Cryogenian Period

Snowball Earth, two low-latitude glaciations and the persistence of life from about 720 to 635 million years ago.

Glaciers and sea ice along a low-latitude Cryogenian coast
A low-latitude Cryogenian coast with grounded ice and leads through sea ice. Ice extent is evidence-based; the exact coastline and weather are reconstructed.

The Cryogenian Period lasted from about 720 to 635 million years ago. It was the middle period of the Neoproterozoic Era, following the Tonian and ending before the Ediacaran. Its name refers to the birth of ice, and its defining history includes the Sturtian and Marinoan glaciations, two of the most extensive ice ages known from the late Precambrian.

The phrase “Snowball Earth” suggests a motionless white planet, but the geological hypothesis is more precise and more complicated. Rocks show that glaciers reached the sea at very low latitudes. They do not provide a photograph of every ocean surface, the thickness of sea ice or the area of open water. The global reach of glaciation and the exact architecture of the frozen world must therefore be considered separately.

The Cryogenian was not one continuous ice age lasting 85 million years. A long interval of open seas, sediment accumulation and changing microbial and eukaryotic ecosystems separated the two great glaciations.

MeasureCryogenian record
PositionSecond period of the Neoproterozoic Era
BeginningAbout 720 million years ago
EndAbout 635 million years ago
DurationAbout 85 million years
Previous periodTonian
Next periodEdiacaran
Formal epochs and stagesNone yet approved
Lower boundaryTemporary calibrated age near 720 Ma; no ratified GSSP
Upper boundaryBase of the cap carbonate above Marinoan glacial deposits at Enorama Creek, South Australia
Major changesTwo low-latitude glaciations, Rodinia breakup, carbon-cycle disruption and a growing role for eukaryotic algae

The dates follow the international geological time scale. The rounded values 720 and 635 Ma help describe time but do not replace physical stratigraphic surfaces. The geological time scale explains the hierarchy of eons, eras and periods, while the Proterozoic guide places the Cryogenian in its longer setting.

Why the period is called Cryogenian

The name combines Greek roots meaning cold or ice and birth. It highlights the extraordinary distribution of glacial deposits. The international division was established in the late 1980s with other units of the numerical Precambrian scale.

The base was originally placed at 850 Ma. Improved dating later showed that the widespread Sturtian glaciation began much later, near 717 Ma. The old boundary left more than 100 million years without a comparable global glacial event inside an ostensibly ice-defined period. The International Commission on Stratigraphy therefore removed that boundary and provisionally moved the base to about 720 Ma.

Why the lower boundary has no golden spike

Most younger geological boundaries are tied to a Global Boundary Stratotype Section and Point, a physical level informally called a golden spike. No such reference has yet been ratified for the base of the Cryogenian. The working group seeks a horizon below the first widely correlatable evidence of Sturtian glaciation that can be recognised among continents.

Selection is difficult. Advancing ice eroded some older deposits. Basins around Rodinia accumulated different sediment. The first local glacial debris need not represent the same instant as a global climatic transition. Until a suitable reference is agreed, the official chart uses the calibrated age near 720 Ma.

The upper boundary is different. It is also the base of the Ediacaran Period and is fixed at Enorama Creek in the Flinders Ranges. There, the Nuccaleena Formation cap carbonate directly overlies diamictite of the Elatina Formation, recording the aftermath of Marinoan glaciation.

Glaciations are not formal epochs

The Cryogenian has no approved international epochs or stages. Sturtian and Marinoan designate major glacial episodes and associated rock packages, not two formal epochs. Their numerical limits continue to be refined.

IntervalApproximate timeWhat happened
Early Cryogenian before widespread ice720 to about 717 MaClimate approached a threshold while rifting and basalt weathering continued
Sturtian glaciationAbout 717–659 MaLow-latitude marine glaciers, diamictites, dropstones and renewed iron formations
Interglacial intervalAbout 659–645 MaOpen seas, cap carbonates, changing oxygen conditions and increasing eukaryotic signals
Marinoan glaciationApproximately 645–635 MaA second low-latitude glaciation, probably shorter than the Sturtian

These ranges are not four official boxes. The beginning of the Marinoan event is especially uncertain. High-precision ages from some basins permit a shorter duration than classic syntheses, and glacial sedimentation may not have begun simultaneously everywhere.

