Visual Observation of the Deep Sky
Jay Reynolds Freeman
IS DEEP-SKY OBSERVING?
means "beyond the solar system". It includes galaxies, star
clusters, and nebulae. Some people add double stars or variable
stars too, and I won't argue, but for the sake of brevity
I will not discuss those objects here.
What about the "observing"? I should make clear that I only
mean visual observing. I have little knowledge of photography
or electronic imaging, and that's not what I am interested
People who do the kind of observing I am talking about are
not really doing science. Many deep-sky observers would recognize
something of scientific interest if they saw it, and would
be able to contact scientists who might want to study it further,
but that's not why most of us are there. If galaxies were
birds. then what we do would be called bird watching, not
ornithology. "Cosmic bird watching" might be a good catch-phrase
for what deep-sky observing is all about.
OBSERVE THE DEEP SKY?
The only real answer to that question is "Because!". This
is a hobby who needs a rational explanation? Some people
do cosmic bird-watching because the birds are pretty, some
do it to see lots of different species, some like to study
a few favorites in detail, and some like to handicap themselves
deliberately in some way, such as by restricting telescope
size or observing time, to make things more fun and more challenging.
Deep-sky observing has different aesthetics and challenges
than lunar or planetary work, though it is hard to describe
just what the differences are. They mostly stem from deep-sky
objects being generally much fainter than the Moon or most
of the planets. Lunar and planetary work generally involves
looking for details that are hard to see, on objects that
are easy to see. Deep-sky work often involves trying to detect
objects that are hard to see in the best of circumstances.
Sometimes those objects are almost impossible to see. We use
terms like "faint fuzzy nothing" and "lumpy darkness" to describe
them. We make obscure references to the "elusive Elvis nebula".
(Some people think that the "King rate" selection on a sidereal
drive is for tracking the Elvis nebula.) The general consensus
is that a good deep-sky observer would make a fantastic spiritualist
medium once you've found some of the stuff we look
at, seeing a ghost is easy, in comparison.
There are even some pragmatic reasons why an amateur astronomer
might pick deep-sky work over other sides of the hobby. For
example, deep-sky observing does not require perfect seeing
the air does not have to be perfectly steady to do
it. It does not require as large and as perfect a telescope
to look for deep-sky objects as to chase down fine and subtle
lunar or planetary detail. There are lots more deep-sky objects
than there are large moons and planets in the solar system,
too, and they are available year 'round. As I write these
words, planetary observers have just gone through several
months during which no bright planets were well placed in
the evening sky. Things like that don't happen with deep-sky
HARD IS DEEP-SKY OBSERVING?
The perception of how difficult it is to detect various deep-sky
objects has changed dramatically over the years, mostly in
the direction of "it's not as hard as they say." Some of this
change is because equipment has gotten better and cheaper
over the last several decades. High-quality telescopes and
binoculars, and in particular, large telescopes, are much
more common now than they were a generation ago, and cost
much less in comparison with other consumer goods.
But not all of that change has to do with hardware. Thus for
example, a generation ago, the Pelican Nebula, located east
of Deneb and just south of the brighter and better-known North
American Nebula, was considered by many to be unobservable
visually, with any equipment. These days, it's not uncommon
for observers at dark sites to report it with the naked eye.
Today's eyes aren't any better than eyes a generation ago.
Today's skies aren't any darker, rather the reverse!
Thus at least some of the increased ease of deep-sky observation
stems from increases and improvements in observing skills,
and from those skills becoming more widely known than before.
Let me illustrate the benefits of observing skill and experience.
At a star party I once attended, a relatively inexperienced
observer, had bought a 15- or 18-inch Dobson, and was looking
for the Horsehead Nebula. The Horsehead is pretty faint, and
he was having trouble locating it. I know the field for the
Horsehead, so I offered to help. Yet when I stepped to the
eyepiece, what do you know? He had it centered! The object
he was looking for was right square in the middle of the field
of view, but he couldn't see it!
Now, the reason I could and he couldn't was surely not that
I have superior vision: I know that I don't, because I have
compared notes with many other experienced observers, and
generally, we can all see about the same things in similar
circumstances. But I do have a lot of experience, and I have
deliberately worked hard to try to develop my observing skills.
In my opinion, that made all the difference. I hope you will
excuse my talking about it, because I am not really boasting
there's nothing I have learned to do that you can't
learn to do just as well, and perhaps knowing of my experiences
will make you decide to try.
