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December 29, 20
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December 5, 200
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December 5, 200
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December 5, 200
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December 7, 200
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February 17, 20
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February 17, 20
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February 18, 2
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February 2, 200
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February 2, 200
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February 20, 20
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February 2000
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February 21, 20
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February 22, 20
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February 22, 20
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February 23, 20
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February 23, 20
(1)
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February 23, 20
(1)
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February 24, 20
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February 24, 20
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February 24, 20
(3)
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February 25, 20
(1)
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February 26, 20
(1)
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February 27, 20
(3)
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February 27, 20
(2)
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February 27, 20
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February 27, 20
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February 28, 20
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February 28, 20
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February 28, 20
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February 3, 200
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February 3, 200
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February 4, 200
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February 6, 200
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February 6, 200
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February 7, 200
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February 7, 200
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February 7, 200
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February 8, 200
(4)
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February 8, 200
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February 8, 200
(1)
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February 9, 200
(1)
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February 9, 200
(1)
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February 9, 200
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February 9, 200
(1)
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January 1, 2001
(3)
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January 1, 2005
(2)
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January 1, 2007
(1)
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January 10, 200
(7)
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January 10, 200
(1)
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January 10, 200
(1)
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January 11, 200
(2)
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January 11, 200
(1)
-
January 11, 200
(4)
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January 12, 200
(1)
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January 12, 200
(2)
-
January 12, 200
(1)
-
January 13, 200
(2)
-
January 13, 200
(2)
-
January 14, 20
(16)
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January 15, 200
(4)
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January 15, 200
(4)
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January 15, 200
(1)
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January 15, 200
(1)
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January 16, 200
(2)
-
January 16, 200
(1)
-
January 17, 200
(1)
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January 17, 200
(2)
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January 17, 200
(1)
-
January 18, 200
(2)
-
January 18, 200
(1)
-
January 18, 200
(1)
-
January 19, 200
(1)
-
January 19, 200
(1)
-
January 19, 200
(1)
-
January 1998
(1)
-
January 2, 2006
(1)
-
January 2, 2007
(1)
-
January 20, 200
(1)
-
January 20, 200
(1)
-
January 2001
(12)
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January 2004
(1)
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January 2005
(16)
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January 2006
(2)
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January 21, 200
(3)
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January 21, 200
(1)
-
January 22, 200
(1)
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January 23, 200
(6)
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January 23, 200
(1)
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January 23, 200
(2)
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January 23,2000
(3)
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January 24, 200
(1)
-
January 24, 200
(1)
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January 24, 200
(2)
-
January 25, 200
(1)
-
January 25, 200
(1)
-
January 25, 200
(1)
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January 26, 200
(1)
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January 26, 200
(2)
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January 26, 200
(1)
-
January 27, 200
(1)
-
January 27, 200
(6)
-
January 28, 200
(1)
-
January 29, 199
(1)
-
January 29, 200
(1)
-
January 3, 2005
(1)
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January 3, 2006
(1)
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January 3, 2007
(2)
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January 30, 200
(3)
-
January 30, 200
(1)
-
January 30, 200
(1)
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January 31, 200
(2)
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January 31, 200
(1)
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January 4, 1998
(1)
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January 4, 2005
(1)
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January 4, 2006
(1)
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January 4, 2007
(1)
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January 5, 2005
(1)
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January 5, 2006
(1)
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January 5, 2007
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January 6, 2005
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January 6, 2006
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January 7, 1998
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January 7, 2005
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January 9, 2007
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July 01, 2004
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July 02, 2006
(1)
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July 03, 2006
(1)
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July 1, 2004
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July 1, 2006
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(2)
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July 10, 2006
(1)
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July 10, 2007
(1)
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July 11, 2005
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July 11, 2006
(3)
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July 11, 2007
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July 12, 1981
