cap carbonates. They argued that an unusual dip in
the carbon isotope ratio signified a temporary shutdown of photosynthetic
activity in the Earth’s oceans.
Challenges
to the Snowball Earth Theory
One
potentially serious challenge to the snowball Earth theory comes from
paleontology. Today, most
geologists agree that there were at least two major ice ages during the
Neoproterozoic: the Sturtian, around 750 million years ago, and the Varanger,
around 590 million years ago. The second of these episodes occurred shortly
before the Cambrian explosion of metazoan life. However, a true snowball Earth
episode would have killed off nearly all eukaryotic life, and it is not clear
that there was enough evolutionary time for life to recover from a global ice
age. Some scientists have used computer models to show that softer versions of
the snowball Earth episode might have been possible—for example, a mostly ice-covered
planet with massive continental ice sheets in the tropics, but largely ice-free
tropical oceans.
Although
scientists generally agree that there was low-latitude glaciation during the
Neoproterozoic, they
continue to use a combination of fieldwork and numerical modeling techniques to
work out the details. The snowball Earth scenario remains an intriguing live
hypothesis.
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