The Cosmic Explorer
(600-2409)                 Projects                   Faxback Doc. # 33045

SUGGESTIONS FOR SCIENCE FAIR PROJECTS:

We don't know if you are a student or adult, but everyone can benefit from
the extraordinary pursuit of knowledge for its own sake.  Here are a few
topics of investigation for the backyard Star Gazer or student in search
of a great Science Fair Project.  The descriptions are skeletal, but you
can flesh out the details by contacting the Amateur Astronomers in your
area by writing to the Astronomical League (address on page 10.

1.  Collecting and Identifying Micrometeoritic Ablation Spheroids:

    Each day the Earth gets peppered by about 1,000,000,000 meteors.  Most
    are sand grain size and burn up in the atmosphere.  You may see some
    as "shooting stars".  Tiny bits melt off due to friction as the
    meteors rush through the air.  These particles are called Ablation
    Spheroids.  They gradually settle to Earth and are found everywhere.
    Many are magnetic.  You can devise a collecting unit using a magnet or
    a white catch basin to trap these particles.  Examination should be
    done at >50X magnifying power.  You will be amazed by all of the
    particulate contaminants found on your specimen slide-including auto
    catalytic converter emission particles, tiny sand grains and dust;
    pollen; factory emissions, and the Ablation Spheroids.  Good sketching
    technique, microphotography and statistical analysis will strengthen
    your research.

2.  Determination of Star Temperatures by Star Trail Photography:  Stars
    appear white to most people who casually glance at the sky.  If you
    spend as little as 1/2 hour looking at the stars on a dark night, you
    will soon notice a great, but subtle, variety of colors.  These range
    from ruby reds to blue whites, with orange and yellow stars in
    between.  Color slide film with ISO speeds of 400-1200 are much more
    sensitive than your eye to dim star colors.  Use a 35mm single lens
    reflex camera with time lapse capability, mounted on a tripod to do
    this project.  Focus the camera sharply on a bright star and open the
    lens to the fastest f/number, be it 1.2, 1.4, 2.0, or whatever.  A 50mm
    lens works best-giving you a field of view of 20 degrees x 30 degrees.
    Not only will the film capture color more easily. You will be astounded
    at how many stars show up on the film.  Start by using a 12 or 24
    exposure roll of film to get your technique right.

    A.  With your equipment set up, point the camera toward the zenith on
        a clear dark night and start your exposure by pressing the plunger
        on the cable release.

    B.  Lock the shutter in the open position.  Don't shake the camera.

    C.  After 25 seconds of exposure, carefully block the starlight from
        entering the lens for 2 minutes.  Don't stop the exposure!

    D.  After 2 minutes, the Earth's rotation will provide a 1/2 degree
        space between the star images recorded in the first 25 second
        exposure and the final exposure which comes next.

    E.  Carefully remove the obstruction you placed in front of the camera
        lens without moving the camera in the least!  Expose the film for
        8 minutes then stop the exposure.  You can repeat this for
        different parts of the sky.

    F.  Use your Cosmic Explorer to identify the star fields and
        constellations photographed before you make the exposure.  Some
        people get so excited, they neglect good record keeping, thinking
        that memory will serve them later, but trust it doesn't work well.
        Take good notes.

    G.  Your developed prints (glossy, not matte) can be examined by eye
        or magnified.  Identify the brightest stars using the Cosmic
        Explorer.  There are star charts and other information available
        to check on the names and other data for dimmer stars.  Use the
        chart of 20 brightest stars for some of your first attempts.

    H.  Compare the color of the 2 degree star trail on the film to the
        spectral type listed in the Star Data Tables.  The K stars should
        be yellow-orange, the M stars red; the G stars, yellow, etc.  Your
        intent is to estimate star temperatures by using color as the
        indicator.  Again, a clear project design will be very helpful.
        This project makes an exciting display.

    I.  Your images will look like this:

        a. 25 second exposure

        b. 2 min space 

        c. color star trail 2 degree long

3.  Spectral Photography of Stars:

    This is a project which uses all the items needed in the above
    exploration plus a medium dispersion transmission diffraction grating
    available from many science education supply houses, like Edmund
    Scientific in Barrington N.J.  These plastic gratings are mounted in
    2X2 slide holders and are quite inexpensive.

    A.  You will have to figure a way to mount the diffraction grating in
        front of the camera so that the spectrum or color of dispersed
        star light falls on the film along with the star.  This is very
        easy to do with a single lens reflex camera and it gives you an
        opportunity to be technically creative.

    B.  Once you are satisfied that the diffraction grating is properly
        positioned, take your unit outdoors on a dark clear night.  Use
        the stars listed in the 20 Brightest List as targets.  Select a
        range of spectral types.

    C.  Point the camera at the star and position it so that the star is
        visible in edge of the field of view and the spectrum, which
        should be visible in the middle of the field of view.

    D.  You want to set the optical system up so that as the Earth
        rotates, the spectrum moves as a band across the film.  It should
        look like this:

        a. Star Trail

        b. Color spectrum band with dark vertical lines.

        A little practice is needed but soon your spectral photos will be
        works of scientific art.

    E.  Use reference information on stellar spectra to help identify the
        nature of the dark absorption lines that should be visible in the
        A-type and M-type stars.

    F.  This is a much more powerful technique than simple color
        photography for identifying star spectra and temperature.  You can
        also experiment with planetary and lunar spectra-all of which are
        reflected solar spectra of a G2V start another challenge is Nebular
        and Cluster photography using your spectral set-up.  This system
        works well at the eyepiece end of a motor driven telescope.  The
        light gathering power of the telescope makes dimmer objects
        manageable.

        Your local amateur astronomy group; planetarium director;
        university astronomy department; and public libraries are all
        great sources of help, information and inspiration.  With a little
        perseverance, the rewards can be astronomical!

GOING FURTHER ON YOUR OWN:

We suggest that you contact the following for resources, information, and
inspiration in your pursuit of knowledge.

1.  The Astronomical Workshop, Furman University, Greenville, SC, 29613,
    USA:  An excellent selection of annual sky calendar, plus books and
    activities for adults and students.

2.  Sky Publishing Corporation, PO Box 9111, Belmont, MA, 02178-9917.
    Complete resource for publications, star atlas, charts, and observing
    aids.

3.  Observer's Handbook by The Royal Astronomical Society of Canada, a
    comprehensive astronomy handbook published annually.  Available from
    Sky Publishing Corp.

4.  The Astronomical League, Science Service Building, 1719 N. Street,
    N.W. Washington, DC, 20030 Attn.: Executive Secretary.  The League has
    chapters of active amateur and professional members across the USA.
    Send a self addressed stamped envelope to the League with a specific
    request for selected free material and chapter locations.


(BR/EB 5/10/96)

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