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July 12, 2003
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July 12, 2005
(3)
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July 12, 2006
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July 12, 2007
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July 13, 2004
(15)
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July 13, 2005
(1)
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July 13, 2006
(1)
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July 13, 2007
(1)
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July 14 2005
(1)
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July 14, 2005
(48)
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July 14, 2006
(1)
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July 15, 2004
(3)
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July 15, 2005
(4)
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July 15, 2006
(2)
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July 16, 2005
(4)
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July 16, 2007
(1)
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July 17, 2004
(2)
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July 17, 2006
(1)
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July 17, 2007
(1)
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July 18, 2005
(2)
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July 18, 2006
(2)
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July 18, 2007
(1)
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July 19, 2004
(6)
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July 19, 2005
(2)
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July 19, 2006
(4)
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July 19, 2007
(1)
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July 1997
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July 2, 2004
(21)
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July 2, 2006
(4)
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July 2, 2007
(5)
-
July 20, 2004
(2)
-
July 20, 2005
(4)
-
July 20, 2006
(1)
-
July 20, 2007
(5)
-
July 2004
(31)
-
July 2006
(10)
-
July 2008
(1)
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July 21, 2004
(4)
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July 21, 2005
(2)
-
July 21, 2006
(4)
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July 21, 2007
(6)
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July 22, 2004
(4)
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July 22, 2005
(3)
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July 22, 2006
(18)
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July 22, 2007
(4)
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July 23, 2002
(1)
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July 23, 2004
(2)
-
July 23, 2006
(16)
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July 23, 2007
(5)
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July 24, 2004
(4)
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July 24, 2006
(5)
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July 24, 2007
(5)
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July 25, 2004
(2)
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July 25, 2005
(5)
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July 25, 2006
(5)
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July 25, 2007
(1)
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July 26, 2004
(2)
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July 26, 2005
(4)
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July 26, 2006
(6)
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July 26, 2007
(1)
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July 27, 2005
(1)
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July 27, 2006
(1)
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July 27, 2007
(2)
-
July 28, 2004
(2)
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July 28, 2005
(1)
-
July 28, 2006
(1)
-
July 28, 2007
(6)
-
July 29, 2005
(5)
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July 29, 2007
(2)
-
July 3, 2004
(19)
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July 3, 2006
(3)
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July 3, 2007
(3)
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July 30, 2004
(3)
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July 30, 2007
(1)
-
July 31, 2005
(8)
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July 31, 2006
(3)
-
July 31, 2007
(1)
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July 4, 2005
(1)
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July 4, 2006
(5)
-
July 4, 2007
(4)
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July 5, 2005
(1)
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July 5, 2006
(3)
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July 5, 2007
(1)
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July 6, 2005
(5)
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July 6, 2006
(1)
-
July 6, 2007
(3)
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July 7, 2005
(3)
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July 7, 2006
(1)
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July 8, 2005
(1)
-
July 8, 2007
(8)
-
July 9, 1995
(1)
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July 9, 2002
(3)
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July 9, 2007
(1)
-
July, 2005
(3)
-
June 1, 2004
(7)
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June 1, 2005
(3)
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June 1, 2006
(3)
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June 1, 2007
(7)
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June 10, 2004
(7)
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June 10, 2005
(8)
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June 10, 2006
(4)
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June 10, 2007
(2)
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June 11, 2004
(18)
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June 11, 2005
(3)
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June 11, 2006
(8)
-
June 11, 2007
(3)
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June 12, 2006
(1)
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June 12, 2007
(13)
-
June 13, 2005
(1)
-
June 13, 2006
(5)
-
June 13, 2007
(3)
-
June 14, 2004
(1)
-
June 14, 2005
(1)
-
June 14, 2006
(1)
-
June 14, 2007
(7)
-
June 15, 2005
(5)
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June 15, 2006
(3)
-
June 15, 2007
(3)
-
June 16, 2005
(1)
-
June 16, 2006
(1)
-
June 17, 2004
(1)
-
June 17, 2005
(1)
-
June 17, 2007
(2)
-
June 18, 2004
(2)
-
June 18, 2007
(3)
-
June 19, 1999
(2)
-
June 19, 2006
(1)
-
June 19, 2007
(1)
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June 1999
(2)
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June 2, 2004
(4)
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June 2, 2005
(3)
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June 2, 2006
(5)
-
June 2, 2007
(4)
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June 20, 2005
(1)
-
June 20, 2006
(1)
-
June 20, 2007
(1)
-
June 2004
(23)
-
June 2005
(4)
-
June 21, 2004
(11)
-
June 21, 2005
(9)
-
June 21, 2006
(2)
-
June 21, 2007
(3)
-
June 22, 2004
(1)
-
June 22, 2005
(1)
-
June 22, 2006
(1)
-
June 22, 2007
(1)
-
June 23, 2005
(1)
-
June 23, 2006
(1)
-
June 24, 1999
(1)
-
June 24, 2005
(1)
-
June 24, 2007
(4)
-
June 25, 2005
(4)
-
June 25, 2006
(2)
-
June 25, 2007
(2)
-
June 26, 2005
(2)
-
June 26, 2006
(1)
-
June 26, 2007
(3)
-
June 27, 2005
(3)
-
June 27, 2006
(1)
-
June 27, 2007
(1)
-
June 28, 2005
(9)
-
June 28, 2006
(5)
-
June 28, 2007
(6)
-
June 29, 2005
(6)
-
June 29, 2006
(1)
-
June 29, 2007
(5)
-
June 3, 2005
(7)
-
June 30, 2004
(5)
-
June 30, 2005
(3)
-
June 30, 2006
(12)
-
June 4, 2005
(2)
-
June 4, 2007
(1)
-
June 5, 2006
(2)
-
June 5, 2007
(3)
-
June 6, 2005
(5)
-
