Society for Popular Astronomy
Partial Eclipse of the Sun
Saturday, October 12
Live Images of the Eclipse
![[Eclipse Photo]](/file/1091/CU Amiga Magazine's Super CD-ROM 18 (1997)(EMAP Images)(GB)[!][issue 1998-01].iso/CUCD/WWW/http/www.u-net.com/ph/spa/eclipse/eclphoto2.gif)
Example of what you may see.
© Copyright Robin Scagell, (No copying). |
There will be a partial eclipse of the Sun visible from the UK and other
parts of Europe on Saturday 12 October 1996. This will be the largest
partial eclipse visible from the UK since 1961 - if the weather
is clear it should be a memorable sight.
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People often remember partial eclipses of the Sun that they saw when they
were young, and this should remain in the memories of many youngsters.
But as far as the UK is concerned, it's just the prelude to the Big One -
the total eclipse due on 11 August
1999. But what is the difference between a partial and a total eclipse?
Eclipses happen when the Sun, Moon and Earth are exactly in line. As the
Moon goes round the Earth, it occasionally hides the Sun from view, or
else it passes through the Earth's shadow. Because its orbit is slightly
inclined to the Sun's path through the
sky, this does not happen every New Moon or Full Moon.
When it gets between us and the Sun, we see its dark outline pass in
front of the Sun, and it is called an eclipse of the Sun. In the other
situation, where it passes through the shadow of the Earth, the Moon
itself dims and we see an eclipse of the Moon.
There was an eclipse of the Moon on 27 September.
Why your location matters
To see an eclipse of the Sun, you have to be in the right spot. The Moon
is just over 2000 miles across, so when it passes in front of the Sun it
casts a shadow of that size on the Earth. Actually, that is only true
near the Equator - if the shadow happe
ns to fall nearer the poles, it will be elongated. Within a few hundred
miles of the centre of the shadow, the Moon can completely hide the Sun
and people in the favoured area see a total eclipse. Outside that area,
the Moon does not completely cover the
Sun and a partial eclipse is visible.
On 12 October, however, there won't be a total eclipse anywhere because
the central part of the Moon's shadow misses the top of the Earth
completely. In the UK we will see about half of the disc of the Sun
covered, those in the north seeing more eclipsed
than those in the south.
When to look
The eclipse takes place on the Saturday afternoon. The exact timings vary
slightly depending on where you are, as shown in the following table.
Eclipse timings for various locations around the UK
Location Start of Middle of End of Maximum area
eclipse eclipse eclipse of Sun
(BST) (BST) (BST) covered
Aberdeen 13.49 15.06 16.20 56%
Belfast 13.47 15.06 16.21 52%
Birmingham 13.55 15.14 16.28 51%
Cardiff 13.55 15.14 16.28 49%
Dover 14.01 15.20 16.33 51%
Edinburgh 13.49 15.07 16.21 54%
London 13.59 15.18 16.31 51%
Manchester 13.53 15.12 16.26 52%
Newcastle 13.52 15.10 16.24 54%
Norwich 13.59 15.17 16.31 53%
Plymouth 13.55 15.15 16.29 48%
Southampton 13.58 15.17 16.31 50%
Very soon after the time shown for the start of the eclipse, you should
see the Moon's disc start to move onto the Sun. The maximum area, at
mid-eclipse, is the actual area of the Sun covered rather than the
percentage of its diameter. The the Moon starts
to move off again, and its disc will completely clear the Sun by the
last time shown.
![[Diagram showing stages]](/file/1091/CU Amiga Magazine's Super CD-ROM 18 (1997)(EMAP Images)(GB)[!][issue 1998-01].iso/CUCD/WWW/http/www.u-net.com/ph/spa/eclipse/diag.gif)
How the eclipse will look in its early, middle and late stages
How to observe the eclipse
Observing an eclipse of the Sun can be very dangerous if you're not
careful. We often underestimate the power of the Sun - following an
eclipse in 1984, many people suffered from eye problems as a direct
result. The important thing to remember is that just cutting down the
light is not enough. Heat rays - invisible infrared light - are just as
dangerous, and many dark materials can be transparent to infrared.
There are ways of using telescopes and binoculars safely, but if you do
not have these there are a few methods you can use.
Filters
Everyone seems to have heard of using smoked glass, but this is not now
recommended because of the infrared problem. Photographic filters come
into the same category. Welder's glass is suitable, as long as it is No
14 or darker.
At one time, people used dense black and white negatives, but again this
is no longer always ideal. Colour film and some modern black and white
film, such as Ilford XP-1, use dyes rather than silver, and let through
infrared. If you have overexposed and developed silver-based black and
white film which is really dense, then observing through one or two
thicknesses of the densest part may be adequate.
Well-equipped amateur astronomers use specially made filters over the
front of their telescopes, but these are expensive and are not easily
available. You can, however, now buy card-mounted spectacles of the same
material. They can be obtained from Eclipse 99 Ltd, Belle Etoile, Rue du
Hamel, Castel, Guernsey GY5 7QJ. Tel 01481 64847. The price for one set,
including a leaflet and postage, is 1.99 UK pounds. Credit cards
are accepted. Eclipse 99's e-mail address which is
100334.1671@compuserve.com.
