Dioptra
A dioptra is a classical astronomical and surveying instrument, dating from the 3rd century BC. The dioptra was a sighting tube or, alternatively, a rod with a sight at both ends, attached to a stand. If fitted with protractors, it could be used to measure angles.
Use
used the dioptra to measure the positions of stars; both Euclid and Geminus refer to the dioptra in their astronomical works.It continued in use as an effective surveying tool. Adapted to surveying, the dioptra is similar to the theodolite, or surveyor's transit, which dates to the sixteenth century. It is a more accurate version of the groma.
There is some speculation that it may have been used to build the Eupalinian aqueduct. Called "one of the greatest engineering achievements of ancient times," it is a tunnel long, excavated through a mountain on the Greek island of Samos during the reign of Polycrates in the sixth century BC. Scholars disagree, however, whether the dioptra was available that early.
An entire book about the construction and surveying usage of the dioptra is credited to Hero of Alexandria. Hero was "one of history’s most ingenious engineers and applied mathematicians."
The dioptra was used extensively on aqueduct building projects. Screw turns on several different parts of the instrument made it easy to calibrate for very precise measurements.
The dioptra was replaced as a surveying instrument by the theodolite.
How it works
The dioptra consists of a sighting tube or rod fitted with sights at both ends and mounted on a stable stand. The stand usually includes adjustable screw turns that allow the instrument to be precisely calibrated. When used for astronomical purposes, the user would align the sights with a specific star or celestial object, and then measure the angle using protractors attached to the instrument. In surveying, the dioptra was used to measure angles and distances by sighting along the rod and taking readings from graduated scales.Advantages and disadvantages
The dioptra offered several advantages over other contemporary instruments. Its ability to measure both vertical and horizontal angles with high precision made it a versatile tool for both astronomy and surveying. The screw turns allowed for fine adjustments, improving accuracy. The instrument's simplicity and robustness made it reliable and easy to use in the field.However, the dioptra also had its limitations. The accuracy of measurements depended on the user's skill and the quality of the instrument's construction. The sighting tube or rod could be affected by environmental factors such as wind or temperature changes, which could introduce errors. Additionally, the dioptra required careful calibration before each use, which could be time-consuming.
Compared to later instruments like the theodolite, the dioptra was less advanced and lacked some of the refinements and improvements that made theodolites more accurate and easier to use. The theodolite eventually replaced the dioptra as the primary instrument for surveying due to its superior performance and reliability.