June 6, 2006
(3)
-
June 6, 2007
(1)
-
June 7, 2005
(5)
-
June 7, 2006
(3)
-
June 7, 2007
(2)
-
June 8, 2005
(9)
-
June 8, 2006
(1)
-
June 8, 2007
(1)
-
June 9, 2005
(2)
-
June 9, 2006
(5)
-
June 9, 2007
(4)
-
June, 11 2004
(3)
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June, 2004
(2)
-
March 1, 2005
(1)
-
March 1, 2006
(1)
-
March 1, 2007
(9)
-
March 10, 2004
(2)
-
March 10, 2005
(1)
-
March 10, 2006
(18)
-
March 10, 2007
(2)
-
March 11, 2005
(10)
-
March 11, 2006
(4)
-
March 12, 2005
(8)
-
March 12, 2007
(1)
-
March 13, 2005
(4)
-
March 13, 2006
(5)
-
March 13, 2007
(4)
-
March 14, 2005
(3)
-
March 14, 2006
(1)
-
March 14, 2007
(5)
-
March 15, 2005
(3)
-
March 15, 2006
(5)
-
March 15, 2007
(2)
-
March 16, 2005
(13)
-
March 16, 2006
(11)
-
March 16, 2007
(3)
-
March 17, 2005
(1)
-
March 17, 2006
(1)
-
March 17, 2007
(4)
-
March 18, 2005
(3)
-
March 18, 2007
(1)
-
March 19, 2005
(6)
-
March 19, 2007
(2)
-
March 2, 2005
(1)
-
March 2, 2006
(5)
-
March 2, 2007
(1)
-
March 20, 2006
(5)
-
March 20, 2007
(1)
-
March 2001
(2)
-
March 2003
(7)
-
March 2004
(9)
-
March 2005
(12)
-
March 21, 2005
(2)
-
March 21, 2006
(9)
-
March 21, 2007
(2)
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March 22, 2001
(4)
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March 22, 2004
(5)
-
March 22, 2005
(1)
-
March 22, 2006
(3)
-
March 22, 2007
(3)
-
March 23, 2005
(1)
-
March 23, 2006
(1)
-
March 23, 2007
(2)
-
March 24, 2005
(6)
-
March 24, 2006
(6)
-
March 24, 2007
(3)
-
March 25, 2005
(3)
-
March 26, 2007
(3)
-
March 27, 2004
(1)
-
March 27, 2006
(12)
-
March 27, 2007
(5)
-
March 28, 2005
(1)
-
March 28, 2006
(1)
-
March 28, 2007
(1)
-
March 29, 2001
(1)
-
March 29, 2005
(1)
-
March 29, 2006
(6)
-
March 29, 2007
(5)
-
March 3, 2005
(3)
-
March 3, 2006
(3)
-
March 30, 2004
(2)
-
March 30, 2005
(4)
-
March 30, 2006
(1)
-
March 30, 2007
(3)
-
March 31, 2004
(3)
-
March 31, 2005
(17)
-
March 31, 2006
(1)
-
March 4, 2005
(1)
-
March 5, 2005
(2)
-
March 5, 2007
(2)
-
March 6, 2005
(4)
-
March 6, 2006
(3)
-
March 6, 2007
(2)
-
March 7, 2005
(14)
-
March 7, 2006
(11)
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March 7, 2007
(2)
-
March 8, 2001
(1)
-
March 8, 2004
(1)
-
March 8, 2005
(3)
-
March 8, 2006
(1)
-
March 8, 2007
(2)
-
March 9, 2005
(33)
-
March 9, 2006
(11)
-
March 9, 2007
(1)
-
March, 2005
(4)
-
May 1, 2004
(2)
-
May 1, 2005
(8)
-
May 1, 2006
(1)
-
May 1, 2007
(5)
-
May 10, 2004
(13)
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May 10, 2005
(4)
-
May 10, 2006
(3)
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May 10, 2007
(2)
-
May 11, 2004
(11)
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May 11, 2006
(5)
-
May 11, 2007
(7)
-
May 12, 2005
(1)
-
May 12, 2006
(5)
-
May 12, 2007
(7)
-
May 13, 2005
(3)
-
May 13, 2006
(2)
-
May 13, 2007
(6)
-
May 14, 2005
(4)
-
May 14, 2006
(2)
-
May 14, 2007
(3)
-
May 15, 2004
(6)
-
May 15, 2006
(1)
-
May 15, 2007
(3)
-
May 16, 2004
(10)
-
May 16, 2005
(1)
-
May 16, 2006
(1)
-
May 16, 2007
(2)
-
May 17, 2005
(1)
-
May 17, 2006
(1)
-
May 17, 2007
(1)
-
May 18, 2004
(2)
-
May 18, 2005
(4)
-
May 18, 2006
(2)
-
May 18, 2007
(1)
-
May 19, 2005
(1)
-
May 19, 2006
(1)
-
May 2, 2005
(9)
-
May 2, 2006
(1)
-
May 2, 2007
(1)
-
May 20, 2004
(4)
-
May 20, 2005
(17)
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May 20, 2006
(2)
-
May 2003
(6)
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May 2005
(4)
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May 21, 2004
(5)
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May 21, 2005
(6)
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May 21, 2006
(4)
-
May 21, 2007
(1)
-
May 22, 1996
(2)
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May 22, 2004
(1)
-
May 22, 2005
(2)
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May 22, 2006
(7)
-
May 22, 2007
(3)
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May 23, 2004
(3)
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May 23, 2005
(5)
-
May 23, 2006
(1)
-
May 23, 2007
(7)
-
May 24, 2005
(5)
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May 24, 2006
(3)
-
May 24, 2007
(3)
-
May 25, 2001
(3)
-
May 25, 2004
(2)
-
May 25, 2005
(3)
-
May 25, 2006
(1)
-
May 25, 2007
(1)
-
May 26, 2004
(7)
-
May 26, 2005
(1)
-
May 26, 2006
(1)
-
May 27, 2005
(1)
-
May 27, 2007
(4)
-
May 28, 2007
(2)
-
May 29, 2006
(1)
-
May 29, 2007
(4)
-
May 3, 2005
(13)
-
May 3, 2006
(7)
-
May 3, 2007
(1)
-
May 30, 2001
(3)
-
May 30, 2005
(1)
-
May 30, 2006
(1)
-
May 30, 2007
(4)
-
May 31, 2005
(1)
-
May 31, 2006
(2)
-
May 31, 2007
(2)
-
May 4, 2004
(2)
-
May 4, 2005
(6)
-
May 4, 2006
(14)
-
May 4, 2007
(3)
-
May 5, 2004
(3)
-
May 5, 2005
(9)
-
May 5, 2006
(4)
-
May 5, 2007
(4)
-
May 6, 2005
(1)
-
May 7, 2004
(4)
-
May 7, 2007
(1)
-
May 8, 2004
(2)
-
May 8, 2006
(5)
-
May 8, 2007
(5)
-
May 9, 2005
(1)
-
May 9, 2006
(1)
-
May 9, 2007
(6)
-
November 1, 200
(5)
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November 1, 200
(1)
-
November 1, 200
(1)
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November 10, 20
(1)
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November 10, 20
(1)
-
November 11, 19
(1)
-
November 11, 20
(1)
-
November 12, 19
(2)
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November 12, 20
(1)
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November 13, 19
(1)
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November 13, 20
(1)
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November 13, 20
(1)
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November 13, 20
(2)
-
November 14, 20
(1)
-
November 14, 20
(1)
-
November 15, 20
(1)
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November 15, 20
(1)
-
November 16, 19
(5)
-
November 16, 20
(2)
-
November 16, 20
(1)
-
November 16, 20
(2)
-
November 17, 20
(7)
-
November 17, 20
(1)
-
November 18, 20
(1)
-
November 19, 20
(1)
-
November 1980
(11)
-
November 1982
(3)
-
November 1988
(3)
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November 1990
(1)
-
November 1995
(3)
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November 1999
(6)
-
November 2, 200
(1)
-
November 2, 200
(1)
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November 2, 200
(1)
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November 20, 19
(1)
-
November 20, 20
(1)
-
November 20, 20
(1)
-
November 2000
(1)
-
November 2005
(1)
-
November 2006
(4)
-
November 21, 20
(1)
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November 21, 20
(1)
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November 21, 20
(1)
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November 22, 20
(1)
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November 22, 20
(1)
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November 22, 20
(1)
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November 23, 20
(1)
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November 23, 20
(1)
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November 24, 20
(1)
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November 25, 20
(1)
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November 26, 19
(2)
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November 26, 20
(1)
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November 27, 20
(1)
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November 27, 20
(1)
-
November 28, 20
(4)
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November 28, 20
(1)
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November 29, 20
(1)
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November 29, 20
(1)
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November 29, 20
(1)
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November 3, 198
(3)
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November 3, 200
(1)
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November 3, 200
(1)
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November 30, 20
(5)
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November 30, 20
(1)
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November 30, 20