Before the first snowball: Rodinia breaks apart

At the opening of the Cryogenian, fragments of Rodinia were separating. Rifts, volcanic provinces and new marine basins developed, while many continental blocks occupied tropical latitudes. That geography mattered because warm, wet conditions accelerate chemical weathering of silicate rocks.

Silicate weathering ultimately transfers atmospheric carbon dioxide into carbonate minerals. Fresh basalt is particularly reactive. The enormous Franklin Large Igneous Province formed immediately before the Sturtian ice age, with precise ages around 719.9–718.6 Ma. Widespread glaciation followed near 717 Ma.

Timing does not prove one cause. Eruptions initially released carbon dioxide, while later weathering of broad basaltic uplands may have removed it. Models also consider continental breakup, runoff, the fainter young Sun and relatively low long-term volcanic carbon input. Cryogenian cooling probably emerged from interacting factors rather than a single eruption.

The rifting continued processes already under way in the Tonian Period. It changed coastlines, ocean circulation, nutrient supply and the area of shallow seas at the same time as climate moved toward instability.

The Sturtian glaciation

The Sturtian glaciation began near 717 Ma and ended around 659 Ma. Uranium-lead dates from volcanic minerals and rhenium-osmium dates from sediment differ slightly, but together imply roughly 55–58 million years of glacial conditions. That is far longer than any individual Quaternary glacial cycle.

Sturtian glacial deposits occur on ancient margins of Laurentia, Australia, South China, Africa and other blocks. Palaeomagnetic measurements place some depositional sites at low latitudes. The evidence is not merely for mountain glaciers near the equator: large ice masses reached sea level.

Layered Cryogenian marine sediment with a dropstone beneath diamictite
A large clast bends fine marine laminae after falling from floating ice. The poorly sorted diamictite above must still be tested against non-glacial origins.

How rocks record the presence of ice

Diamictite contains clasts of many sizes in a fine-grained matrix. It may form beneath or beside a glacier, but poorly sorted sediment can also be produced by landslides and debris flows. Geologists therefore seek a combination of evidence rather than treating every diamictite as proof of ice.

A stone released by an iceberg or ice shelf can deform thin seabed layers and then be buried by later sediment. Such a clast is called a dropstone. Larger surfaces may retain glacial grooves, while faceted and scratched cobbles occur within deposits. Palaeomagnetism estimates ancient latitude, and volcanic ash supplies minerals for radiometric dating.

No single feature draws a global map. The case becomes strong when sedimentary structures, numerical age and continental position agree independently.

What the Snowball Earth hypothesis claims

Ice reflects more sunlight than water or bare rock. If the ice edge advances sufficiently far toward the equator, cooling promotes more ice and the new ice increases planetary reflectivity. This positive feedback can push climate into a stable, extremely cold condition.

Extensive low-latitude glaciation is the secure geological conclusion. Reconstructing open water between glaciers and the thickness of sea ice is harder, so several model families remain in use.

ModelProposed ocean surfacePotential refuges
Hard snowballNearly continuous, locally very thick sea iceCracks, brine channels, thin ice, hydrothermal and subglacial settings
SlushballMuch of the ocean frozen but persistent open-water areas remainSunlit water and habitats at the ice edge
WaterbeltAn equatorial belt remains unfrozenA broad low-latitude refuge for photosynthesis
Dynamic sea glacierThick ice flows equatorward while margins and thickness changeTemporary leads, melt zones and exchange with the atmosphere

These are not four successive stages, and no one label has been proved for every interval. Sediment, isotopes, iron formations and climate physics test them. Even a globally ice-covered ocean could have had moving ice and temporary openings. Snowball does not require the same kilometre-thick lid from pole to pole.

Why iron formations returned

Large banded iron formations became rare through much of the middle Proterozoic but reappeared in several basins during Sturtian glaciation. Beneath extensive ice, deep water could lose oxygen and accumulate dissolved ferrous iron supplied by hydrothermal systems and sediment. When iron-rich water met an oxidant, iron minerals precipitated.

