Parallax Angle Formula:
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Definition: This calculator computes the parallax angle (θ) based on the baseline distance between observation points (b) and the distance to the object (d).
Purpose: It helps astronomers, photographers, and 3D imaging professionals determine the apparent shift in an object's position when viewed from different angles.
The calculator uses the formula:
Where:
Explanation: The arctangent of the ratio between baseline and distance gives the parallax angle in radians, which is then converted to degrees.
Details: Accurate parallax angle measurement is crucial for distance determination in astronomy, stereo photography, and computer vision applications.
Tips: Enter the baseline distance between observation points and the distance to the object. Both values must be positive numbers in meters.
Q1: What is parallax used for in astronomy?
A: Astronomers use stellar parallax to measure distances to nearby stars by observing their apparent movement against distant background stars.
Q2: What's a typical baseline for astronomical measurements?
A: For nearby stars, astronomers often use Earth's orbital diameter (2 AU ≈ 300 million km) as the baseline.
Q3: How does this relate to 3D photography?
A: In stereo photography, the parallax angle determines the perceived depth, with the baseline being the distance between the two camera lenses.
Q4: Why is the result in degrees?
A: Degrees are more intuitive for most users than radians, though the calculation is done in radians internally.
Q5: What's the maximum possible parallax angle?
A: The theoretical maximum is 90° when the baseline equals the distance (d = b), but in practice angles are much smaller.