(2)
-
November 4, 200
(5)
-
November 4, 200
(5)
-
November 5, 198
(1)
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November 5, 200
(1)
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November 6, 200
(1)
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November 7, 200
(1)
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November 7, 200
(1)
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November 7, 200
(1)
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November 8, 200
(1)
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November 8, 200
(1)
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November 8, 200
(1)
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November 9, 200
(2)
-
November 9, 200
(1)
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November 9, 200
(3)
-
November 9, 200
(1)
-
November, 2004
(2)
-
Oct, 26, 2004
(2)
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October 1, 2000
(2)
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October 1, 2007
(1)
-
October 10, 199
(1)
-
October 10, 200
(1)
-
October 10, 200
(2)
-
October 10, 200
(3)
-
October 11, 200
(1)
-
October 11, 20
(15)
-
October 11, 200
(3)
-
October 12, 200
(2)
-
October 12, 200
(3)
-
October 12, 200
(1)
-
October 13, 200
(1)
-
October 13, 200
(1)
-
October 14, 200
(1)
-
October 15, 19
(18)
-
October 15, 20
(13)
-
October 16, 200
(1)
-
October 16, 200
(1)
-
October 17, 200
(6)
-
October 17, 200
(1)
-
October 17, 200
(1)
-
October 18, 200
(1)
-
October 18, 200
(2)
-
October 19, 200
(1)
-
October 19, 200
(1)
-
October 19, 200
(1)
-
October 1997
(11)
-
October 2, 2006
(1)
-
October 2, 2007
(1)
-
October 20, 200
(1)
-
October 20, 200
(1)
-
October 2000
(6)
-
October 2004
(29)
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October 2005
(9)
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October 2007
(2)
-
October 21, 199
(1)
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October 21, 200
(2)
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October 22, 200
(1)
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October 23, 200
(1)
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October 23, 200
(2)
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October 23, 200
(1)
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October 24, 200
(4)
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October 24, 200
(1)
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October 24, 200
(1)
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October 24, 200
(4)
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October 25, 200
(4)
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October 25, 200
(4)
-
October 25, 200
(1)
-
October 25, 200
(1)
-
October 26, 200
(3)
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October 26, 200
(4)
-
October 26, 200
(1)
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October 26, 200
(1)
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October 26, 200
(1)
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October 27, 200
(1)
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October 27, 200
(1)
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October 28, 200
(2)
-
October 29, 200
(1)
-
October 3, 2005
(1)
-
October 3, 2006
(1)
-
October 3, 2007
(1)
-
October 30, 199
(2)
-
October 30, 200
(1)
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October 30, 200
(1)
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October 31, 199
(2)
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October 31, 200
(1)
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October 31, 200
(1)
-
October 31, 200
(1)
-
October 4, 2005
(1)
-
October 4, 2006
(1)
-
October 4, 2007
(1)
-
October 5, 2005
(1)
-
October 5, 2006
(3)
-
October 5, 2007
(1)
-
October 6, 2004
(1)
-
October 6, 2005
(1)
-
October 6, 2006
(1)
-
October 7, 2005
(3)
-
October 8, 200
(14)
-
October 9, 1994
(1)
-
October 9, 2006
(1)
-
October 9, 2007
(2)
-
October, 1996
(2)
-
October, 1997
(2)
-
October, 1998
(2)
-
October, 1999
(2)
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October, 2000
(2)
-
October, 2005
(2)
-
September 1, 20
(1)
-
September 10, 2
(1)
-
September 11, 2
(2)
-
September 11, 2
(3)
-
September 12, 2
(4)
-
September 12, 2
(1)
-
September 12, 2
(4)
-
September 12, 2
(7)
-
September 13, 2
(2)
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September 13, 2
(6)
-
September 13, 2
(1)
-
September 14, 2
(1)
-
September 14, 2
(1)
-
September 14, 2
(3)
-
September 14, 2
(1)
-
September 15, 2
(2)
-
September 15, 2
(1)
-
September 15, 2
(1)
-
September 16, 2
(5)
-
September 17, 2
(1)
-
September 18, 2
(1)
-
September 18, 2
(1)
-
September 19, 2
(1)
-
September 19, 2
(3)
-
September 19, 2
(1)
-
September 2, 20
(2)
-
September 20, 2
(2)
-
September 20, 2
(1)
-
September 20, 2
(1)
-
September 2004
(3)
-
September 2005
(8)
-
September 2007
(5)
-
September 21, 2
(1)
-
September 21, 2
(1)
-
September 21, 2
(1)
-
September 22, 2
(1)
-
September 22, 2
(2)
-
September 23, 2
(2)
-
September 23, 2
(1)
-
September 24, 2
(2)
-
September 24, 2
(1)
-
September 24, 2
(1)
-
September 25, 2
(2)
-
September 25, 2
(1)
-
September 26, 2
(6)
-
September 26, 2
(3)
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September 26, 2
(2)
-
September 27, 2
(2)
-
September 27, 2
(1)
-
September 28, 2
(1)
-
September 28, 2
(1)
-
September 28, 2
(1)
-
September 29, 2
(9)
-
September 29, 2
(1)
-
September 3, 20
(1)
-
September 30, 2
(1)
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September 4, 20
(2)
-
September 5, 2
(13)
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September 5, 20
(2)
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September 5, 20
(3)
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September 6, 20
(1)
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September 6, 20
(1)
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September 7, 20
(2)
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September 7, 20
(1)
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September 7, 20
(1)
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September 8, 20
(2)
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September 8, 20
(1)
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September 9, 20
(1)
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September, 2005
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Seventeenth cen
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The Usual Suspects
NASA's Cassini spacecraft ta
07/15/10
Description |
NASA's Cassini spacecraft takes us on a guided tour of this mysterious lake on Titan. |
Date |
07/15/10 |
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Beautiful Ontario Lacus
See Beautiful Ontario Lacus:
07/15/10
Description |
See Beautiful Ontario Lacus: Guided tour of a Titan lake, courtesy of NASA's Cassini. |
Date |
07/15/10 |
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Three Hot Topics at NASA
In this NASA eClips video di
2008
Description |
In this NASA eClips video discover three hot topics NASA is currently developing. The Cassini-Huygens is a spacecraft NASA sent to check out Saturn and Saturn's moons. Find out what discoveries have been made based on photos from this mission. Another hot topic is Stratospheric Observatory for Infrared Astronomy, or SOFIA, a modified Boeing 757 that holds an infrared telescope. This enables the telescope to capture infrared light. Finally, learn about the new space vehicle NASA will be using in the next decade. NASA will be retiring the space shuttle and will launch ORION. Find out how the ORION differes from the current space shuttle. This video is a NASA eClips (TM) program. |
Date |
2008 |
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Happy Halloween
The Cassini team sends "bats
10/30/09
Description |
The Cassini team sends "bats wishes" for a happy, healthy and fun Halloween. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. Image Credit: NASA |
Date |
10/30/09 |
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Happy New Year!