Let me give another example. At another star party, the owner
of an eighteen-inch Dobson had chased down NGC 6822
Barnard's Galaxy which is fairly large in angular size,
but has a relatively low surface brightness. It is fairly
difficult to see, and the owner of the big Dobson was legitimately
proud to have located it. I asked if he would like to see
it in my telescope, and led him over to the 90 mm refractor
that I had set up on the other side of the observing area.
At first he couldn't see a thing, but after I reminded him
about averted vision, shielding the eyes from stray light,
and a few other tricks, he did indeed see the galaxy in the
Think of that: Knowing HOW TO SEE, allowed users of my tiny
telescope to detect something that other people were finding
difficult with FIVE TIMES as much aperture. That's a big difference.
Actually, Barnard's galaxy was discovered by Barnard
using a five-inch refractor visually, and of course,
Barnard didn't already know it was there. Yet he did know
how to see, and was therefore able to discover it with an
aperture that many people consider too small to see it with,
even when you know where to look.
Knowing just where to look for an object does make a lot of
difference: With that advantage, I have seen Barnard's galaxy
with a 7x50 binocular. I didn't tell that to my friend with
the 18-inch Dobson, though: He was bigger than I was.
Anyhow, I hope it won't surprise you, that in my opinion,
the most important part of my presentation will be about observing
skills. Yet there are a few other things I want to talk about
FANCY IS THE REQUIRED EQUIPMENT?
Although perhaps as forty Messier objects are visible to the
naked eye, and several score other deep-sky objects as well,
nevertheless, I do recommend that you use a telescope or a
binocular for deep-sky observing. To help decide what equipment
to use, I am going to suggest three rules. I will give the
first two immediately, and save the third for later. The first
two rules may seem contradictory, so I am going to talk about
them at some length. But first, let me state them:
me restate rule one: APERTURE WINS, and it wins big. There
is no substitute for large aperture, for visual observation
of deep-sky objects. With rare exceptions, mostly for objects
that are large in angular size, a telescope which collects
a large beam of light will show a better and more easily seen
view of deep-sky objects, than will a smaller instrument.
There are a lot of manufacturers of small telescopes
sometime very expensive small telescopes who would
like you not to believe it, but in my opinion they are all
wrong. An excellent small telescope is at best only a small
telescope. I repeat once more: APERTURE WINS.
On the other hand, just because aperture wins doesn't necessarily
mean that the biggest telescope is the best one to get. There
are many reasons why. Lots of aperture costs lots of money,
perhaps more than you can afford, particularly if you are
just starting out in astronomy and aren't sure how much you
are going to like it. Possibly you do not have enough space
to store a big telescope, or a car sufficiently large to haul
it to an observing site, or time, strength, and energy to
set it up and take it apart when you are done. Maybe you like
using a little telescope because it is more convenient. Or
maybe you prefer a small telescope just because the small
size makes it more fun and challenging: After all, some folks
who go fishing take great delight in landing humungeous fish
with light tackle why shouldn't observing be like that?
These remarks lead to rule two: You don't need large aperture
to do deep-sky observing. Again, I hope you won't mind if
I draw some examples from my own experience.
One thing I like to do to familiarize myself with a new telescope
or binocular, is to do a Messier survey with it to
go through all of the deep-sky objects discovered by the great
French comet-hunter, Charles Messier, and his close colleagues.
I have done that nineteen times so far, with nineteen different
instruments. Three of them had apertures of 50 mm 7x50
and 10x50 binoculars, and a Meade 50 mm refractor. The first
Messier survey I ever performed, which was when I was a quite
inexperienced observer, was with the 7x50 binocular, and I
did indeed find all 109 Messier objects. That proves it doesn't
require either great aperture or great experience to do it.
On the other hand, it did take persistence, dark sky, and
a whole lot of tricks.
One instrument I have used a lot lately is an exquisite small
refractor, made by Vixen, whose objective is only 55 mm in
aperture. I haven't finished my Messier survey with it yet
I haven't had it long enough for all the objects to
be visible in evening hours, and I am too lazy to stay up
all night and get the rest. Yet I have also started another
survey of fainter objects, going through the Astronomical
League's Herschel-400 list. It is a selection of 400 of the
brighter of the 2500 or so objects discovered by the great
observer, William Herschel. I have only logged about 160 of
those objects so far, but those include the two that seem
to be most difficult NGC 6118 and NGC 6540, so I suspect
the little refractor will do it.
