{QTtext}{timescale:100}{size:16}{font:Arial}{backColor:0,0,0} {textColor:65535,65535,65535}{width:480}{height:100}{justify:left} [00:00:00] Equinox at Saturn [00:00:04] Since 2004, Cassini’s Composite Infrared Spectrometer (CIRS), has collected data on the thermal behavior of the main rings of Saturn. [00:00:10] Saturn experiences Equinox as Earth does every spring and fall. [00:00:14] But seasons on Saturn are much longer. [00:00:17] It takes around 30 years for this gas giant to complete a full orbit around the sun... [00:00:21] so an Equinox occurs roughly every 15 Earth years. [00:00:25] Because Saturn’s rotational axis is tiled with respect to its orbital plane, [00:00:29] from the sun, Saturn appears to show its rings at different angles at different points in its orbit. [00:00:45] For nearly half of Saturn’s orbit, the sun shines on the south side of the rings. [00:00:54] For the other half, it shines on the north side. [00:00:57] And every time the rings cross Saturn’s orbital plane, Equinox happens. [00:01:05] As less and less solar energy heats the rings, they cool down. [00:01:14] From 1994 to 2009 the sun illuminated the south side of the rings. [00:01:18] Cassini’s Composite Infrared Spectrometer had a unique view of the cooling of the rings. [00:01:24] Animation shows sun angle changing from December 2004 to August 2009 and shows temperature changes in the rings. [00:01:53] Equinox [00:01:56] The temperature of the side of the rings hidden from the sun changes, too. [00:02:07] Animation shows sun angle changing from December 2004 to August 2009 and shows temperature changes in the rings. [00:02:36] Equinox [00:02:39] NASA, Jet Propulsion Laboratory, California Institute of Technology [00:02:41]