Wishing all a joyful new yea
12/31/09
Description |
Wishing all a joyful new year, members of the Cassini-Huygens team offer us their views of Saturn and the Cassini spacecraft. Cassini-Huygens, a cooperative project of NASA, the European Space Agency and the Italian Space Agency, which is managed by the Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, for NASA. The Cassini orbiter (pictured at the top right of this image) and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. Image Credit: NASA/JPL |
Date |
12/31/09 |
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Staring Mittens
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This is an artist concept and movie of the view from Cassini during the star occultation that detected "Mittens," the small object to the right of the star. As Cassini watched the star pass behind Saturn's F ring (foreground), the star blinked out when Mittens blocked it, indicating it may be a solid moonlet. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The ultraviolet imaging spectrograph was designed and built at, and the team is based at the University of Colorado, Boulder. For more information about the Cassini-Huygens mission, visit: http://saturn.jpl.nasa.gov/home/index.cfm. The ultraviolet imaging spectrograph team home page is at: http://lasp.colorado.edu/cassini . Credit: NASA/JPL/University of Colorado |
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Happy Holidays
Wishing all the happiest of
12/24/09
Description |
Wishing all the happiest of holidays, members of the Cassini-Huygens team offer their views of Saturn and its moons as gifts to the universe. Cassini-Huygens, a cooperative project of NASA, the European Space Agency and the Italian Space Agency, is a mission that is managed by the Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, for NASA. The Cassini orbiter (pictured at the bottom of this image) and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. Image Credit: NASA/JPL |
Date |
12/24/09 |
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Cassini Captures the Cassini
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image shows the region of Saturn's rings known as the Cassini Division. It was taken by the narrow angle camera on the Cassini spacecraft after successful entry into Saturn's orbit. The view shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Close Encounter of a First K
Description |
Close Encounter of a First Kind |
Full Description |
This movie is a condensed version of Cassini's 44-hour approach to Titan. During the movie, the planet rotates about 40 degrees and the spacecraft's distance to the moon ranges from 1,800,000 to 700,000 kilometers (1,000,000 to 435,000 miles). At is closest, on Oct. 26, 2004, Cassini was 1,200 kilometers (745 miles) above the moon. Clouds are seen forming and evolving near the south pole. The images making up this movie were captured by Cassini's imaging science subsystem through near-infrared filters. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For the latest news about the Cassini-Huygens mission, visit http://www.nasa.gov/cassini. For more information about the mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Enceladus Animation
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This animation shows the Cassini spacecraft approaching Saturn's icy moon Enceladus. It shows the highest resolution images obtained of the moon's surface. This is followed by a depiction of Saturn's magnetic field, which interacts with Enceladus' atmosphere and presumed plume coming from the south pole. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . Credit: NASA/JPL |
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Cassini Spacecraft Approache
Title |
Cassini Spacecraft Approaches Jupiter |
Explanation |
A new spacecraft has entered the outer Solar System: Cassini [ http://www.jpl.nasa.gov/cassini/english/spacecraft/ ]. Launched in 1997 [ http://antwrp.gsfc.nasa.gov/apod/ap971016.html ] and bound for Saturn in 2004, Cassini sent back the above image [ http://ciclops.lpl.arizona.edu/ciclops/Images_jupiter.html ] last week while approaching the giant planet Jupiter [ http://www.seds.org/nineplanets/nineplanets/jupiter.html ]. Cassini [ http://quest.arc.nasa.gov/saturn/qa/cassini/ ] joins the Galileo spacecraft [ http://www.jpl.nasa.gov/galileo/mission.html] currently in orbit around Jupiter in studying the gas giant and its moons. In fact, observations [ http://www.jpl.nasa.gov/releases/2000/glextended.html ] involving both spacecraft [ http://www.jpl.nasa.gov/jupiterflyby/ ] simultaneously are planned in the coming months. This color picture [ http://photojournal.jpl.nasa.gov/cgi-bin/ PIAGenCatalogPage.pl?PIA02972 ] was taken when Cassini was 81.3 million kilometers from Jupiter. The alternating dark and bright bands characteristic of Jupiter's cloud tops [ http://antwrp.gsfc.nasa.gov/apod/ap000429.html ] can be easily seen. Jupiter's moon Europa [ http://antwrp.gsfc.nasa.gov/apod/ap000825.html ] is also seen at the far right of the image casting a round shadow on the planet. |
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Tracking Huygens Animation
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
As Huygens descends Titan's atmosphere, Cassini will record the data from 72,000 kilometers (about 44,700 miles). |
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Cassini's Flyby 'Doubleheade
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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Cassini's First Color Movie
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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Cassini's First Color Movie
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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Eyes on Iapetus!