I have an internet friend who is in her late teens. She was
given a 50 mm Jason refractor a few years ago one of
the kinds commonly called "drug-store junk refractors", that
are quite properly shunned by serious amateur astronomers.
She was a complete beginner, and the 50 mm Jason was her first
telescope. Nonetheless, she started a Messier survey with
it, and last I heard, had only four objects left to go.
Yet there are many experienced amateurs who think it takes
a six- or eight-inch telescope to see all of the Messier objects,
and one half again or twice as large to tackle the Herschel
400. I hope I have convinced you that isn't necessarily so.
Now, people who observe in light polluted conditions may need
a larger telescope to do deep-sky work though the 93
Messier objects I have logged so far with my 55 mm refractor
have all been seen from my yard in suburban Palo Alto. Yet
for the most part, folks who complain that they can't see
deep-sky objects with a telescope six inches or more in aperture,
are not complaining about the telescope, they are complaining
about their own lack of ability, or rather, their own lack
of will to sit down and learn how to see what their telescope
can show them.
And that brings me to one area in which small telescopes do
not fail in comparison to larger ones. That is the third rule:
RULE THREE: You can develop observing skills just as well
with a small telescope as with a large one.
three does not provide an escape from rule one APERTURE
WINS but it does provide you with something interesting
and challenging to do with a small telescope. As I have already
discussed, there are plenty of things to look at with such
an instrument, and rule three means that while you are looking,
you can learn and practice skills that will transfer to larger
equipment when you get to use it.
The point of rule three is that it takes just as much effort,
and just as many tricks, to see a 12th magnitude galaxy with
a two-inch telescope, as it does to see a 15th magnitude one
with an eight inch. All that changes is the scale of things
the eight inch might just as well be looking at the
same object as the two inch, only four times as far off. If
you develop the skills to see 12th or 13th magnitude objects
with a two-inch telescope, then when you get hold of an eight-inch,
you will be able to apply those skills at once, to work to
15th or 16th magnitude on the same kind of objects.
WHAT EQUIPMENT DOES IT TAKE?
In case I already haven't said so, APERTURE WINS, so if you
are going out to buy a telescope for deep-sky work, get the
largest one you can afford, and that you will actually use.
By that last, I mean, don't get one too cumbersome to store,
haul around and set up.
For a couple of decades, the cheapest large-aperture telescopes
have been Newtonian reflectors mounted in some variant of
the kind of altazimuth mounting pioneered by John Dobson.
There are at least four commercial manufacturers of Dobson-mounted
Newtonians with apertures as small as six inches, and even
more who make larger units. People who don't already have
a telescope often find a six- or eight-inch Dobson a good
first choice. One of those is small enough to fit in most
automobiles, and light and compact enough for almost anyone
to set up.
The four commercial manufacturers I had in mind are Celestron,
Meade, Murnaghan (who bought the old "Coulter" brand name),
and Orion. As far as I can tell, none of their Dobson telescopes
are truly first rate, but the prices are low enough that they
are all good values. I don't think it makes much difference
which brand you buy.
There are several sources of used telescopes that you may
want to consider. Many clubs run ads for used instruments
available locally, in their newsletters and bulletins. If
you have Internet access, there is a web site devoted to classified
advertising for used equipment; namely, AstroMart.
There are some others, too, and incidentally, most of the
major telescope manufacturers have web sites.
Consider making a telescope. Newtonian mirrors are not that
hard to make, and you can buy finished optics from several
sources. The mechanical parts of Dobson telescopes are very
simple. Commercial Dobson telescopes are inexpensive enough
that making one may not save a lot of money, but it is fun,
and you may well end up with a better telescope than if you
Yet I hope I have said enough so that if you already have
some other kind or size of telescope, or want some other kind,
you will know that you can do deep-sky work with it just fine.
Even a small binocular will show scores or hundreds of deep-sky
objects, and will let you develop your observing skills. Many
people already have a binocular lying around the house, or
can mooch one from family or friends for a while.
Binoculars are actually rather complicated instruments for
the astronomical performance they deliver. Large ones
say 100 mm aperture and up tend to be pretty expensive.
I think that large binoculars are poor values as astronomical
instruments, though I hasten to say that I'm not telling you
not to get one if you happen to like the views. Yet smaller
binoculars are mass-produced in enormous quantity, so the
prices drop a great deal. You can buy a reasonable 7x50 or
10x50 binocular for a good less money than the cost of a decent
beginner telescope. Furthermore, small binoculars are useful
for other things than astronomy like sports, bird-watching,
and spying on the neighbors. So small binoculars are reasonable
choices for beginning astronomers on a low budget.
