Parsec to Decimeter Converter

A parsec (pc) is a unit of length used in astronomy, equal to approximately 3.26 light-years or 206,265 astronomical units. It is defined as the distance at which one astronomical unit subtends an angle of one arcsecond.

The parsec was defined in 1913 by British astronomer Herbert Hall Turner. The name combines 'parallax' and 'arcsecond', referring to the trigonometric parallax method used to measure stellar distances. It became the preferred unit for professional astronomical distance measurements.

Parsecs are the standard unit for measuring stellar and galactic distances in professional astronomy. They're used in stellar catalogs, galactic structure studies, and cosmological research. Kiloparsecs and megaparsecs are used for larger cosmic distances.

A decimeter (dm) is a unit of length in the metric system equal to one-tenth of a meter (0.1 m). It provides a convenient intermediate measurement between centimeters and meters.

The decimeter was established as part of the original metric system in 1795. The prefix 'deci-' comes from the Latin word 'decimus' meaning 'tenth'. While part of the original system, it has seen limited adoption in most practical applications.

Decimeters are occasionally used in some European countries for certain measurements, particularly in education to help students understand metric relationships. They may appear in some technical drawings or scientific contexts, but centimeters and meters are generally preferred.