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As Venus moves closer to sliding behind the Sun, it is a view that no one but SOHO can see (June 4, 2008). Because its LASCO C2 coronagraph blocks out the Sun and some of the corona around it, SOHO can observe how the orbit of the relatively bright planet Venus carries it to a position directly behind the Sun as seen from the Sun-Earth line of sight. This position is called a "superior conjunction." SOHO is about one million miles (1.6 million km) towards the Sun and near the Sun-Earth line of sight. Venus is so bright that it saturates the CCD camera, making it appear much bigger and also causing "bleeding" along pixel rows (the bright horizontal streak on either side of the planet).
This reminds us that we can look forward to the next transit of Venus (when it will cross in front of the Sun as seen from Earth) on June 6, 2012. This will occur near sunset for observers in the U.S. And, this event will not occur again for more than another 100 years, so best not miss it.
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