Astronomy - 06.2019

(John Hannent) #1
16 ASTRONOMY • JUNE 2019

O


ver the years, I’ve
always been an
advocate for the
small-aperture
telescope, tout-
ing its remarkable capabilities
in my writings and through
talks at astronomy conven-
tions and club meetings.
During my salad days as an
amateur astronomer, back in
the 1970s, my telescopic arse-
nal was made up of a 3-inch
f/10 ref lector and a 2.4-inch
f/11 refractor. Modest in size
though they were, these high
focal ratio instruments were
remarkably capable — espe-
cially on double stars, my
favorite night-sky targets.
In the early 1980s, I took
a giant leap and purchased a
13.1-inch Dobsonian-mounted
reflector. This “fast” (f/4.5)
light-gobbling beast revealed
deep-sky wonders well beyond
the grasp of my little scopes.
But it didn’t do well with dou-
ble stars. The bright binary
star Castor, whose component
stars were separated by 2" at
the time, was resolvable in
the 3-inch, but not so in the
13.1-inch. Instead of two sepa-
rate stellar images, my eye was
greeted by an elongated, scin-
tillating blob of light.
Fortunately, the big scope
came with directions to make
an off-axis mask that would
convert it into an unob-
structed 5-inch f/12 long-focus
scope that promised to yield
sharper stellar images. When I
placed a cardboard prototype
over the front of the tube and

pointed the scope at Castor,
the fuzzy blob was indeed
transformed into two
beautifully separated stars.
Encouraged by my success, I
fashioned a more permanent
model out of ⅛-inch plywood.
A few years ago, I sold the
13.1-inch Dobsonian (reluc-
tantly!) for an easier-to-handle
10-inch f/5 instrument.
Although there were no direc-
tions for making an off-axis
mask, I used my previous
experience to cobble together a
crude prototype in less than an
hour. To do the same, all you
need is a sheet of corrugated
cardboard greater in diameter
than the telescope tube, a pen-
cil, a hobby knife, a tape mea-
sure, and a roll of duct tape.

Here’s the process:


  1. To make sure the mask is
    the correct size, hold the card-
    board against the top of the
    tube and trace out a circle that
    matches the telescope’s out-
    side diameter.

  2. Use the tape measure
    to determine the diameter of
    the largest circle that will fit
    between the secondary mirror
    and support vanes. I found
    that to be a 4-inch diameter
    hole for my 10-inch scope.

  3. Use a compass (or an
    appropriately sized can) to
    trace out the opening for the
    mask. To compensate for the


OBSERVINGBASICS
BY GLENN CHAPLE

Make a mask


for double stars


Some stellar pairs are too bright to separate with a large
scope. An off-axis mask can help you easily split them.

thickness of the telescope tube,
place the opening a half-inch
from the edge of the mask.


  1. With the hobby knife,
    cut out the aperture mask and
    the opening.

  2. Attach the mask to the
    telescope with a few strips of
    duct tape, and you’re ready to
    head outside and use it.
    On an evening of fair seeing
    conditions, I tested the mask
    on the striking near-twin dou-
    ble star Epsilon (ε) Arietis,
    whose diamondlike magnitude
    5.2 and 5.6 component stars
    were 1.3" apart. To my scope’s
    credit, the pair was reasonably


split at 212x without the mask.
But with the mask taped in
place, I noticed a slight
improvement. Although the
seeing conditions didn’t war-
rant it, I decided to go for
broke with a 3.2mm eyepiece
that yielded a magnification
of 397x. This time, the view
using the mask was a definite
improvement over what I saw
without it.
There are limitations to a
“new” masked scope, however.
For me, the theoretical resolu-
tion limit was reduced from
0.5" for my 10-inch scope to
a little over 1" for its 4-inch

alter ego. Still, it allowed me
to shift my attention from
faint fuzzies to close double
stars without having to put
the 10-inch away and bring
out my 3.5-inch f/11 refractor.
I made my off-axis mask
last January when Epsilon
Arietis was conveniently
located in the evening sky. If
you make one now, you might
want to test it on Mu (μ)
Draconis (mags 5.7 and 5.7,
sep. 2.3"), Xi (ξ) Ursae Majoris
(4.3 and 4.8, 1.9"), or the clos-
est components to the neat
triple star Xi (ξ) Scorpii (4.
and 5.2, 1.1"), whose third
member (mag 7.3) is 7.6" away.
Once you’ve made a work-
able prototype, you can move
on to a more durable model. As
mentioned, I made mine out of
⅛-inch plywood, then spray-
painted it f lat black on the
inside, and secured it to the
main scope with small metal
L-brackets. I’ll leave it to you to
come up with a final design of
your own once you’ve created a
workable prototype.
Questions, comments, or
suggestions? Email me at
[email protected]. Next
month: We honor an event
that happened 50 years ago.
Clear skies!

BROWSE THE “OBSERVING BASICS” ARCHIVE AT http://www.Astronomy.com/Chaple.

Limiting the brightness
of double stars with an off-
axis mask can significantly
help you separate otherwise
indistinguishable stars. The two
large, bright stars of Castor (which
is really six stars that appear as one)
are seen in this sketch. JEREMY PEREZ

Glenn Chaple has been an
avid observer since a friend
showed him Saturn through a
small backyard scope in 1963.

A mask allowed me to shift my attention
from faint fuzzies to close double stars.
Free download pdf