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Why are earth-based parallax measurements limited to only the nearest star?

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Why are earth-based parallax measurements limited to only the nearest star?

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When astronomers average together many observations they cannot measure parallax with an uncertainty smaller than about 0.002 second of an arc. If you measure a parallax of 0.02 seconds of arc, the uncertainty is about 10 percent. That means that ground-based astronomers can’t measure accurate parallaxes smaller than about 0.02 second of arc, which corresponds to a distance of 50 pc. Consequently, ground-based parallax measurements are limited to only the closest stars.

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