Page 32 - Astronomy - October 2017 USA
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11
                                              Measuring a day


                                                      Jupiter
                                                         3.1°                               Rotation axis  Magnetic axis
                                                      10°
                                             NORTH                   Saturn  26.7°                    47°  28.3°
                                                                                       Uranus   Neptune

                                              Ecliptic
                                              plane                               –97.8°

                                                                                        60°

                                              The outer planets have no solid surface to track as they rotate in order to measure the length
         12                                   of their day. Instead, astronomers track the rotation of the planets’ magnetic poles, which
                                              typically are offset from the axis of rotation. Jupiter’s magnetic pole is offset from its rotational
                                              axis by about 10°, while Uranus’ axes are offset by 60° and Neptune’s by 47°. Saturn’s magnetic
                                              and rotational axes are almost perfectly aligned, with an offset of less than 1°, making
                                              measurements of the length of its day challenging. Both Voyager spacecraft measured the
                                              length of Saturn’s day to be about 10.7 hours, but the Cassini spacecraft has measured the
                                              length to be slightly shorter (10.6 hours) or longer (10.8 hours), depending on the hemisphere
                                              in which measurements are taken. ASTRONOMY: ROEN KELLY


                                             13                                moon somehow feeds the ring. Could there
                                                                               be ice volcanoes on Enceladus, providing
                                                                               the sloshy material that would fill in impact
                                                                               craters? If so, some of that gushing material
                                                                               perhaps could escape the surface and orbit
                                                                               Saturn as part of the E ring. Those first
                                                                               detailed observations from Voyager trig-
                                                                               gered an ongoing fascination with this
                                                                               small, reflective moon, adds Ingersoll.
                                                                                  Scientists now know from the Cassini
                                                                               mission that an underground water ocean
         11. Enhanced color image processing   hydrocarbons perhaps in liquid form at the   feeds geysers at Enceladus’ south pole.
         increases the ability to see clouds and   surface — made Titan even more intrigu-  They’ve also discovered likely
         storms in Saturn’s atmosphere, such
         as the convective clouds in this image   ing for further study. In fact, says Spilker,   hydrothermal activity at the ocean floor.
         taken November 5, 1980, from a range of   “it was really the Voyager flyby of Titan,   On Earth, biological ecosystems thrive in
         5 million miles (8 million km). NASA/JPL-CALTECH  and what we learned and what we didn’t   such environments. Could they do the
                                            learn, that led to this strong desire to go   same on Enceladus? That’s a question a
         12. The spacecraft revealed oval-shaped
         storms in Saturn’s atmosphere, similar   back.” And ultimately, it was that flyby that   future dedicated mission to the small
         to those seen on Jupiter. Imaged   sparked the Cassini mission.       moon might answer.
         November 7, 1980, from a distance    The Titan discoveries were just the
         of 4.6 million miles (7.5 million km),                                The weather out there
         these brown ovals in Saturn’s northern   beginning of revealing the saturnian satel-
         hemisphere span about 6,000 miles   lites. From afar, two of the planet’s closer-  Scientists didn’t send Voyager to Saturn to
         (10,000km) in diameter. NASA/JPL   in moons, Mimas and Enceladus, had been   study only its rings and moons. The planet
                                            considered twins due to their similar sizes.   and its atmosphere were also a science
         13. Winds in Saturn’s upper atmosphere
         are estimated to reach speeds of   But on November 12, 1980, Voyager found   focus. Like that of its sister giant planet,
         1,118 mph (1,800km/h), faster than the   that their surfaces look vastly different.   Jupiter, Saturn’s atmosphere hosts incred-
         winds on Jupiter. This ribbonlike feature   While Mimas was pockmarked with the   ible storms and enormous jet streams, and
         is the result of a westward jet stream   evidence of billions of years of collisions   the Voyager twins were the first spacecraft
         imaged on November 10, 1980, from a
         distance of 2.2 million miles (3.5 million   from space debris, Enceladus, oddly, was   to photograph the details in those cloud
         km). It was still visible to Cassini in 2012,   not. Scientists had expected a heavily cra-  tops up close.
         though its shape had changed in the
                                            tered surface, “and yet there were parts of   While reanalyzing Voyager images of
         intervening years. NASA/JPL
                                            Enceladus that were smooth,” says   Saturn’s poles, astronomer David Godfrey
         14. Saturn’s polar hexagon spans a   Caltech’s Andrew Ingersoll, who was a   discovered a hexagonal shape surrounding
         diameter of 20,000 miles (32,000km) and   member of the Voyager imaging team. The   the northern pole. That surprising shape
         reaches depths of 60 miles (100km) in the   world was also very reflective, similar to   comes from jet streams moving at differ-
         planet’s atmosphere. The bizarre feature
         was first identified in Voyager images and   the brightness of freshly fallen snow.  ent speeds. “It’s really just a meandering
         later confirmed by the Cassini spacecraft,   Observations from Earth of a ring   current flowing east a little faster than the
         which snapped this image June 14, 2013.   around Saturn at the distance of Enceladus’   rest of its neighbors,” explains Ingersoll,
         NASA/JPL-CALTECH/SPACE SCIENCE INSTITUTE
                                            orbit already hinted that perhaps that small   who was also the head of the Voyager
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