Understanding climate change over the long term

In brief

  • The Earth's temperature has fluctuated naturally over hundreds of millions of years. These past changes can help us understand the relationship between temperature, greenhouse gases and other climate drivers today.
  • Some of the clearest changes in the Earth’s temperature and the composition of the atmosphere are recorded in ice cores, with records dating back nearly one million years. These ice core records show that the Earth has experienced cycles of ice ages separated by warm periods (called interglacial periods) approximately every 100 000 years. These are primarily driven by regular 'wobbles' in the Earth's orbit, which affects the amount of radiation (or energy) from the sun reaching the Earth.
  • The past 11 000 years (the Holocene) is marked by small global temperature changes, typically up to 1 to 1.5 °C. During this time, greenhouse gas concentrations were relatively stable until the large and rapid increases that began about 200 years ago as a result of anthropogenic emissions.
  • Since the Industrial Revolution around 1800, human activities have increased greenhouse gas concentrations and the concentration of CO2 is now higher than for at least the past 800 000 years.

In detail

The past 500 million years

During most of the past 500 million years, the Earth was warmer than today and probably completely free of ice sheets. While estimates of greenhouse gas concentrations prior to the last million years are rather uncertain, analysis of geological samples suggests that the warm ice-free periods coincide with high atmospheric CO2 levels.

On million-year time scales, CO2 levels change due to tectonic activity (volcanic eruptions and movement of continents), which affects the rates of CO2 exchange of ocean and atmosphere with the solid Earth (IPCC, 2007, FAQ 6.1).

CO2 levels of more than 4000 parts per million (ppm) occurred during the Ordovician-Silurian (450 million years ago). There is also evidence of a glacial event occurring during this period. This has been used by some to attempt to disprove the link between temperature and CO2. Royer et al. (2006) considered the CO2 forced climate thresholds over the Phanerozoic eon (the last 545 million years). It was found that there is insufficient proxy data to determine that a high CO2 event coincided with the Ordovician-Silurian glacial event. The only proxy CO2 data near this glacial event could be up to five million years younger than the event. Further, the Earth was a very different place during this period including differences in solar luminosity, albedo, distribution of continents and vegetation, orbital parameters and other greenhouse gases.

Atmospheric CO2 concentration and temperature can change rapidly, as demonstrated by a series of events during the early Cenozoic (last 65 million years) known as hyperthermals (Zachos et al. 2008). These were relatively brief intervals (less than a few tens of thousands of years) of extreme global warmth and massive carbon addition, but with widely differing scales of forcing and response. During the most prominent and best-studied hyperthermal, the Paleocene-Eocene thermal maximum (PETM) 55 million years ago, the global temperature increased by more than 5 °C in less than 10 000 years (Zachos et al. 2008).

The sources of massive carbon injections during early Cenozoic hyperthermals remain uncertain (Zachos et al. 2008). Carbon might have come from deeply buried rocks, perhaps liberated as methane and CO2 during intrusive volcanism. Alternatively, it could have come from Earth's surface as a positive feedback to initial warming. Below the sea floor, methane gas is frozen in the pores of sediment known as hydrates or clathrates. A rise in deep-sea temperature might have triggered the decomposition of clathrates on continental margins, releasing substantial amounts of methane and fuelling additional warming. Another such source is the oxidation of organic matter in terrestrial environments.

These warming events show characteristics that are indicative of short-term positive feedbacks, which accelerated and magnified the effects of initial carbon injection before weathering and other negative feedbacks restored the global carbon cycle to a steady state. The positive feedbacks of greatest concern for understanding overall global warming may be those that could release hundreds to thousands of gigatonnes of carbon after initial warming (Zachos et al. 2008). The large masses of organic carbon stored in soils or sediments of shallow aquatic systems represent a potential carbon input, should regions that were humid become drier. Rapid drying or fire could release carbon from these reservoirs at rates faster than carbon uptake by similar environments elsewhere.

The past three million years

The geological record shows that ice ages have come and gone over the past three million years (IPCC, 2007, FAQ 6.1). Ice core measurements of the past 800 000 years reveal how the atmosphere's composition has changed in unison with these climate changes (for example CO2, figure 2). The glacial (cold) and interglacial (warm) cycles are triggered by the variations in the Earth's orbit around the Sun, called Milankovitch cycles (figure 1). These alter the amount of solar radiation reaching different parts of the Earth, leading to changes in the atmospheric circulation and in the distribution of ice over tens of thousands of years. Many studies suggest that the amount of summer sunshine on northern continents is crucial: if it drops below a critical value, snow from the past winter does not melt away in summer and an ice sheet starts to grow as more and more snow accumulates (IPCC, 2007, FAQ 6.1). The next large reduction in northern summer insolation, similar to those that started past ice ages, is due to begin in 30 000 years (IPCC, 2007, FAQ 6.1).

Figure 1

Figure 1: The Milankovitch cycles are composed of the 96 000 year eccentricity (E) cycle (which accounts for the spacing of the past six interglacials), the 40 000 to 41 000 year obliquity (or tilt T) cycle (which accounts for glacial cycles more than 600 000 years ago) and the 19 000 to 23 000 year precession (P) cycle (which accounts for temperature swings in the past 150 000 years) (Bryant, 1997; IPCC, 2007, FAQ 6.1).

