This article is more than 5 years old. 25 years ago two German hikers discovered the mummified corpse of a bronze-age man in the Ötztaler Alps, along the border of Austria and Italy. For archaeologists and for glaciologists, this was a unique discovery. Wounded by an arrow in the back the 45-year-old man had bled to death within minutes. The body was left at the site of the murder — perhaps the aggressors assumed that scavengers and time would erase all the evidences, but in the cold and dry climate at 11,480 ft above sea level the body begun to desiccate. Large scavengers didn’t venture in this desolate region, and only a few flies were able to deposits their eggs on the body — but they weren’t able to destroy it. During the next winter snow accumulated in the gully where the body laid and over the next decades and centuries the snow transformed slowly into ice, protecting and preserving the body. On September 19, 1991 two German tourists, Helmut and Erika Simon, accidentally discovered the body emerging from the ice near the Similaun Hut after a period of marked melting, which had been helped by the sunny weather. The prehistoric mummified corpse, soon known worldwide as “Ötzi” the Iceman, together with its unique set of tools and artifacts provided a unique opportunity for the study of a Copper-Age man. But the mummy provided also insights on the glaciers during a little known warm interval in the last 10.000 years. This phase is not documented by glacial sediments, eroded by later glacial advances, and is only recognizable by proxy data like changes in pollen diagrams or the radiometric ages of organic material formed during this time. During the last glacial maximum some 18,000 years ago the entire area of the Ötztaler Alps was almost completely ice-covered, and only narrow and steep arêtes and horns protruded from the sea of ice. In the area of the Similaun Hut sharp trim lines in a height varying from 10,000 ft to 11,100 ft divide the uppermost frost-shattered crests from the lower slopes, smoothed by glacial erosion. This trim line can also be recognized locally as marked weathering line that separates different oxidized reddish surfaces (as the bed rock consists of iron-rich gneiss and schist the rocks will become rusty over time). A second trim line is marked by an abrupt change in lichen diameter (from 100mm to 40mm) and density. The dating by lichenometry attributes this glacier expansion to the Little Ice Age (1600-1850), which generally corresponds to the maximum glacier expansion in the last 10,000 years. The mummy itself was dated by radiocarbon dating to 4,500+-30 and 4,580+-30yr before present (by convention before 1950), which corresponds to a calibrated age of 5,300-5,050 years. The sudden burial of the corpse in a permanent snow and ice cover indicates a significant climatic change followed by growing glaciers, lasting until recent times. This climatic change is supported also by some soil-evidence found in depression at an altitude of 9,850-10,500ft and dating to the same time the iceman died. Similar recent soils need at least 500 to 1,200 years to develop, suggesting that the climatic conditions on the site were for a long time relative favorable for biological and chemical activity until a relatively quick drop of temperatures. The iceman and his site reveal that between 9,000 and 5,000 years before present the Alpine glaciers were smaller than in the second half of the Holocene (the last 10,000 years of geological history). About 6,400 years ago a warm interval lasting for some centuries allowed the accumulation of organic matter and development of relatively thick soils even at high altitudes. Between 5.300 to 5.050 years ago a rapid climatic cooling took place, producing a persistent snow cover and followed by the rapid expansion of the glaciers. For 5,000 years the ice preserved the body, until the glaciers started to shrink, as it seems, at an unprecedented rate in modern times. Interested in reading more? Try: BARONI, C. & OROMBELLI, G. (1996): Short paper – the alpine “Iceman” and Holocene Climatic Change. Quaternary Research 46: 78-83 MAGNY, M. & HAAS, J.N. (2004): Rapid Communication – A major widespread climatic change around 5300 cal. yr BP at the time of the Alpine Iceman. Journal of Quaternary Science 19(5): 423-430 OEGGL, K. (2009): The significance of the Tyrolean Iceman for the archaeobotany of Central Europe. Veget. Hist. Archaeobot. 18:1-11 This article was first published in August 2014, and it has been updated to include new research published since then. This article is one of a two-part series on past temperatures, including how warm the Earth has been “lately.” Our 4.54-billion-year-old planet probably experienced its hottest temperatures in its earliest days, when it was still colliding with other rocky debris (planetesimals) careening around the solar system. The heat of these collisions would have kept Earth molten, with top-of-the-atmosphere temperatures upward of 3,600° Fahrenheit. Even after those first scorching millennia, however, the planet has often been much warmer than it is now. One of the warmest times was during the geologic period known as the Neoproterozoic, between 600 and 800 million years ago. Conditions were also frequently sweltering between 500 million and 250 million years ago. And within the last 100 million years, two major heat spikes occurred: the Cretaceous Hot Greenhouse (about 92 million years ago), and the Paleocene-Eocene Thermal Maximum (about 56 million years ago). Cartoon by Emily Greenhalgh, NOAA Climate.gov. History of hotTemperature records from thermometers and weather stations exist only for a tiny portion of our planet's 4.54-billion-year-long life. By studying indirect clues—the chemical and structural signatures of rocks, fossils, and crystals, ocean sediments, fossilized reefs, tree rings, and ice cores—however, scientists can infer past temperatures. None of these techniques help with the very early Earth. During the time known as the Hadean (yes, because it was like Hades), Earth’s collisions with other large planetesimals in our young solar system—including a Mars-sized one whose impact with Earth likely created the Moon—would have melted and vaporized most rock at the surface. Because no rocks on Earth have survived from so long ago, scientists have estimated early Earth conditions based on observations of the Moon and on astronomical models. Following the collision that spawned the Moon, the planet was estimated to have been around 2,300 Kelvin (3,680°F). What