Mercury and Venus Transit page


 All images are copyright Paul Money unless otherwise noted.

I hope you enjoy looking at them and perhaps may think to have a go yourselves.
Some of these images were originally taken on slide and print film and have been scanned and  transferred to CD Rom
where they have undergone slight brightness/contrast enhancement so they show better on these pages.
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Transit of Mercury
 Transit of Venus

REMEMBER - always take care when observing the Sun!

 Transit of Mercury May 2003

May 7th 2003 and Mercury crosses the disk of the Sun - called a Transit.

I (Paul) got up at 5 am (all times BST) and despite the cloud cover set up the 10" Newtonian with a Mylar solar screen, with an attached 3" refractor used to project an image onto a large board, the basic laptop to drive the 10" and a 2" refractor with mylar for extra viewing. By 06:11 Lorraine had joined me but despite a brighter patch of hazy sunshine the sun's disk could not be seen but as it happens the bund and shrubs on it would block out the sun until at least 06:30ish. Finally the clouds seemed to change direction of motion at around 07:45ish and by 08:08 Lorraine & I got our first clear view of Mercury on the solar disk. We had intermittent views for the next hour each view steadily getting better and longer as the sky began to clear and from approx. 9 am we had nearly continuous views until about 11 am with only the occasional spot of cloud to briefly spoil things. Took many photos and some of the pics came out - the best ones are shown here. The final 30 minutes had more interruptions with heavier clouds and although I saw part of the disk of Mercury at half off and then 2/3 off the solar disk, the clouds came over and prevented final contact being observed. Having said that it was a great experience and at least I got a large part of the event observed. Noted the large elongated sunspot closer to the centre of the Sun and Mercury was a smaller jet black disk and was more easily visible than even I had suggested in my book - Nightscenes 2003!

All in all I'm glad it was my day off work!

View of equipment at the start of the Transit This view shows how Lorraine and I had to have the telescopes nearer the house to get our first views of the start of the transit. Shown is the 10" Newtonian Reflector with a side mounted 3" Refractor projecting a view onto the lower card that lorraine is looking down at.
The view of the equipment later that morning This is the view later that morning when I had brought into play the 14" Dobsonian to project a 2 foot wide view of the Sun onto a large white card and another smaller telescope for visitors to view the Transit.
Whole Solar disk view of Mercury Transit Mercury is the small 'dot' in the upper part of the image whilst the larger 'splodge' nearer the solar disk centre is a Sunspot. Another set of Sunspots can just be seen on the right hand edge below centre.
Annotated image An annotated view of the view at left
An enlargement of the above image - click to view full size An enlargement of the above view showing just how small Mercury appears against the solar disk and compared with the sunspot group at the lower edge of the image.
The transit is nearly over Nearly over just as the clouds came over and stopped any further observing or photography.

Transit of Venus June 2004

This surely had to be one of the most eagerly awaited events of recent times with Transits of Venus visible in pairs approximately 8 years apart then a gap of either 105 1/2 years or 121 years. The next Transit of Venus will be in 2012 then we'll have a long wait until 2117 and 2125 so I'm really glad that on June 8th 2004 the weather was kind to us here in the UK and across many parts of the world where the Transit was visible.

Last image I took of Venus before it got lost in the glare of the Sun
Venus on Friday June 4th at 17:28 BST




Path of Venus across the Sun on June 8th 2004

Transits of Venus are historically important as it was realised by Edmund Halley that, by observing the start (or end) time from various points on the Earth’s surface, parallax could be used to determine the distance of the Earth to the Sun (known as the Astronomical Unit) and therefore the true scale of the Solar System could also be determined. Perhaps the most famous expedition has to be the one that took in the Transit of Venus in 1769 that involved HMS Endeavour, Capt James Cook, astronomer Charles Green and the Lincolnshire astronomer and naturalist Joseph Banks (not forgetting Joseph Gilbert from Wrangle, Boston, Lincs. Observing from the South Sea Isle of Tahiti they successfully recorded the event and the data combined with observations of the 1761 Transit put the Sun - Earth distance at 95 Million miles - impressive considering the average distance today is given at 93½ Million miles!