No matter how you obtain a telescope, you will need an assortment
of accessories to use with it. Possibly the most important
ones are a decent set of warm clothing particularly
a good hat and a nice thermos bottle for your favorite
hot beverage. But there are some more conventional ones that
require thought, notably eyepieces, finders, and star atlases.
Many people assert that the eyepiece is just as important
as the objective when it comes to telescope performance, yet
I think that statement is seriously misleading. A bad eyepiece
will certainly ruin the view, but even so, no matter how good
the eyepiece, it cannot increase the amount of light gathered
or the amount of detail resolved by the objective. Also, decent
eyepieces are not hard to manufacture. Thus I do not recommend
making eyepieces a high-budget item, at least, not unless
you have lots of extra money, or you already have as large
a telescope as you can handle. Otherwise, if you have extra
money, get a bigger telescope, because RULE ONE: APERTURE
Eventually, you will almost certainly want enough eyepieces
to provide a nice series of magnifications, from very low
to very high. Some magnifications are more useful than others,
however. You should probably get those first.
I think everybody's eyepiece box should include a low-magnification,
wide-field eyepiece, if only because you will need one to
find objects in the first place. Such an eyepiece might give
a magnification of four to six times the telescope clear aperture
in inches. For an f/5 Dobson, that will mean a focal length
of 20 to 30 millimeters. Some of the wide-field designs in
this focal range have lenses big enough to warrant a two-inch
barrel, too -- but don't get one unless you have a telescope
with a two-inch focuser, otherwise the small focuser will
block the light, and you will be wasting all those big, expensive
When I am recommending eyepieces for general use, I generally
next suggest one that gives a magnification of about twenty-five
times the telescope aperture in inches -- that might be 4
to 6 mm for a typical Dobson. But that magnification is a
bit much for most deep-sky work, though it is entirely appropriate
for looking at globular clusters. The next eyepiece beyond
the wide-field one, that I generally use for deep-sky observation,
has a magnification of about fifteen times the aperture in
inches; in my experience, that is about right for showing
the cores of galaxies against the sky background.
Choosing additional eyepieces for deep-sky work also depends
on what you want to look at. For resolving globular clusters,
and for showing small planetaries as non-stellar, you might
want more than twenty-five per inch of aperture. It also depends
on sky brightness with light pollution, the sky background
at low magnification will be bright enough to make contrast
poor and wash out images. In such circumstances, you may not
use your low-magnification eyepiece for anything but finding
objects but you will need it badly then, for the same
sky brightness will make your finder less useful than at a
That brings me to the subject of finders. It is important
for deep-sky observers to be able to point their telescopes
in the right direction, and finders are one of the most useful
tools for doing that. I like the kind that magnifies, in contrast
to unit-magnification, "reflex-sight", types, like the TelRad.
I also like to look straight along the tube, with no prism
or diagonal to change the direction of the light beam. That
last is because it you can use a straight-through finder with
both eyes open, and let your brain project the crosshair image,
as seen through the finder, onto the sky. Thus you can use
a magnifying finder as a reflex sight, too.
Many people prefer unit-magnification finders, though
my dislike of them puts me in the minority. So if you have
any doubt what is the right kind for you, try both before
you make up your mind. But do learn how to use a straight-through
magnifying finder as a reflex sight. That is a very useful
Many people also like to use analog or digital setting circles,
or a "go to" control interface, to find objects. I have generally
found that I can find things about as fast using charts, finders,
and the main telescope optics, as with either kind of setting
circle, and often a lot more accurately. "Go to" control interfaces
are quicker, but they are also rather expensive. I'd say that
if you want to use any of these tools, go ahead, but I personally
would not call them really necessary. The money you spend
for them might better be spent on a larger telescope, because
remember rule one APERTURE WINS.
Charts, and knowing how to use them, make a lot of difference.
I use several kinds. First, when I am planning a night's observations,
I often use a simple planisphere just to remind myself of
what constellations will be visible, and at what times.
Second, I make occasional use of an atlas whose individual
charts show large areas of sky many constellations
at once as an aid to orientation, for those embarrassing
times when I am looking at a more detailed chart with no bright
stars I recognize. The one I happen to pull out when I wondering
"where is delta Sextans, anyway?", is usually an old Norton's
Star Atlas, but many others will do.
