Big Dipper I
Project for Elementary Astronomy
For this project you will observe and sketch the Big Dipper (part of the
constellation Ursa Major) and the North Star (Polaris) several times during
the course of one long night.
Follow this procedure:
- Pick a starting time after it is completely dark,
when the Big Dipper is clearly visible. (If it's very low in the sky, you may be able to
see only part of it.) Try a pay attention to the
weather, and do the project on a night with no clouds in the
forecast.
- Your observing location should have a
good clear view of the northern horizon, without any tall
obstacles in the way (trees, buildings, etc.). You will make all
your observations from the same location.
- Download and print the file PolarPlot.pdf, and use
this to record your sketches. The North Star should be plotted in the middle
of the circles. The interval between one circle and the next is 10° (one fist).
- Each time you observe the Big Dipper,
carefully plot the position of the seven stars that make up
the dipper. Use your hands/fists to measure angles in the sky.
Be very careful to plot each star correctly in relation to the others and
in relation to the North Star. Also record the
date and time of your observations.
- Repeat the observation/sketch procedure
every 2 hours all night long, until just before sunrise. You may either make all sketches
on the same plot (perhaps in different colors), or use a different plot for each. If unexpected clouds
keep you from finishing your observations, try again on the next clear night.
- Note that over the course of your
observations, the stars should not change their distance away from
one another or away from the North Star. Rather, they should seem
to rotate around together in a circle.
For your report, complete the following analysis of
your data:
- Using your sketches, measure the total
number of degrees that the Big Dipper has rotated around the North Star.
- Divide the total number of
degrees by
the total time in hours between your first and last observations. This is the average
number of degrees of motion per hour. If you've been careful, it
should be close to 15° per hour.
- Multiply your result by 24 hours to
predict the angle that the Big Dipper rotates through in one day.
- It is highly unlikely that a single
nightÕs measurements will be accurate enough to get exactly the
correct answer. The correct answer is actually 361°, not
360°. Discuss why the correct answer is 361°. (Hint: think about all of Earth's
motions.)
- Discuss your results and why you think
they might be off from the expected results.
- Be sure to follow the general instructions applicable
to all projects.
Alternate photographic method:
- If you have a suitable camera with a tripod and know how to use it, you can take
photographs of the stars instead of making sketches. The camera must be capable of making
time exposures of at least several seconds. Almost any digital SLR camera can do this, as
can some digital point-and-shoot cameras (including most Canon models). A film camera
with a locking shutter or cable release will also work. Before attempting to do this
project with a camera, please bring the
camera to your instructor to determine whether it is suitable, and to discuss what settings
to use.
- A wide angle lens (or a zoom lens at its widest setting) is best. Even so, you may
not be able to fit all of the Big Dipper into the field of view. That's ok as long as enough
other stars are visible. Aim the camera so the North Star is at the center of the field of view,
with at least one terrestrial object (perhaps a tree or rooftop) also visible. Once the camera is set
up and aimed correctly, don't move it again for the rest of the night. Take a photo every two
hours. (In between photos, you may need to cover the camera
loosely with a sack to prevent dew or frost from forming.)
- Before printing your
photos, it's best to invert them (switching black and white) in Photoshop or a similar program.
Your instructor can help with this.