Paleoclimatology is the study of past climate, for times prior to instrumental weather measurements. Paleoclimatologists use information from natural climate "proxies," such as tree rings, ice cores, corals, and ocean and lake sediments, that record variations in past climate. Records of past climate from these proxy records are important for several reasons. Instrumental records of climate are limited in many parts of the world to the past 100 years or less, and are too short to assess whether climate variability, events, and trends of the 20th and 21st centuries are representative of the long-term natural variability of past centuries and millennia. For example, was the 1930s Dust Bowl drought, a widespread and severe event in the United States, a rare occurrence, or have similar events occurred in past centuries? Knowledge of the long-term natural variability of the Earth Climate system, and its causes, will also allow an understanding of the roles of natural climate variability and human-induced climate change in the current and future climate. In particular, reconstructed temperatures from proxy data for the past 1000 years have allowed an assessment of the warming over recent decades and indicate that the majority of this warming is due to the impact of human activities on climate, according to the Intergovernmental Panel on Climate Change (IPCC) (http://www.ipcc.ch). Geological evidence demonstrates that the Earth's climate is dynamic, and has varied widely from our everyday experience. Over the past two million years, numerous glacial periods have covered much of the northern hemisphere in glacial ice, dropped sea level as much as 125 meters, and significantly cooled even tropical regions. In the more distant past, the Cretaceous Period was significantly warmer than today, with less polar ice, raising sea levels and allowing warm weather organisms to thrive even in near-polar regions. In the past 150 years, instrumental weather records indicate that the Earth has warmed by approximately 0.6C. Our goal is to provide an archive of past climate observations, derived from multiple proxies, that enables scientists to understand and model the many different states of the climate system that have existed in the past. Why Should We Care About Climate Change? If there is one thing that the paleoclimatic record shows, it is the that the Earth's climate is always changing. Climatic variability, including changes in the frequency of extreme events (like droughts, floods and storms), has always had a large impact on humans. A particularly severe El Nino, or relatively short drought, can cost billions of dollars. For this reason, scientists study past climatic variability on various time scales to gain clues that will help society plan for future climate change. Unfortunately, records of past climate change from satellites and human measurements (thermometers, rain gauges) generally cover less than 150 years. These are too short to examine the full range of climatic variability. For this reason, it is critical to examine climate change going back hundreds and thousands of years using paleoclimatic records from trees, corals, sediments, glaciers and natural or "proxy" sources. The study of past climate change also helps us understand how humans influence the Earth's climate system. The climatic record over the last thousand years clearly shows that global temperatures increased significantly in the 20th Century, and that this warming was likely to have been unprecedented in the last 2000 years. The paleoclimatic record also allows us to examine the causes of past climate change, and to help unravel how much of the 20th century warming may be explained by natural causes, such as solar variability, and how much may be explained by human influences. Lastly, most state of the art climate prediction is accomplished using large sophisticated computer models of the climate system. A great deal of research has been focused on ensuring that these models can simulate most aspects of the modern, present-day, climate. It is also important to know how these same models simulate climate change. This can be accomplished by comparing simulations of past climate change with observations from paleoclimatic records. Thus, paleoclimatology helps us improve the ability of computer models to simulate future climate. How Do Scientists Study Past Climates? There are several ways that scientists study how the Earth's climate is changing: satellites, instrumental records, historical records and proxy data. Some scientists look to satellites to study the Earth's changing climate. However, the satellite record is too short (ca. 20 years) to provide much perspective on changing climate. The record of instrumental weather measurements, extending back into the 19th century, provides data from thermometers, rain gauges, historical documents and other instruments. However, this record is too short to study many climatic processes. Also, because we have few instrumented observations from before the major industrial releases of carbon dioxide began, it is difficult to separate human and natural influences on climate. Paleoclimatologists find clues in natural records - proxy data. Proxy data are natural clues to past climate that are buried in sediments at the bottom of the oceans, locked in coral reefs, frozen in glaciers and ice caps, or preserved in the rings of trees. What Do We Know About the History of Climate? Good weather records extend back less than 150 years in most places. In that time, the Earth's global average temperature has increased by approximately 0.7 degrees centigrade or 1.3 degrees Fahrenheit. Some of this warming is natural, however a large part is the result of human induced greenhouse warming. Since the end of the last ice age occurred over 10,000 years ago, the planet has continued to undergo changes in climate. Warming during medieval times and cooling during the "Little Ice Age" a few centuries ago dominate the last millenia. From paleo records, we know that the climate of the past million years has been dominated by the glacial cycle, a pattern of ice ages and glacial retreats lasting thousands of years. Eighteen-thousand years ago, at the peak of the last ice age, scientists estimate that nearly 32% of the earth's land area was covered with ice, including much of Canada, Scandinavia, and the British Isles. These glaciers developed because the earth was in the midst of an ice age. Today ice coversage about 10% of the Earth's land surface. Paleo Proxy Data Paleoclimatologists gather proxy data from natural recorders of climate variability such as tree rings, ice cores, fossil pollen, ocean sediments, corals and