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RAL Observations of the
2004 Transit of Venus
  Logo showing the transit of 2004 June 8th
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2004 Transit of Venus Observations at the UK Hydrographic Office

Dawn broke on June 8th promising relatively clear skies and a good view of the passage of Venus across the solar disc. Sunrise occurred at 4:49 (BST) and the team observing the transit gathered outside R22, the main RAL lecture theatre, at just after 5 o'clock. The transit itself was due to begin at 06:20 (BST) when the Sun had climbed to just over 11° above the horizon. The question high in peoples' minds was whether the thin cloud close to the north-eastern horizon would threaten the early stages of the transit.

The team started work by setting up the telescope, an equatorially-mounted 105-mm Meade ETX Maksutov-Cassegrain with a lunar and planetary imager (a CCD detector) and a solar filter. Once assembled and its equatorial mount aligned with the north celestial pole, the prime focus imager was configured to provide a live feed to R22. The field of view of the detector was about 8 arcminutes by 6 arcminutes providing an impressively large image of Venus on the screen in the lecture theatre.

Projection of Venus crossing the disc of the Sun

By guiding the telescope on the Sun, many people in R22 could experience the transit in complete safety. The video output from the imager was also saved to a laptop hard disk and to an analogue video tape.

Using a solar filter in the presence of variable amounts of cloud can pose a problem. Without the filter on the telescope, the Sun would be far too bright for the imager. With it in place, too much light would be blocked, making the image too faint for the detector.

To provide an alternative method of viewing the transit, a second telescope, a 203-mm Meade LX10 Schmidt-Cassegrain, was set up to project the image of the Sun onto a piece of white card some distance from the telescope. The photograph to the left shows the projection of Venus crossing the disc of the Sun.

With the notable exception of the weather, everything and everyone was ready. Chris Davis, showing commendable foresight and a keen sense of occasion, had even remembered to bring a varied breakfast!

With exterior ingress only a minute or so away, cloud was still interfering with the view of the Sun. Steve Bell monitored the Sun through the eyepiece, ready to switch over to the imager when the cloud cleared. He was watching as Venus started to cross the limb on schedule and alerted everyone to the start of the transit. Fortunately, a few minutes later, the cloud had cleared sufficiently for the imager to be used. The live feed and the Recording started at around 6:35 (BST). The photograph to the right shows Steve Bell guiding the Meade ETX telescope during the latter half of the transit.

Steve Bell guiding the Meade ETX telescope
Chris Davis and Steve Bell monitoring the Meade ETX telescope

The internal ingress as well as the majority of the transit was recorded on disk without too many problems. As the Sun rose higher in the sky, the cloud dissipated quite quickly. As the temperatures climbed to around 27°C or so, keeping the telescope properly focused became more and more challenging.

To add a little extra excitement to the proceedings, the Meade ETX telescope ran into its end stops just before midday. Some quick thinking by Chris Davis suggested reversing the telescope. A rapid re-acquisition of the Sun was necessary to ensure the latter stages of the transit were captured for the audience gathered in the lecture theatre. Fortunately, only a few minutes of coverage were lost. The photograph on the left shows Chris Davis and Steve Bell monitoring the tracking and the focus of the Meade ETX telescope.

Many people at RAL saw the transit. Some saw it by projection on a screen in the R22 lecture theatre, some by viewing the projected image of the Sun on white card several feet from the telescope. Others saw it by using one of a variety of eclipse viewers provided for the event. The photograph to the right shows people using this type of viewer to watch the transit.

Although little new scientific information could be derived from the 2004 transit, the interest generated by the event could not be underestimated. Many, many people came to watch Venus cross the solar disc, some looking for phenomena such as the "the black drop", others to say they had seen something that no one living today had ever seen before.

Watching the transit with eclipse viewers
Children from Greenmere Primary School

Janet Haylett and Natalie Bealing arranged a visit by children from Greenmere Primary School to see the transit and to try and estimate the time of both the internal and external egress. Helen Walker gave a talk to these children on the planets and Venus in particular. They also tried out various activities including painting and making drawings linked with the transit.

Their headmaster, Richard Furniss, kindly commended RAL for the quality of the visit. The picture on left shows the some of the children pointing at Venus on a projection of the Sun.

Perhaps the memories of this event will get some of them up at sunrise on 2012 June 6th to see the latter stages of the only other transit of Venus in the 21st century.

For once, good weather blessed the event which stimulated a good deal of media interest from local newspapers, Six TV - The Oxford Channel and Central TV. In fact, we made the local 6 o'clock evening news on ITV.

The hot weather also encouraged some of us to bring out our more flamboyant shirts! The photograph to the right shows Pete Read aligning the Meade LX10 to project the image of the Sun.

The team involved in the transit of Venus observations were Chris Davis, Pete Read and Steve Bell. The R22 projection and analogue recording of the transit were looked after by Reg Jones. The photographs on this page were provided by Steven Kill and the video clips given below were produced by Nick Horan.

Steve Bell

Pete Read projecting an image of the Sun

Transit Videos

Video clips of three of the four contacts are available below. The times on the top of the video frames are good to approximately one second. However, the date was not set so it defaults to 01-01-01.

red arrow 2nd contact (interior ingress).
red arrow 3rd contact (interior egress).
red arrow 4th contact (exterior egress).
Transit information available:
Transit Home Page 1032 1040 1153 1275 1283 1396 1518 1526 1631 1639 1761 1769 1874
HMNAO Home Page 1882 2004 2012 2117 2125 2247 2255 2360 2368 2490 2498 2603 2611

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HM Nautical Almanac Office
UK Hydrographic Office
E-mail: hmnao@nao.rl.ac.uk
Last revision was made on 2007 November 5

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