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Mercury
in the early morning sky
There
will be a fine opportunity at the end of the month of September
(always weather permitting) to see the planet Mercury in the early
morning sky before dawn.
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Dia
1: Looking east September 24 at 05 45 BST (Click the image
for enlargement)
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On
the morning of the 24th September Mercury will rise at 05 10 BST,
approximately fifty minutes before sunrise.
The
diagram (1) shows Mercury in company with the crescent Moon and
Jupiter at 05 45 BST. At this time Jupiter will be nearly five times
as bright as Mercury. Never the less, Mercury will be brighter than
the bright star Procyon which resembles the planet in colour .
Mercury
moves swiftly eastward under Leo during the course of the next few
days increasing substantially in brightness the while. It may be
visible to the naked eye up to and around 12th October after which,
despite its brilliance, twilight and sinking altitude will make
observation progressively more difficult.
J
V 18/09/03
Choosing
a Binocular
Catering
for the wide range of people likely to access this site we shall,
from time to time, include features of general interest.
Choosing
a binocular.
1)
All-purpose work.
The
main factors to consider are ease of use and effectiveness. Anything
above x8 magnification will be difficult to hold steady for the
majority of users. A light-weight binocular is not necessarily easier
to hold still than a slightly heavier one (for observations of short
duration - about a minute, maybe). The binocular should feel comfortable
in the hands. Always use both hands where possible. There is little
to beat the 8x30 combination of power and aperture for general use.
Remember, the ease with which you can accommodate the emerging light
from the eyepieces is determined by the size of the exit pupil.
The smaller the exit pupil the more critical the eye separation
distance and the more fussy the binocular is to use. (Anything under
3.0 mm falls into this category - see below.)
Most
binoculars have a central focusing wheel with adjustment to the
right eye at the eyepiece. This is to enable the differences between
right and left eye to be accommodated and once set for a given user
should not require adjusting too often. The individual eyepiece
focusing design is usually to be found with 7x50s. This is of advantage
where one is usually observing distant objects (astronomy) and the
focusing setting remains relatively "fixed" for the same
observer.
2)
For use in poor light, 8x40 is strongly recommended. For very poor
light, 8x 42 or 7x50. (For some reason manufacturers avoid 8x50
which is in many ways better than 7x50 since too wide an exit pupil
- larger than the pupil itself - means wasted light).
3)
For bird watching, and for detail at not too great a distance, try
10x40 or 10x42.
Testing
a binocular
Test
the quality of the image for colour - blue fringes to white objects
are a bad sign. Your binocular should focus to give a clear, natural
image with minimal distortion across the field of view. Also make
sure you can focus on close-up objects. For really close work (birds,
say) roof prisms, all else being equal, give the best results. "Double
imaging" (see cautionary footnote) can sometimes occur even
in new instruments. Always be on the lookout for this defect especially
in second-hand binoculars. Inspect the lenses for scratches and
abrasions. Look into each object lens from the front to ensure the
internal prism system is free from discolouration - the un-cementing
of prisms can occur in older instruments.
Binocular
design.
The
two designs most commonly encountered nowadays are the German classical
prism system (the American system is similar), and the roof prism.
In the latter the main lens (object lens) and the eyepiece lens
are in-line. Such binoculars usually enclose all mechanical focusing
parts within the body of the instrument and are therefore dust proof
and sometimes waterproof as well; as a result, they are generally
more expensive than other types. A definite advantage for bird watching
etc. is that the roof prism binocular suffers less from parallax
effects when observing objects at distances of less than 15 metres
or so. Compactness is another plus point; but be WARNED, quality
can vary enormously. Even quite expensive roof prism binoculars
can be outclassed by lower priced older designs from good manufacturers.
The old Eastern Germany Carl Zeiss firm produced fine binoculars
known as the Binoctem and the Deltentum (Deltrentis for individual
eyepiece focusing) ranges. These still come onto the second-hand
market from time to time at reasonable prices.
Pocket,
or compact binoculars. These are almost without exception of the
roof prism design. Remember the earlier remarks on size and weight.
The only way to decide on performance is to compare one binocular
against another on the spot and therefore under identical conditions.
Because
these instruments use small objective lenses (usually 20mm) the
exit pupil will be correspondingly small and therefore the eye separation
distance becomes more critical (getting both eyes lined up with
the eyepiece). There are many inexpensively priced binoculars in
this class. Most give relatively poor light and may have a blue
cast. With compact binoculars, even more than with larger instruments,
you tend to get what you pay for in terms of quality.
