Nearest Stars: A Guided Tour
Observing the Sun — Safely
by John R. Percy,
University of Toronto
(c) 1986 Astronomical
Society of the Pacific
[Editor's note: Since other stars are so far away, much of the progress we are
making in understanding stars in general comes from studying our own "hometown''
star, the Sun. Although most of us associate the study of astronomy with the
night, in this month's activity our newsletter's newest contributing editor
shows that the Sun can lend itself to useful daytime astronomy activities. (Dr.
Percy is professor of astronomy at the University of Toronto in Canada and one
of the world's leaders in the field of astronomy education.)]
We must begin
with an important warning: Never look directly at the Sun, especially when using
binoculars or a telescope. Direct sunlight can cause permanent eye damage
in seconds, without the victim being aware of it until it is too late.
For safe direct
viewing of the Sun, #14 welder's glass can be used, or a proprietary material
known as Solar Skreen (Roger W. Tuthill, Inc., 11 Tanglewood Lane, Mountainside,
NJ 07092). Although some telescopes are equipped with Sun filters, many of these
are not reliable, and should not be used unless you are absolutely
sure of what you are doing. The only reliable filters are some (but not all)
which fit over the front of the telescope, and reflect away most of the light.
The best way to
view the Sun with binoculars or a telescope is by projection —
looking at an image of the Sun rather than at the Sun itself. Instructions for
doing this are given below.
We should note
that some school officials feel that all viewing of the Sun should be forbidden.
Even though there are safe ways to view the Sun, there is always a chance that
some student will not take the necessary precautions, or will disobey instructions,
and an accident will occur. The projection methods described below are quite
safe, however — and the number of astronomy-related school accidents is
far less than the number encountered in other science subjects!
Sun by Projection
This method is relatively
safe and, with it, many people can view the Sun at once. You will need a pair
of binoculars or a small telescope, a piece of plain cardboard about 30 centimeters
square for the "collar,'' and a second piece of white cardboard (or paper)
at least 10 centimeters square for the screen. If you use a telescope, you should
mount it on a tripod. If you use binoculars, you can hold them in your hand, but
it is much more convenient (and you will have a steadier image) if you improvise
some sort of stand or tripod to hold them.
can be done at any time of the day when it is clear and when your class has
access to direct sunlight.
Note: Do not use
binoculars whose front lenses are 50 millimeters across or wider. (Binoculars
usually are described by a pair of numbers separated by an 'x', such as "7
x 3'' or "7 x 50''; the number to the right of the 'x' is the diameter
of the front lenses in millimeters.) Big lenses gather a lot of light, and the
heat generated by direct sunlight in side large binoculars can damage their
- Make a cardboard
collar to fit around the front end of the binocular or telescope, as shown
in the figure. This shades the area where the image will be from sunlight.
and (in the case of binoculars) will cover the lens which you are not using.
- Focus the binocular
or telescope on infinity by looking at a distant object (not the Sun!) in
the normal way. (If you are using a telescope. use a low-magnification eyepiece.)
- Point the binoculars
or telescope at the Sun (do not look through the instrument to do
this!), as shown in the figure, and adjust the direction of pointing until
the image of the Sun appears on the screen. (This may take a minute or two.
One useful trick is to watch the shadow of the binoculars or telescope tube:
if pointed directly toward the Sun, then the sides of the tube will cast no
shadows, and the instrument's shadow will be as small as it can be.)
- Move the screen
toward or away from the eyepiece until the image of the Sun fits neatly in
the middle. and adjust its tilt until the Sun's image is circular.
- Jiggle the binoculars
or telescope very slightly. Any specks on the image of the Sun which do not
jiggle along with the image when you do this are specks in the binoculars
or telescope (or smudges on the screen), and not spots on the Sun itself.
When you and your
students examine an image of the Sun, you will notice the following properties:
- The image is
brighter in the middle of the disc than at the edges. This effect is called
limb-darkening. It occurs because, when we look at the middle of the
Sun's disc, we are looking straight down into the hotter part of the Sun.
At the edges of the disc, we look more obliquely, and see only the cooler,
less bright gases, higher in the Sun's atmosphere.
- The image moves
slowly across the screen. This is due to the east-to-west motion of the Sun
in the sky, caused by the rotation of the Earth. The direction of motion of
the image therefore tells you which direction on the screen (and on the Sun's
image) is west.
- There may be
small darks spots on the image. These are called sunspots and are regions
in the outer layers of the Sun which are cooler and therefore not as bright
as their surroundings. In sunspots, the Sun's magnetic field is exceptionally
strong, and astronomers suspect that this is connected to their being darker
than the material around them. Sunspots, when examined closely with a telescope,
are seen to be very complex. They can form within a few days, and may endure
and evolve for weeks or months.
An Alternate Way
to Project An Image of the Sun
This method produces
an image which is a bit fuzzy, but good enough to show large sunspots, and it
is particularly suitable for observing a partial eclipse of the Sun. It is very
safe, and can be used to show an image of the Sun to an entire class. You will
need a small pocket mirror or hand mirror. a piece of plain cardboard to fit over
the mirror (or some tape to cover it), and a piece of white cardboard or paper
to use as a screen.
- Cut the plain
cardboard or paper so it fits over the mirror.
- Cut or punch
a very small hole, about 5 millimeters in size. in the middle of the plain
cardboard. You could also use tape to cover all but a small portion of the
surface of the mirror.
- Put the mirror
on a window sill in the sunlight such that it catches the rays from the Sun.
Turn the room lights off and draw the window blinds so that as little as possible
of the room other than the mirror is in sunlight.
- Reflect the
sunlight onto a wall of the darkened room.
- Put the white
cardboard or paper on the wall at this point, so you can use it as a screen
to display the image of the Sun.
If you do not have
a classroom in which there is a sunlit window, you can do the activity outdoors.
Find a place where you can catch the sunlight with your mirror, and can reflect
it onto a shaded wall. (Better still, reflect it into a darkened classroom.) Again,
you can use a sheet of white paper or cardboard as a screen. It takes a few minutes
to discover the best arrangement for the mirror and the screen, but once you have
done so, it is easy to set up the demonstration again on any following day.
- You will notice
that the image of the Sun is round (unless an eclipse is in progress), even
if the hole which you cut or punched in the plain cardboard or paper was square!
- You can also
demonstrate that the size of the image of the Sun is proportional to the distance
of the screen from the mirror. The larger the distance. the larger (and fainter)
the image. In a more advanced class, you might want to develop an explanation
for these two observations.
Reading About The Sun
Robert Burnham: "Observing
the Sun,'' Astronomy, August 1984, p. 51.
B. Ralph Chou:
"Safe Solar Filters,'' Sky & Telescope, August 1981, p. 119.
"Close-Up of a Star'', Sky & Telescope, May 1985, p.3 97.
Daytime Star (1981, Scribner's)
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