Personal equation
From Wikipedia, the free encyclopedia
The personal equation, in 19th- and early 20th-century science, referred to the idea that every individual observer had an inherent bias when it came to measurements and observations.
The term originated in astronomy, when it was discovered that numerous observers making the simulataneous observations would record slightly different values (for example, in recording the exact time at which a star crossed a wire in a telescope view-finder), some of which were of a significant enough difference to afford for problems in larger calculations.
In response to this realization, astronomers became increasingly suspicious of the results of other astronomers and their own assistants, and began systematic programs to attempt to find ways to remove or lessen the effects. These included attempts at the automation of observations (appealing to the presumed objectivity of machines), training observers to try and avoid certain known errors (such as those caused by lack of sleep), developing machines which could allow multiple observers to make observations at the same time, the taking of redundant data and using techniques such as the method of least squares to derive possible values from them, and trying to quantify the personal equations of individual workers so that they could be subtracted from the data. It became a major topic in experimental psychology as well, and was a major motivation for developing methods to deal with error in astronomy.
[edit] References
- Simon Schaffer, "Astronomers Mark Time: Discipline and the Personal Equation," Science in Context, 2 (1988), 101-131.
