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Triquetrum

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The Triquetrum, also known historically as the long alidade or parallactic ruler, is a three-arm astronomical instrument used to determine the altitude and zenith distance of celestial objects. By aligning its moving arm with a target and recording the slider position, users can calculate the object’s position in the sky.

Explore Astronomy Through Geometry

The Triquetrum is a remarkable historical astronomical instrument that demonstrates how geometry and observation were used to study the sky.

Unlike the Quadrant, which uses a graduated curved scale, the Triquetrum uses a system of connected arms and geometric calculations to determine the position of celestial objects.

The instrument forms a triangular structure, allowing users to measure the zenith distance of an observed object and then calculate its altitude.

The triquetrum was historically used as an alternative method for measuring celestial positions and was associated with the development of observational astronomy.

How It Works

The Triquetrum consists of a stable supporting structure with connected arms and a movable slider.

To take a measurement:

  1. Look from the bottom hinge along the ruler arm.
  2. Move the slider until the celestial target aligns completely with the sight.
  3. Lock the slider firmly in position.
  4. Record the position of the slider on the ruler as R, measured in centimeters.
  5. Use the geometric relationship of the instrument to calculate the zenith distance.

For the setup described in the manual, the instrument forms an isosceles triangle and uses the following equation:

Z = arccos(R / 2L)

Where:

  • Z = Zenith Distance
  • R = Reading from the ruler arm
  • L = Constant length of the supporting and moving arms

In the manual’s version of the setup, both arms have a length of 93 cm.

After calculating the zenith distance, the final altitude is found by subtracting it from 90°.

θT = 90° − Z

Key Features

  • Historical astronomical measuring instrument
  • Three-part triangular structure
  • Adjustable ruler and slider system
  • Geometric measurement method
  • Designed for celestial observation
  • Measures zenith distance
  • Calculates astronomical altitude
  • Demonstrates the relationship between mathematics and astronomy
  • Suitable for practical educational experiments

A Different Approach to Measuring the Sky

The Triquetrum provides a unique hands-on experience because it combines physical observation with mathematical calculation.

Users do not simply read an angle directly. Instead, they:

Observe → Align → Measure → Calculate → Determine Altitude

This makes the Triquetrum an excellent educational tool for demonstrating practical geometry, trigonometry, historical astronomy, and experimental measurement.

The historical design also reflects an important advantage of straight measuring scales: the triquetrum can determine angular relationships through its geometry rather than relying entirely on a graduated circular arc.

Perfect For

  • Astronomy laboratories
  • Physics education
  • Mathematics demonstrations
  • Trigonometry experiments
  • STEM education
  • Universities and schools
  • Historical astronomy projects
  • Science exhibitions
  • Museum demonstrations

Experimental Learning

Users can observe the Sun or Moon at regular intervals and record measurements using the Triquetrum. These results can then be compared with modern astronomical software to investigate measurement accuracy.

Research and Education

The triquetrum was used to measure the altitude of the Sun and Moon at different times. The readings were taken at LUMS, Lahore and compared with Stellarium values. The results for the Sun and Moon are given separately below.
 

Observation and Results of the Sun

To test the Triquetrum, the Sun was observed on February 13, 2026, from 8:40 AM to 4:20 PM at LUMS, Lahore. A total of 24 readings were taken every 20 minutes and compared with Stellarium data. The highest recorded altitude was around 47.8° at 1:20 PM, with earlier peaks of 47.5° at 12:00 PM and 12:20 PM (compared to Stellarium’s peak of 45.1° at 12:20 PM). The readings then decreased during the afternoon.

Safety: Never view the Sun directly without a certified solar filter, as it causes severe eye damage.

The comparison between the Triquetrum readings and Stellarium values is shown in the graph below.

 

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 

 

 

 

Observation and Results of the Moon

To test the Triquetrum, the Moon was observed from 20th March to 17th April 2026 (129 Shawal 1447 AH) at LUMS, Lahore. Readings were taken on select dates during this period and compared with Stellarium data. The highest altitude recorded was around 64° between 29th and 30th March, after which the altitude steadily decreased into early April. Overall, the Triquetrum readings aligned closely with the expected values from Stellarium.

The Moon’s altitude plot and the comparison between the Triquetrum readings and Stellarium values are shown in the graph below.

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 

 

 
 
 

Manual and Documents

User Manual

Urdu Manual

Additional Resources: Altitude: A Historical Perspective — Astrolab

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