Description |
This map of the surface of Iapetus, generated from images taken by NASA's Cassini and Voyager spacecraft, illustrates the imaging coverage planned for Cassini's very close flyby of the two-toned moon on Sept. 10, 2007. |
Full Description |
This map of the surface of Iapetus, generated from images taken by NASA's Cassini and Voyager spacecraft, illustrates the imaging coverage planned for Cassini's very close flyby of the two-toned moon on Sept. 10, 2007. This flyby will be Cassini's only close approach to Iapetus (1,468 kilometers, or 912 miles across) during the entire planned mission. At closest approach, Cassini will be 1,640 kilometers (1,020 miles) above the surface of Iapetus. The spacecraft will pass the moon at a speed of about 2.4 kilometers (1.5 miles) per second--a relatively leisurely pace that will allow plenty of time for the scientific instruments on board to collect massive amounts of data. Cassini's previous encounter with Iapetus, on Dec. 31, 2004, focused on the mysterious territory in Cassini Regio, the region blanketed by dark material that covers most of the moon's leading hemisphere. The upcoming encounter will be primarily concerned with terrain farther west, in the important transition region between Cassini Regio and the bright trailing hemisphere. Scientists hope to learn a great deal more about the composition of the materials that compose the surface of Iapetus during this encounter. Another area of focus is the large equatorial ridge that overlies the moon's equator (see Encountering Iapetus). The ridge reaches 20 kilometers (12 miles) high in some places and extends over 1,300 kilometers (808 miles) in length. No other moon in the solar system has a geological feature like this striking ridge. The tallest mountains on the ridge rival Olympus Mons on Mars, which is approximately three times the height of Mt. Everest. Such giant mountains are a surprising feature for such a small body as Iapetus, which is nearly five times smaller than Mars and nearly nine times smaller than Earth. Colored lines on the map enclose regions that will be covered at different imaging scales as Cassini encounters Iapetus. The highest expected resolution of Cassini images from this flyby is about 20 meters (65 feet) per pixel--significantly higher than the 2004 encounter. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . *Credit:* NASA/JPL/Space Science Institute |
Date |
September 5, 2007 |
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Cassini to Look In, Out and
Description |
Cassini to Look In, Out and Over Titan |
Full Description |
Two years after reaching Saturn, the Cassini spacecraft is halfway to completing its orbital mission. On July 2, Cassini will perform its 16th flyby of Saturn's largest moon, Titan. Cassini will focus on the interactions between Titan's atmosphere and the big bubble that surrounds Saturn, called the magnetosphere. Cassini will also study Titan's surface to enable a better understanding of its properties and composition. + View Flyby page |
Date |
June 30, 2006 |
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Titan's First Close-Up
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image is one of the closest ever taken of Saturn's hazy moon Titan. It was captured by Cassini's imaging science subsystem on Oct. 26, 2004, as the spacecraft flew by Titan. At its closest, Cassini was 1,200 kilometers (745 miles) above the moon, 300 times closer than during its first flyby on July 3, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Titan's First Close-Up
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image is one of the closest ever taken of Saturn's hazy moon Titan. It was captured by Cassini's imaging science subsystem on Oct. 26, 2004, as the spacecraft flew by Titan. At its closest, Cassini was 1,200 kilometers (745 miles) above the moon, 300 times closer than during its first flyby on July 3, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Titan's First Close-Up
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image is one of the closest ever taken of Saturn's hazy moon Titan. It was captured by Cassini's imaging science subsystem on Oct. 26, 2004, as the spacecraft flew by Titan. At its closest, Cassini was 1,200 kilometers (745 miles) above the moon, 300 times closer than during its first flyby on July 3, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Titan's First Close-Up
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image is one of the closest ever taken of Saturn's hazy moon Titan. It was captured by Cassini's imaging science subsystem on Oct. 26, 2004, as the spacecraft flew by Titan. At its closest, Cassini was 1,200 kilometers (745 miles) above the moon, 300 times closer than during its first flyby on July 3, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Titan's First Close-Up
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image is one of the closest ever taken of Saturn's hazy moon Titan. It was captured by Cassini's imaging science subsystem on Oct. 26, 2004, as the spacecraft flew by Titan. At its closest, Cassini was 1,200 kilometers (745 miles) above the moon, 300 times closer than during its first flyby on July 3, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Titan's First Close-Up
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This image is one of the closest ever taken of Saturn's hazy moon Titan. It was captured by Cassini's imaging science subsystem on Oct. 26, 2004, as the spacecraft flew by Titan. At its closest, Cassini was 1,200 kilometers (745 miles) above the moon, 300 times closer than during its first flyby on July 3, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Titan's Dark Terrain
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This view from Cassini's second close flyby of Titan on Dec. 13, 2004 shows bright material within the large dark region west of Xanadu. The area in this image is a region that has not previously been seen by Cassini at this high resolution. The image was taken with the Cassini spacecraft narrow angle camera at a distance of approximately 125,900 kilometers (78,200 miles) from Titan, using a filter centered at 938 nanometers that emphasizes the moon's surface and clouds. The image scale is 735 meters (2,400 feet) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Saturn's Waves
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This Cassini image shows beautifully the complex eddies and wave patterns in Saturn's cloud bands. The image was taken with the Cassini spacecraft narrow angle camera on Sept. 7, 2004, at a distance of 8.9 million kilometers (5.5 million miles) from Saturn, through a filter sensitive to wavelengths of infrared light centered at 727 nanometers. The image scale is 53 kilometers (33 miles) per pixel. The image was magnified by a factor of two and slightly contrast-enhanced to improve visibility of features in the atmosphere. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Shadow of the Rings
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
The inner edges of Saturn's rings arc gracefully across the top of this image from Cassini. Thin shadows cast by the rings are visible at upper right through the optically thin C ring. The image was taken with the Cassini spacecraft narrow angle camera on Sept. 15, 2004, at a distance of 8.5 million kilometers (5.3 million miles) from Saturn through a filter sensitive to wavelengths of infrared light centered at 727 nanometers. The image scale is 50 kilometers (31 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Light and Dark Bands
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
Saturn's southern hemisphere boasts a great deal of fine detail in the turbulent boundaries between the atmospheric bands in this Cassini image. Note the faint bright spot in the band north of the dark polar region. The image was taken with the Cassini spacecraft narrow angle camera on Sept. 3, 2004, at a distance of 9 million kilometers (5.6 million miles) from Saturn, through a filter sensitive to wavelengths of infrared light. The image scale is 53 kilometers (33 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Delicate Southern Detail
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
Wavy cloud bands in Saturn's atmosphere near the south pole show a great deal of delicate structure and contrast and even a bright storm in this view from Cassini. The image was taken with the Cassini spacecraft narrow angle camera on Aug. 18, 2004, at a distance of 8.9 million kilometers (5.5 million miles) from Saturn through a filter sensitive to wavelengths of infrared light. The image scale is 53 kilometers (33 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Gazing Down
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
