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Transit of Venus |
REMEMBER - always take care when observing the Sun!
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!
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. |
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. |
An annotated view of the
view at left |
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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. |
Nearly over just as the
clouds came over and stopped any further observing or photography. |
Last image I took of Venus before it got lost in the glare of the Sun
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!