Astrophysics (index)about

Parsec

(pc)
(about 3.26 light-years)

A Parsec is the distance corresponding to a Parallax of one arcsecond, i.e., if an object shows a parallax of one arcsecond, it is one parsec from the Sun.

Equivalence:

If a star appears to move back and forth two arcseconds over the course of a year as the Earth moves to and from a spot 2 AU away (1 arcsecond parallax angle), the star is 1 parsec distant. If the movement is half that, then the star is twice as distant.


(distance,unit)
http://en.wikipedia.org/wiki/Parsec

Referenced by:
Absolute Magnitude (M)
Astronomical Quantities
Astronomical Unit (AU)
Baryon Acoustic Oscillations (BAO)
Bok Globule
Distance Modulus (u)
DQ Tau
Dwarf Galaxy
F-Type Star (F)
Filament
Final Parsec Problem
Galaxy
GJ 1132 b
GJ 1214 b
Gould's Belt
Kennicutt-Schmidt Law
Magnitude
Molecular Cloud
NANOGrav
Nessie
Orion Nebula Cluster (ONC)
Orion Molecular Cloud Complex
Parallax
PAWS
Rho Ophiuchi Cloud Complex
Scholz's Star
Stellar Distance Determination
Taurus-Auriga Complex
Taurus Molecular Cloud 1 (TMC-1)
Trapezium Cluster
Wide-Field Multi-Object Spectrograph (WFMOS)

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