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The “hockey stick” graph featured in the 2001 IPCC assessment, showing temperature (departures from the 1961–1990 average) in the Northern Hemisphere during the past 1000 years. (IPCC)
Earth’s orbit around the sun is not precisely circular, but elliptical, with the sun positioned slightly to one side of the center point. Currently, this brings Earth about 3% closer to the sun in early January (perihelion) than in early July (aphelion), with about 7% more solar energy reaching Earth at perihelion. The eccentricity, or “off-centeredness,” of the orbit varies over time in a complicated way. The net result is two main cycles, one that averages about 100,000 years and another that runs about 400,000 years. When the eccentricity is low, there’s little change through the year in the Earth–sun distance. When eccentricity is high, the sunlight reaching Earth can be more than 20% stronger at perihelion than at aphelion. This either intensifies or counteracts seasonality, depending on the hemisphere and the time of year that perihelion and aphelion occur. The last eight ice ages have come and gone roughly in sync with the 100,000-year eccentricity cycle, but it’s not yet clear how strongly the two are related (see p. 296).
Over billions of years. On this scale, the details are blurry, but the overall picture is clear. The sun will continue to heat up and eventually undergo changes to its size and structure, producing a climate on Earth hot enough to evaporate the oceans and make life impossible. Eventually, the sun will shrink and start to fade, with the solar system reaching its cold “final configuration” in around 12 billion years.
James Croll. (J.C. Irons/photo courtesy NOAA)