Saturn, Opposition 2006, 2007, 2008, 2009, 2011, 2016 |
Datas of Saturn |
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Diameter at equator |
120'536 km ( 9,4 x earth ) |
Saturn is the sixth planet from the Sun, and the
second largest in the solar system. The fascinating ring system is made of ice and
rock particles. It was noticed first 1610 by Galileo Galilei, but recognized as a real
ring 1656 by the Dutch physicist and astronomer Christiaan Huygens. |
Saturnpictures of the year 2002 to
2005 klick here
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7.6.2016, 22:06h UT Saturn 18" f , Horizonthöhe = 20° 140 / 980 mm Apo-Refraktor (TEC 140), F/23 3'000 / 10'000 Frames |
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140 / 980 mm Apo-Refractor
(TEC 140), F/23, LRGB, each channel 600 of
34000 frames added |
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The dark line across the planet is the shadow of
the ring. The ring itself in very thin. 140 / 980 mm Apo-Refractor
(TEC 140), F/25, LRGB, each channel 500 of
4000 frames added |
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20,1" f , 0.6 mag 140 / 980 mm Apo-Refractor
(TEC 140), F/45, 800 of 4000 frames added |
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140 / 980 mm Apo-Refractor
(TEC 140), F/48, 570 of 5000 frames added |
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This picture is a composit of two: Moons from left: 140 / 980 mm Apo-Refractor
(TEC 140), F/48, |
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Equator diameter = 20,4". The arrow points to a small bright spot south of a dark band. This is a storm in the upper atmosphere of Saturn. These storms are rare. They have a lifetime of some days to some weeks. I was lucky to "catch" such a storm. On the picture below is an animation, showing the rotation of the storm. Comparing the picture with those taken in the last years, it can be noticed, that the opening of the ring is now getting smaller. 140 / 980 mm Apo-Refractor
(TEC 140), F/56, 500 of 3000 frames added |
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Animation of two pictures. The second one was shot 18 minutes later than the first one. It shows the storm region (arrow in the upper picture) rotating with the planet. Saturn has a full ratotion in 10,5 hours. Taking the second video the seeing was much worse. So the second picture is not so good as the first one. Instrument and equipment the same as above. |
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