The greater the distance to the star, the wider the baseline required for obtaining a discernible parallax. The distance d to the star (measured in parsecs) is equal to the reciprocal of the parallax angle p (in arc-seconds): The parallax of the star is equal to the angular radius of the Earth's orbit as seen from the star. The closer a star is to the Earth the greater the observed parallax.įigure 3.1: Astronomers measure the apparent shift in the star's position at different times of the year.Īs in the diagram, the lines of sight and the line connecting the observer's position form a triangle, with the star at the apex. As the Earth orbits the Sun during this period, the observer (taking measurements at the opposite sides of the Earth's orbit) notices an apparent movement of the star compared to more distant stars. To determine the distance to a star, astronomers measure the apparent change in its position over one year. Next article: Stellar Parallax > Stellar Parallax
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