Page 140 - Earth's Climate Past and Future
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Equinox
                                                 March 20
                                          Northern hemisphere spring
                                          Southern hemisphere autumn
                    Solstice
                    June 21
            Northern hemisphere summer
             Southern hemisphere winter
                                                      23    ˚
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                                                     Solstice
                                                   December 21
                                              Northern hemisphere winter
                                             Southern hemisphere summer

                          Equinox
                        September 22
                   Northern hemisphere autumn
                   Southern hemisphere spring

           Orbital changes All aspects of Earth’s present orbit have changed with
           time: the tilt of its axis, the shape of its path around the Sun, and the
           positions of the seasons on this path. These changes in orbit have driven  n Part III we move from tectonic-scale
           climatic changes on Earth. (Adapted from F. K. Lutgens and E. J. Tarbuck,  climate changes to orbital-scale changes
           The Atmosphere [Englewood Cliffs, NJ: Prentice-Hall, 1992].)
                                                                       Iduring the last several million years, a

                                                                       time when the continents and oceans were
                                                            reaching their present positions. During this interval,
                                                            changes in Earth’s orbit have been the major driver of
                                                            climate by altering the amount of solar radiation
                                                            received by season and by latitude (Chapter 7). Three
                                                            aspects of Earth’s orbit have varied over cycles ranging
                                                            in length from roughly 20,000 to 400,000 years: the tilt
                                                            of its axis, the shape of its yearly path of revolution
                                                            around the Sun, and the changing positions of the

                                                            seasons along that path.
                                                               Orbital-scale changes have occurred throughout
                                                            Earth’s history, but our focus here is on the last 3 Myr
                                                            because well-dated climate records are available from
                                                            far more sites than in earlier times. The resulting
                                                            increase in regional coverage provides greater insight
                                                            into the operation of the climate system. Most climate
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