The variations in solar radiation alone are not large enough to have caused the observed temperature changes, their rate of change or their global extent, particularly during the 100 000 year interglacials. Changes in greenhouse gases, particularly CO2 (figure 2) have played significant amplifying roles (Petit et al. 1999; Shackleton, 2000; Weaver et al. 1998). During glacial periods, the CO2 concentration is low (around 180 ppm), while during inter-glacial periods the concentration is high (up to 300 ppm) (Lüthi et al. 2008). Processes in the atmosphere, in the ocean, in marine sediments and on land, and the dynamics of sea ice and ice sheets must be considered (IPCC, 2007, Box 6.2). On glacial-interglacial time scales, atmospheric CO2 levels are mainly governed by the interplay between ocean circulation, marine biological activity, ocean-sediment interactions, seawater carbonate chemistry and air-sea exchange. A number of hypotheses for the low glacial CO2 concentrations have emerged over the past 20 years (Webb et al. 1997; Broecker and Henderson, 1998; Archer et al. 2000; Sigman and Boyle, 2000; Caillon et al. 2003; Kohfeld et al. 2005; Jouzel et al. 2007; Ahn and Brook, 2008).

For example, Caillon et al. (2003) suggest that when emerging from an ice age, significant warming begins in the Antarctic. It then takes about 800 years for the Antarctic warming to transform into a CO2 increase through ocean processes. The Northern Hemisphere deglaciation follows the CO2 increase. The warming takes about 5000 years to complete. Therefore, increases in CO2 contribute to the latter 4200 years of warming, amplifying the initial warming, i.e. a positive feedback. Ice sheets also cause feedbacks as their surface albedo (reflectivity) is larger than the water or land masses they cover. Methane and nitrous oxide concentrations also change closely in time with the glacial-interglacial periods, contributing further to the positive feedback.

Much attention has been on the rapid methane increases at the end of ice ages, in concert with warming events (possibly destabilising clathrates). Though the methane change is too small to have been the primary cause of the warming, it caused a small positive feedback. Recent evidence from radiocarbon measurements confirm that wetland emissions, not clathrates, were the main cause of the methane increase during the last rapid warming about 12 000 years ago (Petrenko et al. 2009).

Figure 2

Figure 2: Top: Atmospheric CO2 concentration from ice cores in blue (EPICA Dome C: Luthi et al, 2008; Vostok: Petit et al. 1999; Law Dome: Etheridge et al. 1996; MacFarling Meure et al. 2006) and Cape Grim Station, Tasmania in orange (Steele et al. 2007). Bottom: Antarctic temperature variations derived from ice core isotopic proxies (Jouzel et al. 2007). Timescale is years before present (2009) (Source: David Etheridge, CSIRO).

The past 11 000 years

The past 11 000 years is known as the Holocene Warm Period. It is the current inter-glacial and the time during which modern civilization has emerged. The climate of the Holocene has been relatively stable, with global temperature variations less than 1 to 1.5 °C.

Over the past 2000 years, temperature fluctuations of 1.0 to 1.5 °C have occurred (Bryant, 1997; Moberg et al. 2005) as quantified by proxy data from tree rings, ice cores, lake sediments, coral rings, bore holes, etcetera, which go back more than a thousand years with decreasing spatial coverage for earlier periods. All published reconstructions indicate that Northern Hemisphere temperatures were warm during medieval times (950 to 1100 AD), cool in the 17th, 18th and 19th centuries, and then warmed rapidly (National Research Council, 2006). Average Northern Hemisphere temperatures during the second half of the 20th century were very likely higher than during any other 50-year period in the last 500 years and likely the highest in at least the past 1300 years (National Research Council, 2006; IPCC, 2007, Mann et al. 2008, 2009).

The linear warming trend over the past 50 years (0.13 °C per decade) is much more rapid than the 4 °C to 7 °C warming between ice ages and warm interglacial periods, which takes about 5000 years, i.e. about 0.01 °C per decade. The changes in climate and CO2 during the Little Ice Age (1500 to 1750 AD) are strongly correlated, with temperature leading CO2 by about 50 years (Scheffer et al. 2006). These records indicate a tight relation between CO2 and climate, with a gradient of 40ppm/ °C of global warming. However, given the discrepancies between different temperature reconstructions, and the uncertainties associated with interpreting Northern Hemisphere climate proxies in terms of global mean temperature, Cox and Jones (2008) estimate a gradient of 20 to 60 ppm/°C of global warming.

A remarkable feature of the Holocene is the large and rapid increase in the global concentrations of CO2, methane, and nitrous oxide, beginning about 200 years ago (MacFarling Meure et al. 2006), to levels not observed for the past 800 000 years or more (see figure 2). The average rate of increase in atmospheric CO2 was at least five times larger over the period from 1960 to 1999 than over any other 40-year period during the two millennia before the industrial era (MacFarling Meure et al. 2006). The average rate of increase in atmospheric methane was at least six times larger, and that for nitrous oxide at least two times larger (MacFarling Meure et al. 2006). Isotopic analysis of the CO2 and a decline in atmospheric oxygen concentration confirms that the majority of the increase comes from burning fossil fuels (IPCC, 2007, Ch 2).

Simulations by a range of global climate models taking into account all known climate forcings (solar variations, volcanic and anthropogenic aerosols, land cover and greenhouse gases) closely reproduce the observed temperature changes of the past millennium. Simulations without greenhouse gases and aerosols fail to account for the warming over the past century. Most of the warming since the mid-20th century is very likely due to anthropogenic increases in greenhouse gases (IPCC, 2007).

There is no evidence for large clathrate releases to the atmosphere in the Holocene or industrial period (post 1750). Because clathrates are metastable, warming or physical disturbances might destabilise them. Only a relatively small amount of the massive clathrate store would need to be released to cause a large increase in atmospheric concentrations (of methane and eventually CO2 as it is oxidised) and subsequent climate warming. Thus clathrate release is proposed as a small likelihood-large outcome risk for the future. But both evidence and modelling suggests that the clathrate store is likely to be stable for a while yet.

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