For final homing in on an object, I like to use charts that
show stars approximately as faint as I can see in my telescopes'
finders -- it is much easier to interpret between sky and
chart when exactly the same stars are visible on both. At
the moment, my favorite atlas for this purpose is the Uranometria
2000.0, with a stellar magnitude limit of about 9.5. The
new Millennium Star Atlas has a fainter limit, but
it does not have very good coverage of objects from the NGC
and IC catalogs. Those catalogs have inconsistencies and irregularities
in coverage which are perhaps reasonable cause for celestial
cartographers to shy away from them, but the NGC and IC are
likely to be with us for a long time to come, so I think the
creators of Millennium Star Atlas should have taken
more care to deal with them.
A lot of people like atlases that don't have quite as faint
a stellar magnitude limit as Uranometria. The best-known
of these is the Tirion Sky Atlas 2000. I don't like
these atlases -- there aren't enough stars for me to make
good use of my finder. They make good place mats, though,
for those times when you want to use the flat surfaces of
your Dobson as a picnic table.
Computer planetarium programs can do all the things for you
that charts can, but it is sometimes awkward to work with
computers in the field. To be fair, I should mention that
I am rather more down on computer assistance than are many
of my fellow observers, simply because I write computer programs
for a living, and far too many of them. I tend to look for
hobbies that don't have anything to do with electrons.
I should perhaps mention one other accessory: People sometimes
ask about light-pollution filters. There are several kinds,
and they do work, though they work better for nebulae than
for star clusters and galaxies. I have only encountered one
object which I could see with such a filter, that I could
not see when I removed the filter, so I do not consider them
really necessary, but if you observe in light-polluted conditions,
you might try one or two, and decide whether they are worth
it for you.
ARE GOOD OBSERVING SITES?
The kind of stuff you can see depends on where you observe.
The basic requirement for an excellent deep-sky site is that
the sky be dark and clear, with the emphasis on dark. For
most of us, that means a drive of several hours to get to
where we will set up. It takes local knowledge to find these
sites, but it is worth looking for them.
Yet decent deep-sky work can be done when the sky is brighter,
at least on those objects which have high surface brightnesses.
Globular clusters and open clusters can often be observed
well from within cities, even when the Moon is up. A little
more darkness permits looking at galaxies with bright central
regions. I don't give up too much of my telescopes' capabilities
when I observe these objects at magnifications of 15 per inch
from my yard in Palo Alto. The main problem in my yard is
finding a spot sheltered from direct illumination by street
ARE SOME GOOD PROGRAMS AND OBSERVING LISTS?
You don't have to have a program or an observing list to use
a telescope, but some people sometimes feel silly setting
up and then spending most of their time wondering what to
look at next. For these folks, a little planning may help.
For people starting out, a relatively easy, short observing
program is to observe all the Messier objects. By the time
you have done that, you will likely know what kinds of things
you particularly like to look at, and can seek out specialized
sources which list them. The Royal Astronomical Society of
Canada's Observer's Handbook has a number of lists
of deep-sky objects in its back pages, grouped both by type
of object and by degree of difficulty. Sky Catalog 2000.0
has more comprehensive lists, by type.
One list to be aware of is the one of all 2500-odd deep-sky
objects observed by William Herschel. It is available on the
world-wide web, and perhaps in other places. The interest
here, besides its size, is that it was made by visual observation,
by one observer, who for the most part used a telescope not
much more powerful than the ones we use today an 18-inch
reflector with speculum metal mirrors. All the objects on
this list are within range of amateur telescopes, and you
can get most of them with a six inch.
Burnham's Celestial Handbook is a three-volume observer's
guide to the deep sky. Some of the scientific information
in it is getting a little out of date, but it still has excellent
lists of things objects to observe, grouped by constellation,
and it includes the southern hemisphere as well as the northern.
The faintest stuff in Burnham is generally not as faint as
on the big Herschel-2500 list. Burnham includes only about
half the stuff that Herschel found.
SKILLS ARE USEFUL, AND HOW DO YOU DEVELOP THEM?
Even some experienced amateur astronomers think that seeing
things comes free and easy, with no more effort than opening
your eyes: But as current popular slang so evocatively articulates,
Vision is an acquired skill. You must learn it, you must practice,
and you must keep learning new things, and practicing them,
Buying a big telescope to see better is like buying a big
pot to cook better, or a big computer to program better. It
might help, but cooking and programming depend more on knowledge
and experience than on hardware. So does visual astronomy.