Cassini pierced the ring plane and rounded Saturn on Oct. 27, 2004, capturing this view of the dark portion of the rings. A portion of the planet's atmosphere is visible here, as is its shadow on the surface of the rings. The image was taken with the Cassini spacecraft wide angle camera on Oct. 27, 2004, at a distance of about 618,000 kilometers (384,000 miles) from Saturn through a filter sensitive to wavelengths of infrared light centered at 1001 nanometers. The image scale is 33 kilometers (21 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Cassini Radar Titan Movie
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
This animation shows the Cassini spacecraft approaching Titan. The strips of data on the globe represent areas observed with the Cassini radar instrument. The pink swatch is the area observed by the radar instrument during the Oct. 2004 flyby, while the blue area represents the coverage observed during the Feb. 15 flyby. The movie zooms into several interesting areas on Titan, including a giant crater the size of Iowa, an area with bright hills and ridges surrounded by a dark plain, and a smaller crater with a blanket of material surrounding it, possibly due to ejected material being thrown out of the crater after an impact. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The radar instrument team is based at JPL, working with team members from the United States and several European countries. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov. Credit: NASA/JPL |
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Panoramic Rings
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
Saturn's most prominent feature, its dazzling ring system, takes center stage in this stunning natural color mosaic which reveals the color and diversity present in this wonder of the solar system. Gaps, gravitational resonances and wave patterns are all present, and the delicate color variations across the system are clearly visible. This mosaic of six images covers a distance of approximately 62,000 kilometers along the ring plane, from a radius of 74,565 kilometers to 136,780 kilometers (46,333 to 84,991 miles) from the planet's center. This view is from Cassini's vantage point beneath the ring plane. The rings are tilted away from Cassini at an angle of about 4 degrees. Images taken using red, green and blue spectral filters were used to create this natural color mosaic. The images were acquired using the Cassini spacecraft narrow angle camera on Dec. 12, 2004, at a distance of approximately 1.8 million kilometers (1.1 million miles). The image scale is 10.5 kilometers (6.5 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org. Credit: NASA/JPL/Space Science Institute |
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Gazing Down
Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
Cassini pierced the ring plane and rounded Saturn on Oct. 27, 2004, capturing this view of the dark portion of the rings. A portion of the planet's atmosphere is visible here, as is its shadow on the surface of the rings. The image was taken with the Cassini spacecraft wide angle camera on Oct. 27, 2004, at a distance of about 618,000 kilometers (384,000 miles) from Saturn through a filter sensitive to wavelengths of infrared light centered at 1001 nanometers. The image scale is 33 kilometers (21 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Flight over Iapetus
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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Cassini sails low over the surface of Iapetus on approach to its close encounter with the enigmatic moon on Sept. 10, 2007. Its flight takes it over the rugged, mountainous ridge along the moon's equator, where ancient, impact battered peaks -- some topping 10 kilometers (6 miles) in height -- are seen rising over the horizon and slipping beneath the spacecraft as it flies. Frames used in this movie were acquired with the Cassini wide-angle camera on Sept. 10, 2007, as the intrepid robot soared past Iapetus (1,468 kilometers, or 912 miles across), within a few thousand kilometers of the surface. Additional simulated images were inserted between the Cassini images in this movie in order to smooth the appearance of the movement, a scheme called interpolation. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov. The Cassini imaging team homepage is at http://ciclops.org. Credit: NASA/JPL/Space Science Institute |
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Shadow of the Rings
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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The inner edges of Saturn's rings arc gracefully across the top of this image from Cassini. Thin shadows cast by the rings are visible at upper right through the optically thin C ring. The image was taken with the Cassini spacecraft narrow angle camera on Sept. 15, 2004, at a distance of 8.5 million kilometers (5.3 million miles) from Saturn through a filter sensitive to wavelengths of infrared light centered at 727 nanometers. The image scale is 50 kilometers (31 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Southern Hemisphere in Ultra
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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With ultraviolet eyes, Cassini gazes at cloud bands and wavy structures in Saturn's southern hemisphere. In the ultraviolet, the gaseous part of the atmosphere is bright and high clouds and aerosols tend to be dark. The Cassini spacecraft narrow angle camera took the image on May 15, 2004, from a distance of 24.7 million kilometers (15.4 million miles) from Saturn through a filter centered at 298 nanometers. The image scale is 147 kilometers (91 miles) per pixel. Contrast in the image was enhanced to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission visit, http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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First Flyby of Dione
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First Flyby of Dione |
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This map of Saturn's moon Dione, generated from Cassini images taken during the spacecraft's first two orbits of Saturn, illustrates the imaging coverage planned during Cassini's first Dione flyby on Dec. 14, 2004. Colored lines enclose regions that will be covered at different imaging scales as Cassini approaches Dione. Cassini will zoom past Dione at a distance of approximately 81,400 kilometers (50,600 miles) during this flyby. An even closer encounter with Dione is in store for Cassini in October 2005, when the spacecraft is slated to fly past the icy moon at a mere 500 kilometers (311 miles). Images from this week's flyby will be superior in resolution to those obtained by NASA's Voyager 1 in November 1980. Voyager 1 passed Dione at a distance of 161,520 kilometers (100,364 miles) at closest approach, yielding a best resolution of approximately 1 kilometer per pixel. The area to be imaged at highest resolution by Cassini during this upcoming flyby will be centered on the bright, wispy terrain on Dione's trailing hemisphere, marked by the red outline on this map. The resolution of Cassini images in this region will be 500 meters per pixel and better. The map was created by images acquired in visible light using the Cassini narrow angle camera. The highest southern latitudes on Dione have not yet been seen by Cassini, resulting in the map's lower limit of approximately 80 degrees south latitude. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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First Flyby of Dione
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First Flyby of Dione |
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This map of Saturn's moon Dione, generated from Cassini images taken during the spacecraft's first two orbits of Saturn, illustrates the imaging coverage planned during Cassini's first Dione flyby on Dec. 14, 2004. Colored lines enclose regions that will be covered at different imaging scales as Cassini approaches Dione. Cassini will zoom past Dione at a distance of approximately 81,400 kilometers (50,600 miles) during this flyby. An even closer encounter with Dione is in store for Cassini in October 2005, when the spacecraft is slated to fly past the icy moon at a mere 500 kilometers (311 miles). Images from this week's flyby will be superior in resolution to those obtained by NASA's Voyager 1 in November 1980. Voyager 1 passed Dione at a distance of 161,520 kilometers (100,364 miles) at closest approach, yielding a best resolution of approximately 1 kilometer per pixel. The area to be imaged at highest resolution by Cassini during this upcoming flyby will be centered on the bright, wispy terrain on Dione's trailing hemisphere, marked by the red outline on this map. The resolution of Cassini images in this region will be 500 meters per pixel and better. The map was created by images acquired in visible light using the Cassini narrow angle camera. The highest southern latitudes on Dione have not yet been seen by Cassini, resulting in the map's lower limit of approximately 80 degrees south latitude. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Off Saturn's Shoulder
