Labs / Astronomy

Parallax Distance Finder

As Earth swings from one side of its orbit to the other, a nearby star appears to slide back and forth against the far-off background. Drag Earth around its orbit and set the star's true distance — the tinier the wobble, the farther the star. The half-angle of that wobble, measured over a one-astronomical-unit baseline, is the parallax, and its distance in parsecs is simply 1 divided by that angle.

Labs / Astronomy / Parallax Distance Finder

Astronomy20–30 minFoundation

Parallax Distance Finder

As Earth swings from one side of its orbit to the other, a nearby star appears to slide back and forth against the far-off background. Drag Earth around its orbit and set the star's true distance — the tinier the wobble, the farther the star. The half-angle of that wobble, measured over a one-astronomical-unit baseline, is the parallax, and its distance in parsecs is simply 1 divided by that angle.

Why it matters

Why explore this?

Astronomy uses patterns in light and motion to explain objects we cannot touch directly. This model lets you change one part of a space system and see what the evidence would look like.