Stellar Motions and Distances
Goal: To Measure Parallax
Materials and tools
- Paper, pencil, and metric ruler
Procedure
- Tape paper together to make a strip at least 1 meter long. Draw a straight line down the 1m length the paper and mark it at 10cm intervals.

- Position the paper on a wall or window such that you can stand at least 8 feet away.
- Take your position between 8 and 12 feet from your meter grid. Measure your distance D to grid in meters.
- Hold your thumb up about 20 cm (8 inches, the width of a sheet of paper) from your eyes, and align it between the grid marks. Record the distance r1 to your thumb in meters.
- Close one eye and look at your thumb. Record its apparent position x1 against the background grid and which eye you are using.
- Close that eye and open the other. Record your thumb's new apparent position x2 against the background grid.
- Repeat the two measurements with your thumb at arm's length (X3, X4). Record the distance r2 to your thumb in meters.
- Measure the separation E between the center of your eyes (or use the "normal" value 2.5in = 6.3cm).
Data Analysis
- Calculate the separation of the two measurements at the shorter distance S1 =|x2 - x1|.
- Calculate the separation of the two measurements at the greater distance S2 = |X2 - X1|.
- There are 360° in a circle = 2πr. If we set r = 1, we can calculate the ratio 360/2π = 57.3 and use this to convert linear distance to circumference degrees, or angular measurements.Convert your separation measurements to angular measurements in degrees using the relationship θ1 = S1 * 57.3°/(D - r1). Make sure that S1, r1, and D use the same units!
- Repeat your calculation for θ2 = S2 * 57.3° /(D - r2).
- We now have two proportional triangles, related by a common angle θ:

Using the separation E for your eyes, calculate the distance between your eyes and your thumb for the short position using r1 = 57.3°E / θ
- Repeat the above calculation for the distance to your thumb in the far position, using r2.
- Compare your computations for the distances to your thumb with the distances you measured. Are you calculations reasonable?
- The star ε Eridani has a parallax angle θ of 310.94 milliarcseconds (310.94 * 10-3arcsec). Can you determine the distance to this star using the Earth's baseline distance E = 2 * Earth's distance to the sun = 2 * 150 * 106km?
Data Table and Calculations
Trial |
Distance D observation position to grid |
Distance r to Thumb |
Separation S |
Angular measure θ = S * 57.3°)/(D - r) |
Far Separation with Thumb at close distance (20-25cm) |
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Far Separation Thumb at far distance (60-80cm) |
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Eye separation (20-25cm) |
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Eye Separation Thumb at far distance (60-80cm) |
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Report
Write a report of all your observations and post it to the lab assignment link at the Moodle.
- A description of the equipment and procedures you used in sufficient detail for someone else to repeat your experiment.
- All of your data, in tabular form if possible.
- All of your computations and conclusions for the data analysis section.
- Any other observations you think interesting or important.
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