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Types of Errors Common sources of error in astronomy laboratory ...

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<strong>Types</strong> <strong>of</strong> <strong>Errors</strong><br />

Measurement <strong>error</strong>s may be classified as either random or systematic, depend<strong>in</strong>g on<br />

how the measurement was obta<strong>in</strong>ed (an <strong>in</strong>strument could cause a random <strong>error</strong> <strong>in</strong> one<br />

situation and a systematic <strong>error</strong> <strong>in</strong> another).<br />

Random <strong>error</strong>s are statistical fluctuations (<strong>in</strong> either direction) <strong>in</strong> the measured data due<br />

to the precision limitations <strong>of</strong> the measurement device. Random <strong>error</strong>s can be evaluated<br />

through statistical analysis and can be reduced by averag<strong>in</strong>g over a large number <strong>of</strong><br />

observations (see standard <strong>error</strong>).<br />

Systematic <strong>error</strong>s are reproducible <strong>in</strong>accuracies that are consistently <strong>in</strong> the same<br />

direction. These <strong>error</strong>s are difficult to detect and cannot be analyzed statistically. If a<br />

systematic <strong>error</strong> is identified when calibrat<strong>in</strong>g aga<strong>in</strong>st a standard, apply<strong>in</strong>g a correction or<br />

correction factor to compensate for the effect can reduce the bias. Unlike random <strong>error</strong>s,<br />

systematic <strong>error</strong>s cannot be detected or reduced by <strong>in</strong>creas<strong>in</strong>g the number <strong>of</strong> observations.<br />

Our strategy is to reduce as many <strong>sources</strong> <strong>of</strong> <strong>error</strong> as we can, and then to keep track <strong>of</strong><br />

those <strong>error</strong>s that we can’t elim<strong>in</strong>ate. It is useful to study the types <strong>of</strong> <strong>error</strong>s that may<br />

occur, so that we may recognize them when they arise.<br />

<strong>Common</strong> <strong>sources</strong> <strong>of</strong> <strong>error</strong> <strong>in</strong> <strong>astronomy</strong> <strong>laboratory</strong> experiments:<br />

Use the follow<strong>in</strong>g as a guide to th<strong>in</strong>k<strong>in</strong>g about <strong>sources</strong> <strong>of</strong> <strong>error</strong>. Just list<strong>in</strong>g the below<br />

terms will not receive any credit. You must expla<strong>in</strong> the source <strong>of</strong> <strong>error</strong> and how it<br />

affected your measurements.<br />

Incomplete def<strong>in</strong>ition (may be systematic or random) - One reason that it is impossible<br />

to make exact measurements is that the measurement is not always clearly def<strong>in</strong>ed. For<br />

example, if two different people measure the length <strong>of</strong> the same rope, they would<br />

probably get different results because each person may stretch the rope with a different<br />

tension. The best way to m<strong>in</strong>imize def<strong>in</strong>ition <strong>error</strong>s is to carefully consider and specify<br />

the conditions that could affect the measurement.<br />

Failure to account for a factor (usually systematic) – The most challeng<strong>in</strong>g part <strong>of</strong><br />

design<strong>in</strong>g an experiment is try<strong>in</strong>g to control or account for all possible factors except the<br />

one <strong>in</strong>dependent variable that is be<strong>in</strong>g analyzed. For <strong>in</strong>stance, you may <strong>in</strong>advertently<br />

ignore air resistance when measur<strong>in</strong>g free-fall acceleration, or you may fail to account for<br />

the effect <strong>of</strong> the Earth’s magnetic field when measur<strong>in</strong>g the field <strong>of</strong> a small magnet. The<br />

best way to account for these <strong>sources</strong> <strong>of</strong> <strong>error</strong> is to bra<strong>in</strong>storm with your peers about all<br />

the factors that could possibly affect your result. This bra<strong>in</strong>storm should be done before<br />

beg<strong>in</strong>n<strong>in</strong>g the experiment so that arrangements can be made to account for the<br />

confound<strong>in</strong>g factors before tak<strong>in</strong>g data. Sometimes a correction can be applied to a result<br />

after tak<strong>in</strong>g data to account for an <strong>error</strong> that was not detected.


Instrument resolution (random) - All <strong>in</strong>struments have f<strong>in</strong>ite precision that limits the<br />

ability to resolve small measurement differences. For <strong>in</strong>stance, a meter stick cannot<br />

dist<strong>in</strong>guish distances to a precision much better than about half <strong>of</strong> its smallest scale<br />

division (0.5 mm <strong>in</strong> this case).<br />

Physical variations (random) - It is always wise to obta<strong>in</strong> multiple measurements over<br />

the entire range be<strong>in</strong>g <strong>in</strong>vestigated. Do<strong>in</strong>g so <strong>of</strong>ten reveals variations that might otherwise<br />

go undetected. These variations may call for closer exam<strong>in</strong>ation, or they may be<br />

comb<strong>in</strong>ed to f<strong>in</strong>d an average value.<br />

Parallax (systematic or random) - This <strong>error</strong> can occur whenever there is some distance<br />

between the measur<strong>in</strong>g scale and the <strong>in</strong>dicator used to obta<strong>in</strong> a measurement. If the<br />

observer’s eye is not squarely aligned with the po<strong>in</strong>ter and scale, the read<strong>in</strong>g may be too<br />

high or low (some analog meters have mirrors to help with this alignment).<br />

Personal <strong>error</strong>s come from carelessness, poor technique, or bias on the part <strong>of</strong> the<br />

experimenter. The experimenter may measure <strong>in</strong>correctly, or may use poor technique <strong>in</strong><br />

tak<strong>in</strong>g a measurement, or may <strong>in</strong>troduce a bias <strong>in</strong>to measurements by expect<strong>in</strong>g (and<br />

<strong>in</strong>advertently forc<strong>in</strong>g) the results to agree with the expected outcome. Personal <strong>error</strong>s,<br />

sometimes called mistakes or blunders, should be avoided and corrected if discovered.<br />

The term human <strong>error</strong> should never be used when describ<strong>in</strong>g <strong>sources</strong> <strong>of</strong> <strong>error</strong>. If it<br />

was a human <strong>error</strong>, don’t be lazy, fix it!

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