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The Cassini spacecraft spies Enceladus and Epimetheus near the limb of Saturn. |
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The Cassini spacecraft spies Enceladus and Epimetheus near the limb of Saturn. Geologically active Enceladus is 505 kilometers (314 miles) across, smaller, more irregularly shaped Epimetheus is 116 kilometers (72 miles) across. This view looks toward the unilluminated side of the rings from less than a degree above the ringplane. The image was taken in polarized green light with the Cassini spacecraft narrow-angle camera on Oct. 27, 2007. The view was acquired at a distance of approximately 1.4 million kilometers (857,000 miles) from Enceladus. Epimetheus is 91,000 kilometers (57,000 miles) farther away from Cassini here. Image scale is about 8 kilometers (5 miles) per pixel on both moons. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
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December 12, 2007 |
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Cassini's Visit to Dione
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Cassini to Tour Moon with Streaks |
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This map of the surface of Saturn's moon Dione illustrates the regions that will be imaged by Cassini during the spacecraft's very close flyby of the moon on Oct. 11, 2005. At closest approach, the spacecraft is expected to pass approximately 500 kilometers (310 miles) above the moon's surface. Dione is 1,126 kilometers (700 miles) across. The colored lines delineate the regions that will be imaged at differing resolutions, listed in the legend at the bottom. Imaging scientists expect the Dione encounter to be one of the highlights of Cassini's mission. In terms of planning, this particular flyby is perhaps the most sophisticated yet undertaken by the Cassini imaging team. The timing of the imaging sequence has been optimized to within seconds, relative to the spacecraft's pointing during the encounter. As Cassini approaches Dione, the cameras will capture regional-scale, medium resolution mosaics, with some coverage of the moon's relatively poorly imaged leading hemisphere (the region centered on 90 degrees longitude). Planned inbound coverage also includes high-resolution images of the south pole and the well-known streaked terrain on Dione's trailing hemisphere. The previous flyby showed the markings to be an elaborate system of braided tectonic fractures. During the outbound portion of the flyby, Cassini will image a crescent Dione as the moon recedes into the distance. While staring at the moon's dark side, Cassini will take images using long exposure times, in order to see terrain that is dimly illuminated by reflected light from Saturn. Such a technique was successfully employed during the New Year's Eve 2004 encounter with Iapetus (see PIA06146 and PIA06169). This map was made from images obtained by both the Cassini and Voyager spacecraft. Cassini previously flew past Dione at a distance of approximately 72,100 kilometers (44,800 miles) on Dec. 14, 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . *Credit:* NASA/JPL/Space Science Institute |
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October 7, 2005 |
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Cassini Enters Saturn's Orbi
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the planet's rings. It was taken by the spacecraft's narrow angle camera and shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Cassini Enters Saturn's Orbi
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the planet's rings. It was taken by the spacecraft's narrow angle camera and shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Cassini Enters Saturn's Orbi
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the planet's rings. It was taken by the spacecraft's narrow angle camera and shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Cassini Enters Saturn's Orbi
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the planet's rings. It was taken by the spacecraft's narrow angle camera and shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Cassini Enters Saturn's Orbi
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the planet's rings. It was taken by the spacecraft's narrow angle camera and shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Cassini Enters Saturn's Orbi
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
Full Description |
After becoming the first spacecraft to enter Saturn's orbit, Cassini sent back this image of a portion of the planet's rings. It was taken by the spacecraft's narrow angle camera and shows the dark, or unlit, side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Cassini's First Picture of F
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Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
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This is one of the first images taken of Saturn's F ring by the Cassini spacecraft after it successfully entered Saturn's orbit. It was taken by the spacecraft's narrow angle camera and shows the sunlit side of the rings. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL |
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Craters of Tethys
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Craters of Tethys |
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Two large craters and hints of several smaller ones are visible in this Cassini image of Saturn's icy moon Tethys (1060 kilometers, or 659 miles, across). The image was taken in visible light with the Cassini spacecraft narrow angle camera on Sept. 23, 2004, at a distance of 7.9 million kilometers (4.9 million miles) from Tethys and at a Sun- Tethys-spacecraft, or phase, angle of 80 degrees. The image scale is 48 kilometers (30 miles) per pixel. The image has been contrast-enhanced and magnified by a factor of four to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . *Image Credit:* NASA/JPL/Space Science Institute |
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Intriguing Enceladus
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Intriguing Enceladus |
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This Cassini view of Enceladus hints at the curvilinear, groove-like features that crisscross the moon's surface, as seen in images from NASA's Voyager spacecraft. The image shows the trailing hemisphere of Enceladus, which is the side opposite the moon's direction of motion in its orbit. Enceladus is 499 kilometers (310 miles) across. The image was taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 27, 2004, at a distance of about 766,000 kilometers (476,000 miles) from Enceladus and at a Sun-Enceladus-spacecraft, or phase, angle of 34 degrees. The image scale is 4.6 kilometers (2.8 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . *Image Credit:* NASA/JPL/Space Science Institute |
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Dione Flyby Animation
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Dione Flyby Animation |
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This computer animation shows the observations to be taken by the Cassini spacecraft spanning roughly a nine-hour period surrounding its upcoming flyby of Dione on Dec. 14, 2004. Cassini will pass within 81,400 kilometers (50,600 miles) of the icy moon. Red indicates observations to be taken in the infrared, white in the visible, and purple in the ultraviolet. Green indicates radar observations. The name of instrument team that designed each observation -- Imaging Science Subsystem, Visual and Infrared Mapping Spectrometer, Composite and Infrared Spectrometer, Ultraviolet Imaging Spectrograph and radar, is shown. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org . Image Credit: NASA/JPL/Space Science Institute |
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Mimas in View
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Mimas in View |
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The Cassini spacecraft zooms in on Mimas, pitted by craters and slightly out-of-round. Cassini images taken during a flyby of Mimas in August 2005 were compiled into a movie showing the moon's battered surface up close (see Flying Over Mimas). This view shows the Saturn-facing hemisphere of Mimas (397 kilometers, or 247 miles across). North is up and rotated 24 degrees to the left. The moon's night side is dimly lit by Saturnshine, which is sunlight reflected by the planet. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Sept. 25, 2006 at a distance of approximately 552,000 kilometers (343,000 miles) from Mimas and at a Sun-Mimas-spacecraft, or phase, angle of 106 degrees. Image scale is 3 kilometers (2 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
Date |
October 17, 2006 |
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