Folded banded iron formation of Cryogenian age
Red iron-rich and dark silica-rich layers record repeated changes in deposition. The folding happened later and is not a trace of moving Cryogenian ice.

Their return was once treated as almost direct proof of a sealed global ocean. Modern circulation and geochemical models allow more possibilities. Similar iron distribution can develop beneath partial ice cover when circulation, iron supply and oxidation zones are considered. The rocks record an unusual redox regime, but they do not measure the area of open water by themselves.

Life beneath the ice

Life was already billions of years old. Cryogenian oceans contained bacteria, archaea and varied single-celled eukaryotes. Photosynthetic organisms needed light and liquid water; aerobic organisms also required oxygen. A thick opaque lid lasting millions of years would have been a severe challenge, yet these lineages survived.

Possible shallow refuge for microbial life beneath sea ice
Light enters through fractured and comparatively thin ice above microbial mats. The location and size of such refuges cannot be observed directly in rocks.

Possible refuges include wind- or current-driven leads, thin dusty ice at low latitude, brine channels, meltwater ponds, ice margins where fresh and marine water mixed, hydrothermal systems independent of sunlight, and subglacial zones supplied with oxidants by meltwater.

Geochemistry from syn-glacial strata indicates that active nitrogen cycling, primary production and oxygen-bearing surface water persisted locally. This supports habitable patches more directly than an image of a wholly dead ocean. Modern Antarctic lakes and sea ice offer process analogues, not exact replicas of Cryogenian communities.

Between the two glaciations

Around 659 Ma, the Sturtian icehouse gave way to open seas. Carbonate beds accumulated above glacial sediment, sea level rose and intense weathering delivered dissolved matter and particles. On a commonly used chronology, the interglacial interval lasted about 14 million years, although local limits depend on the section.

Open shallow sea between the Sturtian and Marinoan glaciations
The barren shore and microbial mats are plausible. Greenish water only signals microscopic primary production, not visible plants or animals.

Molecular fossils in organic matter show increasing diversity of steranes associated with eukaryotic producers. A particularly marked shift toward algal plankton has been placed between the Sturtian and Marinoan glaciations. One proposal links it to phosphorus released by erosion and weathering of continents.

This signal does not mean algae suddenly originated. Eukaryotes were older, and biomarker abundance depends on producer ecology and preservation. The evidence instead suggests a change in marine food webs. Some shelf waters became more persistently oxygenated while deeper water often remained anoxic and rich in dissolved iron.

Were animals present?

Many molecular-clock analyses place the separation of major animal branches before the Ediacaran. Steroid molecules from some late Precambrian rocks were initially linked to sponges, but other organisms or altered organic matter can produce the same compounds or their precursors. A biomarker is not a fossil animal body.

No secure Cryogenian assemblage of large animals comparable with Ediacaran communities is known. Some late Cryogenian carbonaceous macrofossils are interpreted as algae or other eukaryotes. They matter to the history of complex life but do not justify adding sponges, worms or jellyfish to every icy sea.

Large, recognisable soft-bodied communities became characteristic in the following period. Mineralised skeletons and complex burrowing spread later still, especially during the Cambrian Period.

The Marinoan glaciation

The second great glaciation began approximately 645 Ma and ended near 635 Ma. Classic syntheses give it at least five and perhaps about ten million years. New high-precision geochronology from particular successions permits estimates of only a few million years. That difference is why the starting age should not be stated with false precision.

Marinoan diamictites and related marine deposits occur on many ancient continents. Palaeomagnetic evidence again places marine glaciers in tropical latitudes. Together with a near-synchronous end, this makes the Marinoan event the second major foundation of the Snowball Earth hypothesis.

Black shales within glacial deposits of the Nantuo Formation in South China preserve carbonaceous macrofossils interpreted as bottom-dwelling photosynthetic eukaryotes. Geochemistry indicates oxygen cycling in surface water above oxygen-poor depths. The site records liquid, illuminated habitat as glaciation waned, not one globally open ocean.

