The Hirnantian glaciation, also known as the Andean-Saharan glaciation, Early Paleozoic Ice Age (EPIA), the Early Paleozoic Icehouse, the Late Ordovician glaciation, or the end-Ordovician glaciation, occurred during the Paleozoic from around 460 to 420 million years ago. The major glaciation during this period was formerly thought only to consist of the Hirnantian glaciation itself but has now been recognized as a longer, more gradual event, which began as early as the Darriwilian, and possibly even the Floian. Evidence of this glaciation can be seen in places such as Arabia, North Africa, South Africa, Brazil, Peru, Bolivia, Chile, Argentina, and Wyoming. More evidence derived from isotopic data is that during the Late Ordovician, tropical ocean temperatures were about 5 °C cooler than present day; this would have been a major factor that aided in the glaciation process.
Cold temperatures are widely considered to be the leading cause of the Late Ordovician mass extinction, and it is the only glacial episode that appears to have coincided with a major mass extinction of nearly 61% of marine life. Estimates of peak ice sheet volume range from 50 to 250 million cubic kilometres, and its duration from 35 million to less than 1 million years. At its height during the Hirnantian, the ice age is believed to have been significantly more extreme than the Last Glacial Maximum occurring during the terminal Pleistocene. Glaciation of the Northern Hemisphere was minimal because a large amount of the land was in the Southern Hemisphere.
Timeline Pre-Hirnantian glaciations The earliest evidence for possible glaciation comes from Floian conodont apatite oxygen isotope fluctuations, which display a periodicity characteristic of Milankovitch cycles and have been interpreted as reflecting cyclic waxing and waning of polar ice caps. A speculated glaciation in the middle Darriwilian corresponds to the MDICE positive carbon isotope excursion. Sea level changes likely reflective of glacioeustasy are known from this geologic stage, around 467 million years ago. However, there are no known Middle Ordovician glacial deposits that would provide direct geological evidence of glaciation. Isotopic evidence from the Sandbian reveals three possible glaciations: an early Sandbian glaciation, a middle Sandbian glaciation, a late Sandbian glaciation. Although biostratigraphy dating the glacial deposits in Gondwana has been problematic, there is evidence suggesting the presence of glaciation by the Sandbian stage. Graptolite distribution during the time interval delineated by the Nemacanthus gracilis graptolite biozone indicates a latitudinal extent of the subtropics and tropics similar to that of today, as evidenced by a steep faunal gradient that is uncharacteristic of greenhouse periods, suggesting that Earth was in a mild icehouse state by the start of the Sandbian, around 460 million years ago. Many possible short glaciation occurred during the Katian: three very short glaciations during the early Katian, the Rakvere glaciation during the late early Katian, a middle Katian glaciation, the Early Ashgill glaciation of the early late Katian, and a latest Katian glaciation that was followed by a rapid warming event in the Paraorthograptus pacificus graptolite biozone immediately before the Hirnantian glaciation itself. Evidence of major changes in bottom water formation, which usually indicates a sudden change in global climate, is known from the Katian. Shifts in isotopic ratios of carbon and neodymium that correspond to graptolite biostratigraphy lend further evidence in favour of the existence of glacioeustatic cycles during the Katian, as do conodont apatite δ18O fluctuations from Kentucky and Quebec that likely reflect glacioeustatic sea level changes. However, the existence of glacials during the Katian remains controversial. Katian brachiopod and seawater δ18O values from Cincinnati Arch indicate ocean temperatures characteristic of a global greenhouse state.
Hirnantian glaciation
At the Katian-Hirnantian boundary, a sudden cooling event caused a rapid expansion of glaciers, resulting in one of the most severe glaciations of the Phanerozoic, an extreme cooling event generally believed to be coincident with the first pulse of the Late Ordovician mass extinction. An δ18O shift occurs at the start of the Hirnantian; the magnitude of this shift (+2-4‰) was extraordinary. Its direction implies glacial cooling and possibly increases in ice-volume. The observed shifts in the δ18O isotopic indicator would require a sea-level fall of 100 meters and a drop of 10 °C in tropical ocean temperatures to have occurred during this glacial episode. Sedimentological data shows that Late Ordovician ice sheets glacierized the Al Kufrah Basin. Ice sheets also probably formed continuous ice cover over North Africa and the Arabian Peninsula. In all areas of North Africa where Early Silurian shale occurs, Late Ordovician glaciogenic deposits occur beneath, likely due to the anoxia promoted in these basins.
At the end of the Hirnantian, an abrupt retreat of glaciers concurrent with the second pulse of the Late Ordovician mass extinction occurred, after which Earth receded back into a much warmer climate during the Rhuddanian. Late Hirnantian warming was marked by a similarly meteoric shift in δ18O towards more negative values. δ13C values likewise fall sharply at the beginning of the Silurian.
Silurian glaciations Following the relatively warm Rhuddanian, glacial events occurred during the early and latest Aeronian. A further glaciation occurred from the late Telychian to middle Sheinwoodian. From the early to late Homerian, Earth was in yet another glacial phase. The last major glaciation of the EPIA occurred during the Ludfordian and was associated with the Lau event.