Broadhurst, Clarkson and Fuller can provide safe eclipse viewing filters for
£1.95 post free. 63 Farringdon Road, London EC1M 3JB. Tel 0171-405 2156.
Beware! The sun filters supplied with some small telescopes should never
in fact be used on the telescope for direct observation. They are
intended to be screwed into the eyepiece, but they can overheat and
shatter.
Don't look through the viewfinder of your camera if it is pointed at the
Sun, even if you have a dense filter over the front of the lens.
Projecting the Sun's image
This is the only safe way to observe the eclipse.
![[Binocular Projection]](/file/1091/CU Amiga Magazine's Super CD-ROM 18 (1997)(EMAP Images)(GB)[!][issue 1998-01].iso/CUCD/WWW/http/www.u-net.com/ph/spa/eclipse/binproj.gif)
If you have a telescope or binoculars, point it at the Sun. In the case
of a telescope, make sure that any small finder telescope is capped, and
keep the cover on one half of the binoculars. The easiest way to find the
Sun is tilt your instrument to get the smallest shadow.
![[Projected Image]](/file/1091/CU Amiga Magazine's Super CD-ROM 18 (1997)(EMAP Images)(GB)[!][issue 1998-01].iso/CUCD/WWW/http/www.u-net.com/ph/spa/eclipse/project2.gif) |
Hold a piece of white card about 15 cm (6 inches) behind the eyepiece to
act as a screen on which you can catch the image. You should see a bright
circle of light, probably blurred, on the screen. Focus the instrument
until the circle is sharp. This is the disc of the Sun itself. If the
eclipse is in progress you should see the Moon
as a dark bite out of one edge.
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Moving the card farther away gives a larger but fainter image, and vice
versa. Fixing the instrument firmly on a tripod helps enormously. The
advantage of projection is that many people can see the image at once.
![[Pin Hole]](/file/1091/CU Amiga Magazine's Super CD-ROM 18 (1997)(EMAP Images)(GB)[!][issue 1998-01].iso/CUCD/WWW/http/www.u-net.com/ph/spa/eclipse/pinhole.gif)
If you have no telescope, you can actually project a faint image of the
Sun through a pinhole in the same sort of way. Get a bit of card - a good
old cereal packet is fine - and use a drawing pin to make a hole about 1
mm across. Hold your screen about 15 cm behind this and you should see a
small image of the Sun on it. Again, the farther away it is the larger
and fainter it becomes.
Also see Other Methods of Observing the Eclipse.
Photographing the eclipse
![[Photo]](/file/1091/CU Amiga Magazine's Super CD-ROM 18 (1997)(EMAP Images)(GB)[!][issue 1998-01].iso/CUCD/WWW/http/www.u-net.com/ph/spa/eclipse/partial3.gif)
The simplest method is to photograph the projected image. If you have a
suitable filter you can put this over the lens of your camera to cut down
the light when photographing directly. But bear in mind the warnings
about photographic filters letting through infrared.
The camera's standard lens will give only a small image of the Sun. You
really need at least a 135 mm telephoto to give a decent sized image.
Getting the exposure right is a big problem. Automatic exposure meters
see a small bright disc with a dark surrounding and try to balance the
two, overexposing the Sun. Experiment with a stop or two less exposure
than the meter suggests.
Things to look for
There may be one or two sunspots - dark areas on the Sun's disc - but at
the moment the Sun is at a quiet stage in its solar cycle and there may
not be any. If there are, and the Moon's disc happens to cut across one,
you should see that the Moon is still dark against the sunspot. This is
because the spots are only dark in comparison with the rest of the Sun -
they are still quite bright.
You may be able to see that the Moon's edge (technically called the
'limb') is not completely smooth. Its mountains and craters can be seen
in profile if you look carefully.
The limbs of the Sun and Moon may seem to be in constant motion, rippling
up and down. This is caused by the Earth's unsteady atmosphere.
You should not see any features beyond the Sun's limb. The dramatic pink
prominences which you have seen in pictures are far too faint to be
visible, and only appear when the Sun is totally eclipsed.
Look beneath trees to see crescent-shaped images of the Sun and
mid-eclipse, caused by the gaps between leaves acting as pinholes.
Dos and don'ts
- Do make sure that you are properly equipped before the event rather than
rely on anything that comes to hand at the last minute
- Do tell children and others not to look at the Sun directly
- Do enjoy what is a rare and beautiful event
- Don't look at the Sun directly, not even through a pinhole
- Don't take chances observing through materials that look dark, even if
they seem OK at the time. Your eye is not sensitive to infrared so there
is no reflex action to prevent damage.
A study of patients who went to just one hospital in Manchester after the
1984 partial eclipse showed that five had looked at the Sun directly,
three looked directly though a pinhole, two used black plastic bags, one
wore two pairs of sunglasses and another used a camera with two filters
attached.
Warning
Neither the Society for Popular Astronomy, nor anyone responsible for the
production or distribution of this material, shall be liable for damages
arising from the use of this information.
The Society for Popular Astronomy
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astronomy as a hobby. We help enthusiasts of all ages to enjoy the fun
of observing, and there are special sections to cover particular areas of
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Astronomy site of the day 10/11/96