Parallax Angle Formula:
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Definition: This calculator determines the parallax angle (θ) based on the baseline distance (b) and the distance to the object (d).
Purpose: It helps astronomers, surveyors, and photographers calculate angular measurements for distance estimation and perspective analysis.
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 determining astronomical distances, 3D imaging, and various surveying applications.
Tips: Enter the baseline distance (b) and object distance (d) in meters. Both values must be positive numbers.
Q1: What is parallax angle used for?
A: It's primarily used in astronomy to measure stellar distances, in photography for 3D effects, and in surveying for distance measurements.
Q2: What's a typical baseline distance for astronomical measurements?
A: For stellar parallax, astronomers often use Earth's orbital diameter (2 AU ≈ 300 million km) as the baseline.
Q3: How accurate is this calculation?
A: For small angles (when d ≫ b), the approximation θ ≈ b/d (in radians) is often used, but this calculator provides the exact arctangent value.
Q4: Can I use different units?
A: Yes, as long as both b and d use the same units. The calculator currently expects meters but will work with any consistent unit.
Q5: Why does the angle decrease as distance increases?
A: Because the same baseline spans a smaller angular width when viewed from greater distances (inverse relationship).