historical data. By analyzing records taken from these and other proxy sources, scientists can extend our understanding of climate far beyond the 100+ year instrumental record. Listed below are some widely used proxy climate data types: Historical documents contain a wealth of information about past climates. Observations of weather and climatic conditions can be found in ship and farmers' logs, travelers' diaries, newspaper accounts, and other written records. When properly evaluated, historical data can yield both qualitative and quantitative information about past climate. Corals build their hard skeletons from calcium carbonate, a mineral extracted from sea water. The carbonate contains isotopes of oxygen, as well as trace metals, that can be used to determine the temperature of the water in which the coral grew. These temperature recordings can then be used to reconstruct climate when the coral lived. All flowering plants produce pollen grains. Their distinctive shapes can be used to identify the type of plant from which they came. Since pollen grains are well preserved in the sediment layers in the bottom of a pond, lake or ocean, an analysis of the pollen grains in each layer tell us what kinds of plants were growing at the time the sediment was deposited. Inferences can then be made about the climate based on the types of plants found in each layer. Since tree growth is influenced by climatic conditions, patterns in tree-ring widths, density, and isotopic composition reflect variations in climate. In temperate regions where there is a distinct growing season, trees generally produce one ring a year, and thus record the climatic conditions of each year. Trees can grow to be hundreds to thousands of years old and can contain annually-resolved records of climate for centuries to millennia. Located high in mountains and in polar ice caps, ice has accumulated from snowfall over many millenia. Scientists drill through the deep ice to collect ice cores. These cores contain dust, air bubbles, and isotopes of oxygen, that can be used to interpret the past climate of that area. Billions of tons of sediment accumulate in the ocean and lake basins each year. Scientist drill cores of sediment from the basin floors. Ocean and lake sediments include tiny fossils and chemicals that are used to interpret past climates. What is Glaciation? What Causes it? The Laurentide Ice Sheet covered most of Canada and northern areas of the United States 18,000 years ago. Geologists have found material left by the ice throughout this area, proving that virtually all of Canada and some of the northern US were once covered by thick glacial ice. Similar findings show that ice was also widespread in many other parts of the world. Scientists believe that changes in the earth's climate caused the ice sheets to grow. The explanation for these climate changes is believed to be variations in the earth's orbit around the sun (The Milankovitch Theory), combined with positive feedbacks from albedo (reflection of sunlight from snow and ice) and decreases in Carbon Dioxide concentrations in the atmosphere. What is The Milankovitch Theory? The Milankovitch or astronomical theory of climate change is an explanation for changes in the seasons which result from changes in the earth's orbit around the sun. The theory is named for Serbian astronomer Milutin Milankovitch, who calculated the slow changes in the earth's orbit by careful measurements of the position of the stars, and through equations using the gravitational pull of other planets and stars. He determined that the earth "wobbles" in its orbit. The earth's "tilt" is what causes seasons, and changes in the tilt of the earth change the strength of the seasons. The seasons can also be accentuated or modified by the eccentricity (degree of roundness) of the orbital path around the sun, and the precession effect, the position of the solstices in the annual orbit. The earth wobbles in space so that its tilt changes between about 22 and 25 degrees on a cycle of about 41,000 years. It is the cool summers which are thought to allow snow and ice to last from year to year in high latitudes, eventually building up into massive ice sheets. There are positive feedbacks in the climate system as well, because an earth covered with more snow reflects more of the sun's energy into space, causing additional cooling. In addition, it appears that the amount of Carbon Dioxide in the atmosphere falls as ice sheets grow, also adding to the cooling of the climate. The earth's orbit around the sun is not quite circular, which means that the earth is slightly closer to the sun at some times of the year than others. The closest approach of the earth to the sun is called perihelion, and it now occurs in January, making northern hemisphere winters slightly milder. This change in timing of perihelion is known as the precession of the equinoxes, and occurs on a period of 22,000 years. 11,000 years ago, perihelion occurred in July, making the seasons more severe than today. The "roundness", or eccentricity, of the earth's orbit varies on cycles of 100,000 and 400,000 years, and this affects how important the timing of perihelion is to the strength of the seasons. The combination of the 41,000 year tilt cycle and the 22,000 year precession cycles, plus the smaller eccentricity signal, affect the relative severity of summer and winter, and are thought to control the growth and retreat of ice sheets. Cool summers in the northern hemisphere, where most of the earth's land mass is located, appear to allow snow and ice to persist to the next winter, allowing the development of large ice sheets over hundreds to thousands of years. Conversely, warmer summers shrink ice sheets by melting more ice than the amount accumulating during the winter. For more detailed explanations of orbital variations with graphic representations, please see WDC Paleo's educational slide set "The Ice Ages": ftp://ftp.ncdc.noaa.gov/pub/data/paleo/slidesets/iceage/ What does The Milankovitch Theory say about future climate change? Orbital changes occur over thousands of years, and the climate system may also take thousands of years to respond to orbital forcing. Theory suggests that the primary driver of ice ages is the total summer radiation received in northern latitude zones where major ice sheets have formed in the past, near 65 degrees north. Past ice ages correlate well to 65N summer insolation (Imbrie 1982). Astronomical calculations show that 65N summer insolation should increase gradually over the next 25,000 years, and that no 65N summer insolation declines sufficient to cause an ice age are expected in the next 50,000 - 100,000 years.