Transit of Venus: Picture Gallery

   Laxfield solar observatory is open for business! The trusty refractor points skywards through the blackout curtains. And no, it wasn't in shade during the transit!!
   What every stylish telescope is wearing this summer - eclipse specs! The web-cam is visible as the white object next to the finder-scope at top centre: its cable is snaking away through the garage window.
And this is what we've been waiting for! At 6:20am Venus nicks the edge of the sun's disc and the transit begins.  
Twenty minutes later and it's "2nd contact" as Venus' silhouette is just fully visible.  
As the transit proceeds, the only moment of concern arrives when light cloud crosses the sun. Fortunately it soon clears and perfect conditions are restored once more.  
At 9:22am the maximum extent of the transit is reached as Venus passes closest to the sun's centre, but still only about 1/3 of the way in to the centre from the edge. This is slightly nearer than average, however, as it never gets particularly close to the centre.  
   A composite of eleven images taken from the projected view shows the naked eye appearance of Venus' track as the transit proceeds. For an explanation as to why the track is a curve and why it differs from the image below, see the last paragraph of the "Technical Info" page.
   And here we have an enhanced composite of images taken from the webcam to show that Venus' "true" track is indeed a straight line. This image has been rotated so that the sun's North pole is at the top (with East to the left). The slight gap in the track is due a tree getting in the way temporarily!
Third contact - 11:04am. Venus touches the edge of the sun and begins its departure.  
Just past 11:23am, and the end of the transit is upon us. Must be time for a late breakfast!  

   Just to show what can be done with relatively simple apparatus, this close-up was formed by projecting the image from the refractor onto a translucent screen: difficult to get in focus but very effective when you do.

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