How Earth escaped the frozen state

Volcanoes continued to supply carbon dioxide during severe glaciation. Chemical weathering weakened on a cold, ice-covered surface, so the main long-term carbon sink slowed. Over millions of years, greenhouse gas could accumulate until warming overcame the high reflectivity of ice.

Melting marine ice and sediment runoff at the end of Marinoan glaciation
The reconstruction shows final retreat. Once melting began, dark water and bare rock absorbed more sunlight while runoff carried intense weathering products to the sea.

Once the ice margin retreated, feedback changed direction. Dark water absorbed sunlight, temperature rose and melting accelerated. Models permit a rapid climatic switch, but rapid may still mean thousands of years, and glaciers in different basins need not have vanished in one season.

Warming produced a humid greenhouse with intense weathering. Rivers carried calcium, magnesium, silica, phosphorus and alkalinity. Sea level rose, and a fresher meltwater layer may have spread above denser seawater. These processes prepared the unusual chemistry of cap carbonates.

Cap carbonates above glacial rocks

On several continents, pale dolostone or limestone lies directly above Marinoan diamictite. These relatively thin but laterally extensive cap beds can contain crystal fans, tube-like structures and unusually large wave ripples.

Pale cap carbonate resting above dark Marinoan diamictite
The field reconstruction emphasises the key relationship between poorly sorted glacial deposits and overlying carbonate. Real sections differ in thickness and structure.

An early model explained cap carbonates mainly through an enormous atmospheric carbon dioxide reservoir and rapid postglacial weathering. Modern calculations add exchange with oceanic crust, alkalinity stored in deep water, mixing of meltwater and seawater, and several phases of precipitation. Cap carbonates remain strong evidence of abrupt postglacial reorganisation, but no single mechanism explains every feature.

At Enorama Creek, the base of this cap marks the Ediacaran boundary. The end of the Cryogenian is therefore defined by a particular surface in rock, not by the last iceberg anywhere on Earth.

Observation, model and open question

ConfidenceCryogenian example
Direct observationDiamictites, dropstones, iron formations and overlying carbonates occur in dated sections
Multi-method inferenceGlaciers reached sea level at low latitude and the two major deglaciations were broadly synchronous among basins
Developed modelIce-albedo feedback intensified cooling and volcanic carbon dioxide helped terminate glaciation
Open questionHow continuous and thick sea ice was, and where persistent open-water refuges occurred
Disputed biological interpretationWhether animals already existed and which organisms produced certain steroid biomarkers

What changed after the Cryogenian

Animals did not fill the oceans immediately after Marinoan melting. The ocean remained chemically patchy, with oxygenated and anoxic water coexisting during early Ediacaran time. Cryogenian weathering and circulation changes may nevertheless have increased nutrient delivery, altered primary production and created new ecological opportunities.

Large soft-bodied organisms, directed movement and early mineralised constructions appeared during the Ediacaran. The Cambrian later brought diverse skeletons, active predators and deep sediment mixing. A connection between glaciation and these changes is plausible, but “ice created animals” is not an adequate causal explanation.

The Cryogenian world lacked dinosaurs, fish, trilobites, land plants, forests and soil animals. Land was rock, sand, volcanic terrain, ice and perhaps local microbial communities. Its principal actors were ice, water, atmospheric carbon, moving continents and microscopic life. Those forces helped shape the environmental foundation for the much later Palaeozoic Era.

Frequently asked questions

When was the Cryogenian Period?

The Cryogenian lasted from about 720 to 635 million years ago, roughly 85 million years. Its lower age remains temporary because no GSSP has yet been ratified for the base.

Was the whole Earth completely covered by ice?

Rocks demonstrate that glaciers reached sea level at low latitudes during two major glaciations. Whether sea ice was continuous and where open water persisted remain model-dependent questions.

How did life survive Cryogenian glaciation?

Liquid and habitable water could persist in leads, beneath thin ice, in brine channels, at ice margins and around hydrothermal systems. Geochemistry records local primary production and oxygenated water during glaciation.

Why did the Cryogenian end?

Volcanic carbon dioxide continued to accumulate while cold conditions weakened silicate weathering. Greenhouse warming began deglaciation, and lower surface reflectivity accelerated it. The formal boundary lies at the base of a cap carbonate in South Australia.