March 2010 | Diese Seite in deutsch |
| Index: | Links to Astronomy... |
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...with astronomical dusk/dawn for 52°31'30" North and 13°18'45" East at 3m above sealevel (StarryNight 2.0)
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1.: 04:59
11.: 04:36
21.: 04:10
31.: 03:42 (MET) | |
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1.: 06:55
11.: 06:32
21.: 06:09
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1.: 17:43
11.: 18:02
21.: 18:19
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1.: 19:39
11.: 19:58
21.: 20:19
31.: 20:41 (MET) |
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| 7.: 16:42 |
| 15.: 22:01 |
| 23.: 12:00 |
| 30.: 3:25 (MET) |
Illustrations: StarryNight 2.0 & -- jd --
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Saturn and its Moons, NASA Collage |
At the 10th of August 2009 the Sun gleamed directly onto the ring plane of Saturn so that neither the Northern nor the Souther side of the largest ring system of the Solar system was distinctively shone. This event was nearly not visible from Earth because Saturn seemed to be next to the Sun. But since the 1st of July 2004 an artificial moon circles around Saturn, the NASA probe Cassini, which could take a picture of this event within its "Cassini Equinox Mission":
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This month Saturn reaches its opposition position to the Sun, this means that Sun and Saturn are placed on a virtual line which goes throuth the Earth, where the Sun is on one side and Saturn on the other. The Sun now shines on the Northern side of the ring plane. As seen from Earth the ring opening is only 3.2 degrees:
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The exact date of the opposition position is March 22, 2010 at 2 a.m. The ringed planet will have a brightness of 0m.5 at the Earthen sky and a virtual diameter of 19.5 arc seconds. Even in a small telescope the oblateness of the planetary disc will be visible, because the polar diameter of Saturn will be only 17.4 arc seconds. Also in a small telescope the largest moon of Saturn will be visible: Titan with its 5150 kilometer in diameter:
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As the only moon of the Solar system Titan has a dense atmosphere and appears as a reddish shimmering dot as seen from Earth. Titan circles Saturn in a mean distance of 1.22 million kilometer within 15.945 days. Saturn has 61 moons in total, of which besides of Titan only Rhea, Dione, Tethys and under special circumstances Japetus can be seen from Earth with "normal" instruments. Only Jupiter has more moons than Saturn, that are 63.
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With 1528 kilometer in diameter Rhea is the second largest moon of Saturn and will reach a brightness of about 9m.6 as seen from Earth. It circles Saturn in a mean distance of ca. 527000 kilometer within 4.518 days.
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With 1118 kilometer in diameter Dione is the fourth largest moon of Saturn and will reach a brightness of about 10m.3. It circles around Saturn in a mean distance of ca. 377500 kilometer within 2.737 days.
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Tethys has a mean diameter of 1060 kilometer and with this its the fifth largest moon of the ringed planet. The maximum brightness of Tethys as seen from Earth is about 10m.1. Tethys circles around Saturn in a mean distance of ca. 294700 kilometer within 1.888 days.
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Japetus has a mean diameter of 1436 kilometer and with this its the third largest moon of the ringed planet. Its maximum brightness is about 10m.4, but its brightness varies much regarding which of its unequal bright sides is pointing to Earth. Japetus circles Saturn in a somewhat highly inclined orbit with a mean distance of 3.56 million kilometer within 79.331 days.
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The artificial Saturn moon Cassini will circle at least until the mid of this year around the ringed planet to send more pictures of Saturn, its rings and its moons to Earth.
As seen from Earth Saturn is located in the constellation of Virgo. March 29 the following situation can be seen at the Eastsoutheastern sky:
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Shortly after moonrise in the evening the two celestial bodies will have a distance of 9.4 degrees to each other. Also the following encounters between Saturn and Moon won't be that special. - The source of the Saturn pictures and the pictures of the Saturnian moons is the archive of the NASA Astronomy Picture of the Day (APOD). The moons of Saturn are also a topic of the Kosmos-Himmelsjahr in April 2010.
created: 2009-10-24 from German version
modified: 2009-10-25 translated
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