During this period, glaciation is known from Arabia, Sahara, West Africa, the south Amazon, and the Andes, and the centre of glaciation is known to have migrated from the Sahara in the Ordovician (450–440 Mya) to South America in the Silurian (440–420 Mya). According to Eyles and Young, "A major glacial episode at c. 440 Ma, is recorded in Late Ordovician strata (predominantly Ashgillian) in West Africa (Tamadjert Formation of the Sahara), in Morocco (Tindouf Basin) and in west-central Saudi Arabia, all areas at polar latitudes at the time. From the Late Ordovician to the Early Silurian the centre of glaciation moved from northern Africa to southwestern South America." Continental glaciers developed in Africa and eastern Brazil, while alpine glaciers formed in the Andes. In western South America (Peru, Bolivia and northern Argentina) were found glacio-marine diamictites interbedded with turbidites, shales, mud flows and debris flows, dated as early Silurian (Llandonvery), with a southward extension into northern Argentina and western Paraguay, and with a probably northern extension into Peru, Ecuador and Colombia.
A major ice age, the Andean-Saharan was preceded by the Baykonurian glaciation, often referred to as a Snowball Earth, and followed by the Late Paleozoic icehouse.
Evidence Lithologic The sequence of the stratigraphic architecture of the Bighorn Dolomite (which represents end of the Ordovician period), is consistent with the gradual buildup of glacial ice. The sequences of the Bighorn Dolomite display systematic changes in their component cycles, and the changes in these cycles are interpreted as being a change from a greenhouse climate to a transitional ice house climate.
Possible causes
Carbon dioxide depletion One of the factors that hindered glaciation during the early Paleozoic was atmospheric Carbon dioxide concentrations, which at the time were somewhere between 8 and 20 times pre-industrial levels. However, solar irradiance was significantly lower during the Late Ordovician; 450 million years ago, solar irradiance of Earth was about 1,312 Wm−2 compared to 1,360.89 Wm−2 in the present day. Furthermore, Carbon dioxide concentrations are thought to have dropped significantly during the Hirnantian, which could have induced widespread glaciation during an overall cooling trend. Methods for the removal of Carbon dioxide during this time were not well known, and are still hotly debated, with the radiation of terrestrial plants, enhanced oceanic organic carbon burial, and a reduction in volcanic outgassing of carbon dioxide having been proposed. It could have been possible for glaciation to initiate with high levels of Carbon dioxide, but it would have depended highly on continental configuration.
Silicate weathering Long-term silicate weathering is a major mechanism through which Carbon dioxide is removed from the atmosphere, converting it into bicarbonate which is stored in marine sediments. This has often been linked to the Taconic Orogeny, a mountain-building event on the east coast of Laurentia (present-day North America). Another hypothesis is that a hypothetical large igneous province in the Katian led to basaltic flooding caused by high continental volcanic activity during that period. In the short term, this would have released a large amount of Carbon dioxide into the atmosphere, which may explain a warming pulse in the Katian. However, in the long term flood basalts would have left behind plains of basaltic rock, replacing exposures of granitic rock. Basaltic rocks weather substantially faster than granitic rocks, which would quickly remove Carbon dioxide from the atmosphere at a much faster rate than before the volcanic activity. Carbon dioxide levels could also have decreased due to accelerated silicate weathering caused by the expansion of terrestrial non-vascular plants. Vascular plants only appeared 15 million years after the glaciation.
Organic carbon burial Isotopic evidence points to a global Hirnantian positive shift in δ13C at nearly the same time as the positive shift in marine carbonate δ18O. This shift is known as the Hirnantian Isotopic Carbon Excursion (HICE). The positive shift in δ13C implies a change in the carbon cycle leading to more burial of organic carbon, though some researchers hold a conflicting interpretation of this δ13C change as being caused by increased weathering of carbonate platforms exposed by sea level fall. This enhanced organic carbon burial resulted in a decrease in the atmospheric Carbon dioxide levels and an inverse greenhouse effect, allowing glaciation to occur more readily.
Gamma-ray burst A gamma-ray burst (GRB) has been suggested by some researchers as the cause of the abrupt glaciation at the beginning of the Hirnantian. The effects of a ten second GRB occurring within two kiloparsecs of Earth would have delivered it a fluence of 100 kilojoules per square metre. This would have resulted in large amounts of nitric acid raining down on Earth's surface in the aftermath of the gamma-ray burst, causing blooms of nitrate-limited photosynthesisers that would have sequestered large amounts of carbon dioxide from the atmosphere. Additionally, the GRB would have initiated a major depletion of ozone, another potent greenhouse gas, through its reaction with nitric oxide produced as a result of the GRB's dissociation of diatomic nitrogen and subsequent reaction of nitrogen atoms with oxygen.
Asteroid impact Ordovician meteor event The breakup of the L-chondrite parent body caused a rain of extraterrestrial material onto the Earth called the Ordovician meteor event. This event increased stratospheric dust by 3 or 4 orders of magnitude and may have triggered the ice age by reflecting sunlight back into space.
Deniliquin impact structure A 2023 paper has proposed that the Hirnantian glaciation could have come about due to an impact winter generated by the impact that formed the Deniliquin multiple-ring feature in what is now southeastern Australia, although this hypothesis currently remains untested.
Debris ring