The transition of Venus in 6/6/2012

I used the Stellarium to simulate the transition of Venus in 6/6/2012. I found that the path of Venus on the sun disc during the transition would be funny. In contrast to that of 2004, which is basically a straight line, http://www.hko.gov.hk/gts/event/event-v ... nsit_e.htm, the path is a non-trial curve with non-uniform speed. The first contact will be at about 06:08. It will move on a curve of small curvature. As it approaching the edge of the sun at about 12:00, it will not leave the sun but will move close to the edge and accelerate within the sun accordingly. It will move about 180o, half of the circumference of the sun, and finally will leave the sun at 12:42. This means that it moves slowly on sun surface relative to an observation on Earth for about 6 hours and moves fasters for the last 40 mins. I don’t know whether there is error in the simulation. I counter checked the 2004 transition with Stellarium. The result was the same as Hong Kong Observatory. Anyone can try this in Stellarium and see if there is the same result.



