This is Core Activity 6.2 in the HOA curriculum and is
titled Estimating Magnitudes Using Interpolation. It is
a good introductory activity, teaching students how to
estimate just the magnitudes, or apparent brightness,
of stars.
To estimate magnitudes of variable stars, you will need
to interpolate. Interpolation is the process of
estimating a value between two known values. Near the
variable star you will be observing are two or more
comparison stars of known magnitude. These stars do not
change in brightness and are used to compare the
brightness of the variable star. Knowing the values of
the magnitudes of the comparison stars and the
magnitude range of the variable star itself, you can
interpolate or estimate the magnitude of the variable
star as it changes over time.
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Given below are three star fields. The magnitudes
of the comparison stars are given. Estimate to the
nearest tenth the magnitude of the variable star (offset by
the lines in each field [- -]). Note: In star
fields, the decimals are not indicated. A
magnitude of 6.4 is written as 64, so that the
fields are not cluttered and the decimal points
are not mistaken for stars.
In field A, the magnitude of the variable star
seems to lie between 6.1 and 6.4, almost half way,
maybe a little closer to 6.1, so the magnitude
estimate is 6.2. Your estimate may be different
from this and that is okay. Make a table like the
one below, and record your estimate.
Make estimates of the other two star fields. Also,
record the estimates made by two of your
classmates. Do your estimates differ from theirs?
-
Compare your estimated magnitudes with those of
the rest of the class. Does everyone have the same
answers?
| Magnitude (Your own) | Magnitude (classmate 1) | Magnitude (classmate 2) |
(A) | | | |
(B) | | | |
(C) | | | |
The lesson then moves into Core Activity 6.3 titled How
accurate are your results?. In this lesson students
learn how to calculate absolute error/percentage of
error, the concept of significant digits, and
systematic vs. random error.
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