Stellar parallax is the apparent shift of a nearby star against the distant background when Earth moves from one side of its orbit to the other. The angle measured, called the parallax angle (p), is extremely smallβtypically measured in arcseconds.
Because the baseline of Earth’s orbit is known (1 astronomical unit on each side, giving a total baseline of 2 AU), the distance to the star can be derived directly from simple trigonometry. The relationship is inverse: a smaller parallax means a larger distance.
Astronomers define the parsec (pc) as the distance at which a star would have a parallax of exactly one arcsecond. Using this definition, the distance in parsecs is simply the reciprocal of the parallax angle measured in arcseconds.
What is stellar parallax?
How do you calculate distance from parallax angle?
Why is parallax used to measure distances in astronomy?
What is the unit of measurement for parallax angle?
How does a smaller parallax angle affect distance calculation?
What is the baseline used in parallax calculations?
Can parallax be used to measure distances to all stars?
Results are for informational purposes only and do not constitute professional advice.
