Venus transits occur in pairs about 8 years apart, but with more than a century between different pairs. The 2012 transit was preceded by a transit in 2004, but the next two transits won't take place until 2117 and 2125. Historically the transits of Venus were very important because they were used to determine the distance between Earth and the Sun.
For more information about this fascinating topic, see www.transitofvenus.org. The remainder of this page focuses on observations of the Venus transit made at Berry College.
The equipment for the transit viewing included two 8-inch Celesteron Schmidt-Cassegrain telescopes with solar filters. One of these telescopes was dedicated to photography and video recording of the transit, while the other was used to allow visitors to view the transit.
A small crowd (it was summer, after all) of Berry students, faculty, and staff and other interested people gathered to observe the transit starting around 6 PM (before the start of the transit) until after 8:30 PM when the sun was no longer visible. The transit lasted until about 1 AM on June 6 (Eastern Daylight time), but the second half of the transit was not visible from Georgia. The images below show the group gathered to see the transit, as well as Kalen photographing the transit.

![]() 6:19:13 Disk of Venus partially visible at the upper right limb. |
![]() 6:38:03 Disk of Venus fully visible. |
![]() 7:33:20 Disk of Venus has moved toward interior of solar disk. |
![]() 8:06:03 Some clouds in the way. |
![]() 8:09:48 Sun begins dropping behind some low-lying clouds. |
![]() 8:10:00 More cloud cover. |
![]() 8:30:24 Lots of clouds covering the bottom of the Sun. |
![]() 8:30:54 Our last image of the transit. |