Attention was also drawn to the ‘black drop effect’ where once the Venusian disk was just inside that of the solar disk there lingered a sliver of black connecting the planets disk to the limb of the Sun. The expedition hoped that with their much superior instruments that the effect would be greatly reduced helping to improve the accuracy of their timings but even so it was still noticeable. This is something that to my observation  was not clearly apparent during the 2004 Transit perhaps due to using the webcams (see my simulation of the effect at left). The effect is due to the fact that Venus has an atmosphere so its disk is not as sharply defined. The Solar disk itself is not as sharply defined either due to its gaseous nature so the solar limb is also slightly blurry - put the two together and you can see why getting an accurate measurement of ‘first (and last) contact’ is actually quite a challenge. Note that in my simulation the atmosphere of Venus is greatly exaggerated to help show the effect. As with the Mercury transit, Venus was jet black against the disk of the Sun and so was unlikely to be confused with any sunspots that may be visible. Sunspots are great magnetic storms on the surface of the photosphere and often have a dark umbra surrounded by a lighter penumbra.

Interestingly at least three different motions are occurring whilst we observed this event. Firstly the Sun got higher in the sky as it was rising due to the turning of the Earth (which gives us day and night). Secondly the Sun was moving slowly along the ecliptic from right to left on the above chart due to the motion of the Earth orbiting the Sun and thirdly there was the actual motion of Venus in its own orbit about the Sun as it moves from left to right across the solar disk! It's an 8 year wait until the next and final transit of Venus in our lifetime! The second Transit is only partially seen from the UK and Ireland so I reckon that now is the time to start saving up for a very special holiday in 2012!

The day itself
I set up an array of equipment to both webcam the event live on the Internet and capture images both full disk view of the sun and close up with the 10" Newtonian Reflector thus I had 2 webcams on the go and switched between them. I also had the trusty 3" Refractor mounted aside the 10" and it projected a view onto a large card whilst there was also my 6.25" Binocular scope and a 6" Newtionian both with Mylar filters in place to give direct views for the numerous visitors we had during the transit - all of whom seemed to really enjoy the experience. Note that the weather was not perfect all through the transit and thus the quality of the individual images does vary - this is especially noticable in the animations. Note that I use UT (Universal Time) for the following images rather than the BST used on the transit chart shown above.


Transit Webcam1 Transit Webcam 1 (ToUCam Pro 740c) with a 135mm lens and a 2X convertor with Mylar filter to give the whole Solar Disk views. Note also the back of the 3" Refractor and the projection card for its image.
Transit Webcam2 Transit Webcam 2 (ToUCam Pro II attached to the 10" Newtonian Reflector and the laptop in a box (provided better contrast when looking at the screen). This gave the close up detailed views of the Transit. 
The view of the main laptop displaying the images live This is the view of the laptop displaying the live images collected from the webcams
and the Public dropped by as well! We had mentioned live on BBC Radio Lincolnshire that anyone living near enough could 'pop in' and view the event live from our garden and we had a steady stream of people including family and friends turn up during the Transit.
Animated Gif's
Whole Solar Disk view of Transit-animation This is the full disk animation view using Webcam 1
Animated Gif of the Ingress stage Animated Gif of the Ingress of Venus shortly after First Contact taken using the 10" and Webcam 2.  These are the first decent 7 images combined to give a feel of the motion of Venus as it crept further onto the disk. I missed the actual 1st Contact as there was problems with the web cam - fortunately quickly resolved!
Venus moves off the Solar Disk Animated Gif of the Egress of Venus off the Solar disk using the 10" and Webcam 2
Venus atmosphere at egress The Atmosphere of Venus showed up as a thin sliver of light as the limb of Venus started to leave the limb of the Sun and this was due to the scattering of sunlight around the limb of the planet - a sure sign that Venus has an atmosphere!
A selection of the still images
Whole Sun at 05:35UT 05:35 UT Whole disk view with Webcam 1
Whole disk view at 07:25UT 07:25 UT
Whole disk view at 09:04UT 09:04 UT
Whole disk view at 10:18UT 10:18 UT
and so it begins... Ingress 05:25UT
Nearly on Ingress 05:38UT
Just a sliver left Ingress 05:39UT
Well on the disk now Ingress 05:51UT
The big black disk on the Sun 07:00UT and Venus is a big black disk on the Sun
Closest image to mid transit 08:18UT this is the closest image to mid transit I managed to get (Mid transit around 08:22UT)
Heading for the other limb now 10:44UT heading towards the other limb now and soon to be over for 8 years.
closing the gap 10:58UT closing the gap now
beginning of the end of the transit 11:05UT moving off the disk
Half off the disk now 11:11UT virtually half off the disk and it's almost over.
The interesting extra that was not observed visually by myself or any of our visitors but was captured with the close up webcam was the faint glow of the atmosphere of Venus as it's disk began to leave the Solar disk. Here are 3 enhanced images showing the effect of the scattered light around the disk of Venus giving proof that the planet has an atmosphere.
The atmosphere of Venus beyond the limb of the Sun




ã Paul L Money 2005