- Astronomical length/distance
A parsec is also equivalent to approximately 3.26 light years (the journey distance if you travelled at the speed of light for three years and three months).
Astronomers used trigonometry to calculate the distance to stars long before the term parsec was coined, but the new unit made it easier to conceptualise unfathomable distances.
A parsec is the distance from the sun to an astronomical object which has a parallax angle of one arcsecond (1/3600 of a degree). The parallax angle is found by measuring the parallax motion (or apparent movement of a star relative to stable, more distant stars) when the star is observed from opposite sides of the Sun (an interval of six months on Earth). The parallax angle is obtained by halving the angular difference in measurements.
Once the parallax angle is established you can calculate the distance to a star using trigonometry, because we know Earth’s distance from the Sun. The distance from the Sun of a body with a parallax angle of 1 arcsecond was thus defined as a unit and, thanks to Turner, named the parsec.
With the parsec defined, deriving and describing huge distances became easy, since a distance i
The term parsec was coined by British astronomer Herbert Hall Turner in 1913. A unit of distance useful in astronomy had been defined but was without a name, and the Astronomer Royal appealed for suggestions. Turner’s was accepted – parsec being derived from the definition of the unit as the distance from the sun to an astronomical object which has a parallax angle of one arcsecond.
- Proxima Centauri – the nearest star to the Earth other than the Sun, is 1.29 parsecs away.
- The centre of the Milky Way is over 8kpc from the earth.
Astronomy – despite the enormous distance it describes, the parsec is a relatively small unit in astronomical terms. The megaparsec (Mpc) is commonly used to describe distances of one million parsecs.
- kiloparsec (kpc) – 1,000 pc
- megaparsec (Mpc) – 1,000,000 pc
- gigaparsec (Gpc) – 1,000,000,000 pc