People with garages full of telescopes (I can't close the
door to mine) are victims of materialism, marketeering, and
hyperbole. Practice is cheaper, and works better. As I said
before, an experienced observer may see things with a small
telescope that a beginner will miss with one five times larger.
Canadian amateur astronomer Gary Seronik has said that telescopes
are like musical instruments. It takes time to learn to play
them well, and even an accomplished musician cannot necessarily
make beautiful music with a new or unfamiliar instrument right
away. And it certainly doesn't make sense to buy a bigger
piano or guitar with the hope of thereby making better music.
What skills may you hope to cultivate? What techniques should
you practice? Not all have names, but here are a few, in what
I think is order of importance; what matters most comes first.
Patience. It can take a long time to see everything in
a field, even if you know exactly what you are looking
(b) Persistence. Eyes, telescope, and sky vary from night
(c) Dark adaptation. Avoid bright lights before observing:
It takes your eyes hours to reach their full power of
seeing faint objects.
(d) Averted vision. The part of your retina that sees
detail best, sees low light worst. Look "off to the side"
to find lumps in the dark.
Many observers use averted vision on faint objects, but
forget it for bright ones. Detecting something doesn't
mean you've seen all of it. Don't let the dazzle of a
galaxy's lens make you miss spiral arms that go beyond
the field edge. How about increasing magnification, and
using averted vision to seek more detail in the paler,
Averted vision helps with double stars, when one star
is much fainter than the other, even if the faint star
is bright enough not to need averted vision if it were
by itself. I don't know why.
(e) Stray light avoidance. Even when it's dark, background
glow interferes with detecting faint objects. Keep it
out of your telescope and out of your eyes. Try eye patches,
and eye cups for eyepieces.
My first view of the Sculptor Dwarf Galaxy was with my
jacket collar pulled up over my binocular eyepieces. I
looked like a cross between the Headless Horseman and
the Guns of Navaronne, but I saw the galaxy.
(f) Changing magnification. Old sources about observing
faint objects sometimes suggest only such low magnifications
as 0.15 to 0.20 times the telescope aperture in millimeters.
Yet I sometimes find best detection of faint galaxies
at magnifications of 0.7 to 1.0 times telescope aperture
in millimeters. For bright objects in poor seeing, many
people back off the magnification till seeing jitter is
not visible, but doing so foregoes glimpses of fine detail
when things are momentarily steady.
If you don't change magnifications, how can you be sure
you are using the best one?
(g) Focusing critically. Particularly at higher magnification,
precise focus is important to see all the detail. In poor
seeing, it can take a long time to get the focus set right,
but it's worth doing.
(h) Moving the telescope. The eye sometimes detects motion,
or changing levels of brightness, more easily than static
images. Jiggle the telescope, or move it back and forth,
to make an object "pop out", perhaps only in the moment
just after the motion stops. Try all this while using
(i) Not moving the telescope. The eye sometimes adds up
photons over many seconds; if you can hold your eye still
for a long time, faint things may appear. Try it with
(j) Respiratory and circulatory health. If you smoke,
try taking a break before and during observing -- carbon
monoxide from incomplete combustion interferes with the
ability of the blood to transport oxygen.
(k) Hyperventilation. Don't risk fainting, but a long
series of deep breaths, or at least, a conscious effort
not to hold your breath, may better oxygenate your blood
and so improve your ability to detect faint objects.
My name is Jay Freeman. I live in Palo Alto, California, and
write computer programs for a living. I have a Ph.D. in physics,
via doctoral thesis data from an astronomy experiment that
flew on a spacecraft, so you could call me an astrophysicist.
But all my professional work was done using frequencies of
light that the human eye cannot see I have retained
amateur standing in the visual wavelengths.
I have been doing visual amateur astronomy for over forty
years. I started when I was eight, with a 50 mm spotting telescope
so junky it made modern beginner refractors look good, and
that's hard to do. Last time I added up my logbook, I found
I had made not quite ten thousand observations of more than
four thousand different objects. Most of them were deep-sky
objects. I have used about twenty different telescopes and
binoculars enough to know them well; these have had apertures
from 50 mm through fourteen inches.
This article is the text of a talk originally given by Jay
at a meeting of the Tri-Valley Stargazers Astronomy Club in
Livermore, California on July 10, 1998. It appeared shortly
thereafter on USENET in the sci.astro.amateur
newsgroup where Jay is a regular participant.
More articles written by Jay, and other writers, may be found
The Astronomy Connection.