Thursday, June 7, 2012

Transit of Venus 6 June 2012 from Sri Lanka




A transit of Venus is one of the rarest of all predictable astronomical phenomena. It occurs when the planet Venus pass over the visible face of the Sun as observed from Earth. Transits of Venus occur in pairs, separated by eight years. These pairs of transits are separated form the previous/next cycle by a period which can vary from approximately 105 to 122 years or so. Hence transits of Venus have been observed only eight times since invention of the telescope (c. 1610). In this century transits occurred on 8th June 2004 and 6th June 2012.

Observing a transit of the planet as it passes across the Sun’s disk requires special precautions due to the fact that an unprotected human eye can be severely damaged or even blinded by the Sun’s rays, especially its ultraviolet and infrared radiation.

I had observed and photographed the transit in 2004 and was extremely keen to observe the 2012 one. As I wished to share the experience I invited some others to join my wife and me in observing the phenomenon. We were joined by Enoka and Chris, Shiranie and Trevine, Hasantha and Rangitha. I fitted three binoculars, my vintage Asahi Pentax telescope and my forty-five year old Pentax Spotmatic (film) SLR with Baader AstroSolar(R) filters. Trevine brought his high-tech digital SLR with a 400mm lens which he used with a sheet of polyester solar filter film that I had. 






(Left) Setting up Equipment. I am fitting my solar filter equipped Audubon 8.5 x 44 binoculars on to a camera tripod. The binoculars gave an excellent view of the transit.






Observations were carried out from my home at Dampe which bears the astronomy station designation SXT 94 (see below). Wednesday 6th June started out with heavy clouds and drizzle and we were rather pessimistic about our chances of seeing the transit. Providentially the skies started to clear up at around 8.30 a.m. There was a rush to view the transit which was well in progress. Venus was seen clearly in silhouette against the solar disk along with several sunspots.                         


Coordinates of the observing station (SXT 94) are 6° 45’ 42”.25 N,   79° 55’ 27”.2 E   alt + 021msl


                                

Transit team
Transit team 2..

Binoculars with solar filter

Telescope and camera with solar filters

Shirani and Trevin photograph the transit.
                                              Trevine's images


  

                                                   Rex's image (processed)




                                                 

Heavy clouds appeared towards the end of the transit with the Sun being visible in occasional clear patches. I viewed the transit to its very end, but saw no “black drop” effect that has occasionally been reported in the past.

We were extremely fortunate to view this transit as the next one will only occur in approximately 105 years (i.e. 2117).


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