Astronomical
use
A
good binocular can provide very rewarding views of the night sky
not accessible to a telescope. A binocular has a wider field of
view, for one thing, and two eyes are better than one for wide-field
work. The Pleiades and the Beehive Cluster, for example, show well
in a small binocular and the Andromeda Galaxy can look impressive
in a pair of 7x50s. For comets 10x42 is generally preferable to
something with a larger aperture and lower power since magnification
is important. Another factor to bear in mind when viewing objects
in a twilight sky, or a sky badly affected by light pollution, is
that so-called twilight value works to our disadvantage. (See explanation
for "stellar enhancement".) For wide-field astronomical
work the old Zeiss 7x50 Binoctem is a very useful tool. The same
firm also produced a 10x60 glass of the German design. Anything
larger than this would be difficult to use without a mounting.
For
serious comet searching 15x80s would be a good compromise. Instruments
of reasonable quality of this size may be had for around £260
- £300; 25x100 for a little under £500. Cost escalates
once one moves up into larger binoculars of quality - you may expect
to pay at least £1500 for a good 20x100 (or 30x100). A tripod
is, of course, essential and will add to the above costs. The much
larger, and therefore weightier, 30x150 instruments used by serious
comet hunters will be beyond the aspirations of most people.
It
is important to bear in mind that as soon as a power greater than
x10 is used, whether in a binocular or small telescope, hand shake
becomes significant. There are now binoculars available with compensating
mechanisms for movement and shake. These instruments are more expensive.
Although many people may find such binoculars handy for all-round
use, conventional designs - tripod mounted - will be more useful
for astronomical work.
Sample
binocular specifications
Mag./Aperture Twilight Relative Stellar Exit
'm' 'a' Performance Light Enhancement Pupil
(mm)
6 X 20 8.16 40 49 3.3
8 X 20 7.07 40 56.5 2.5
10 X 25 7.9 62.5 79 2.5
8 X 30* 10.6 90 85 3.75
7 X 35 13.2 122 105 5.0
8 X 40** 14.1 160 113 5.0
10 X 40 12.65 160 126.5 4.0
7 X 42** 15.87 176 111 6.0
10 X 50 15.81 250 158 5.0
7 X 50** 18.9 250 132 7.1
8 X 56 19.8 313 158 7.0
15X 60 15.49 360 232 4.0
16X 70 17.5 490 280 4.4
20X 80 17.8 640 358 4.0
'a'
= aperture (mm).
'm' = magnification.
In the first three columns, efficiency is proportional to numerical
value.
*
Recommended for general use.
** Recommended for terrestrial use in conditions of poor light.
Anything above x10 magnification will require a support system -
tripod etc.
Notes:
Twilight
Performance: This represents the field brightness. A
higher magnification at the same aperture will have the effect for
an extended object of 'spreading' the available light thereby producing
a fainter image.
Relative
light. This is the 'light collecting' capacity for a given instrument.
For a point source (e.g. star) it is purely a function of the relative
'surface area' of the object lens. But for an extended object the
same principle applies as for twilight etc. and magnification becomes
a significant factor.
"Stellar
Enhancement":
When a point source (e.g. star) is observed against a continuous
background, magnification has the effect spreading or 'diluting'
the background light, thereby increasing the perceived contrast
between the background and the point source. A star will appear
brighter, therefore, the higher the magnification for a given aperture.
Exit
Pupil: The diameter of the cone of light leaving the
eyepiece. This can be demonstrated by holding the binocular at some
distance. The small illuminated disc seen in the eyepiece is the
exit pupil. The fully dilated pupil for the average human eye is
8mm.* This will be smaller, depending on the brightness of the light
perceived. Consider half this value for the eye working under daylight
conditions. There is little to be gained by having an exit pupil
much in excess of this since the light cannot enter the eye and
would tend to be 'wasted'. On the other hand, a too small exit pupil
means the eye will have more difficulty locating it. (This usually
arises when using compact instruments e.g.. 8 x 20, 10x25.)
Note:
magnification may be calculated by dividing the diameter of the
object lens by the aperture of the exit pupil.
*
This decreases with age - of the user, not the instrument!
CAUTION:
Always carry your binoculars with a strap or lanyard slung from
the neck. It is all too easy to drop binoculars. Even if you are
fortunate enough not to break the lenses the internal prisms will
almost certainly suffer. Binoculars damaged in this way give "double
images" and will have to be re-aligned by an expert.
J.Vetterlein.
1992/93 (updated 2003)
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