the collision that spawned Earth's Moon may have looked like. Collisions between Earth and rocky debris in the early solar system would have kept the surface molten and surface temperatures blistering. Image courtesy NASA. Even after collisions stopped, and the planet had tens of millions of years to cool, surface temperatures were likely more than 400° Fahrenheit. Zircon crystals from Australia, only about 150 million years younger than the Earth itself, hint that our planet may have cooled faster than scientists previously thought. Still, in its infancy, Earth would have experienced temperatures far higher than we humans could possibly survive. But suppose we exclude the violent and scorching years when Earth first formed. When else has Earth’s surface sweltered? Thawing the freezerBetween 600 and 800 million years ago—a period of time geologists call the Neoproterozoic—evidence suggests the Earth underwent an ice age so cold that ice sheets not only capped the polar latitudes, but may have extended all the way to sea level near the equator. Reflecting ever more sunlight back into space as they expanded, the ice sheets cooled the climate and reinforced their own growth. Obviously, the Earth didn’t remain stuck in the freezer, so how did the planet thaw? A geologic history of Earth since its formation 4.6 billion years ago, divided by eon and period, and showing fossils typical of a given period. Fossils reveal not only ancient plants and animals, but also ancient climates. Artwork © Ray Troll, 2010. Used with permission. Even while ice sheets covered more and more of Earth’s surface, tectonic plates continued to drift and collide, so volcanic activity also continued. Volcanoes emit the greenhouse gas carbon dioxide. In our current, mostly ice-free world, the natural weathering of silicate rock by rainfall consumes carbon dioxide over geologic time scales. During the frigid conditions of the Neoproterozoic, rainfall became rare. With volcanoes churning out carbon dioxide and little or no rainfall to weather rocks and consume the greenhouse gas, temperatures climbed. What evidence do scientists have that all this actually happened some 700 million years ago? Some of the best evidence is "cap carbonates" lying directly over Neoproterozoic-age glacial deposits. Cap carbonates—layers of calcium-rich rock such as limestone—only form in warm water. Rock formation in Namibia that shows a type of rock that only forms in warm water (cap dolostone) lying directly over a type of jumbled sedimentary rock, dated to 635 million years ago, that is commonly found at the margin of glaciers (diamictite). Image from teaching slides available at SnowballEarth.org. The fact that these thick, calcium-rich rock layers sat directly on top of rock deposits left behind by retreating glaciers indicate that temperatures rose significantly near the end of the Neoproterozoic, perhaps reaching a global average higher than 90° Fahrenheit. (Today's global average is lower than 60°F.) The tropical ArcticA Smithsonian Institution project has tried to reconstruct temperatures for the Phanerozoic Eon, or roughly the last half a billion years. Preliminary results released in 2019 showed warm temperatures dominating most of that time, with global temperatures repeatedly rising above 80°F and even 90°F—much too warm for ice sheets or perennial sea ice. About 250 million years ago, around the equator of the supercontinent Pangea, it was even too hot for peat swamps! Preliminary results from a Smithsonian Institution project led by Scott Wing and Paul Huber, showing Earth's average surface temperature over the past 500 million years. For most of the time, global temperatures appear to have been too warm (red portions of line) for persistent polar ice caps. The most recent 50 million years are an exception. Image adapted from Smithsonian National Museum of Natural History. Geologists and paleontologists have found that, in the last 100 million years, global temperatures have peaked twice. One spike was the Cretaceous Hot Greenhouse roughly 92 million years ago, about 25 million years before Earth’s last dinosaurs went extinct. Widespread volcanic activity may have boosted atmospheric carbon dioxide. Temperatures were so high that champsosaurs (crocodile-like reptiles) lived as far north as the Canadian Arctic, and warm-temperature forests thrived near the South Pole. Another hothouse period was the Paleocene-Eocene Thermal Maximum (PETM) about 55-56 million years ago. Though not quite as hot as the Cretaceous hothouse, the PETM brought rapidly rising temperatures. During much of the Paleocene and early Eocene, the poles were free of ice caps, and palm trees and crocodiles lived above the Arctic Circle. Around the time of the Paleocene-Eocene Thermal Maximum, much of the continental United States had a sub-tropical environment. This fossil palm is from Fossil Butte National Monument, Wyoming. Image courtesy U.S. National Park Service. During the PETM, the global mean temperature appears to have risen by as much as 5-8°C (9-14°F) to an average temperature as high as 73°F. (Again, today’s global average is shy of 60°F.) At roughly the same time, paleoclimate data like fossilized phytoplankton and ocean sediments record a massive release of carbon dioxide into the atmosphere, at least doubling or possibly even quadrupling the background concentrations. Deep ocean temperatures were generally high throughout the Paleocene and Eocene, with a particularly warm spike at the boundary between the two geological epochs around 56 million years ago. Temperatures in the distant past are inferred from proxies (oxygen isotope ratios from fossil foraminifera). "Q" stands of Quarternary. Graph by Hunter Allen and Michon Scott, using data from the NOAA National Climatic Data Center, courtesy Carrie Morrill. It is still uncertain where all the carbon dioxide came from and what the exact sequence of events was. Scientists have considered the drying up of large inland seas, volcanic activity, thawing permafrost, release of methane from warming ocean sediments, huge wildfires, and even—briefly—a comet. Like nothing we’ve ever seenEarth’s hottest periods—the Hadean, the late Neoproterozoic, the Cretaceous Hot Greenhouse, the PETM—occurred before humans existed. Those ancient climates would have been like nothing our species has ever seen. Modern human civilization, with its permanent agriculture and settlements, has developed over just the past 10,000 years or so. 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