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Earth Science · Astronomy & Space

Annual parallax and stellar distances

As Earth orbits the Sun, a nearby star appears to shift relative to background stars. Standard annual parallax is half the total angular shift between the two observations.

Related experiment: Annual parallax and distance →
Annual parallax and distance
Annual parallax and distance: simulation view →

Meaning and mechanism

Time difference is the phenomenon where the apparent direction of an object changes when the observation point is changed. The difference in direction is greater when the object is closer.

When observed from the opposite side of Earth’s orbit, the reference point is approximately 2 AU. Since the standard time offset, ‘p’, is defined relative to 1 AU, it is distinguished from the overall displacement 2p.

Relationships and conditions

In the small-angle approximation, d(pc)=1/p, with p measured in arcseconds. If p=0.1 arcseconds, the distance is 10 pc. Changing the baseline changes both the observed angular displacement and its conversion to distance.

It is necessary to consider observation errors, the proper motion of stars, and the shape of the differential ellipse depending on the position of celestial bodies. The magnified angles of the experiment are not read as the actual size of the sky.

What to observe in the simulation

If p=0.1″, then 10 pc≈32.6 light years. The more distant a star is, the smaller the parallax is.

It is a small angle approximation assuming a circular orbit and a star oriented perpendicular to the orbital plane. p is always the standard parallax angle for 1 AU. At radius b AU, total displacement = 2bp, distance = b/(displacement/2). Background stars are fixed and intrinsic motion, atmospheric shaking, and measurement errors are omitted. The screen angle is an enlarged picture, not the actual angle.

Key relationships and symbols

d(pc)=1/p(″) · Standard total angular displacement=2p

Symbols and units used in the formulas
SymbolMeaningUnit
pAnnual parallax for a 1 AU baselineArcseconds
dDistance to the starpc
AUReference mean Earth–Sun distanceUnit of length

Worked example

What is the relationship between the standard parallax p and the total angular displacement between the two observation points?

p is a semi-angle corresponding to the orbital radius of 1 AU. The total angular displacement at both ends is 2p and d(pc)=1/p(″).

Common misconceptions

  • If you directly input the entire coordinate change over 6 months into the standard p, you may obtain an incorrect distance.

Explore this concept through experiments

References

OpenStax · Measuring the Distance to Stars (English)