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Proper Motion

Bernard's Star in Ophiuchus has the largest apparent motion, at 10.3" per year. - Steve Quirk

Proper motion refers to the apparent motion of stars across the sky over time as observed from Earth. This motion is caused by the actual motion of the stars through space. It's important to note that proper motion is distinct from the apparent daily motion of stars caused by Earth's rotation.

Stars move due to their individual velocities through the galaxy. This motion can be observed by comparing the position of a star relative to distant, fixed reference points over time. Proper motion is typically measured in arcseconds per year (arcsec/yr), where one arcsecond is 1/3600th of a degree.

The study of proper motion is essential for understanding the dynamics of our galaxy and the universe. It helps astronomers determine the orbits of stars within the Milky Way, identify stars belonging to star clusters or moving groups, and investigate the distribution of mass in the galaxy.

Astronomers use techniques like astrometry, which precisely measures the positions and motions of celestial objects, to determine proper motions. This can be done by comparing images taken at different times, typically using instruments like space telescopes or large ground-based telescopes equipped with advanced cameras.

Proper motion can also be combined with measurements of a star's radial velocity (its motion along the line of sight) to determine its true space velocity relative to the Sun.



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