List of common astronomy symbols

From Wikipedia, the free encyclopedia

This is a compilation of symbols commonly used in astronomy, particularly professional astronomy.

Age (stellar)[]

  • τ - age

Astrometry parameters[]

Astrometry parameters

  • Rv - radial velocity
  • cz - apparent radial velocity
  • z - Redshift
  • μ - proper motion
  • π - parallax
  • J - epoch
  • α - Right Ascension
  • δ - Declination
  • λ - Ecliptic longitude
  • β - Ecliptic latitude
  • l - Galactic longitude
  • b - Galactic latitude

Cosmological parameters[]

Cosmological parameters

Distance description[]

Distance description for orbital and non-orbital parameters:

Galaxy comparison[]

Galaxy type and spectral comparison:

Luminosity comparison[]

Luminosity comparison:

  • LS, L - luminosity of the Sun (Sol)

Luminosity of certain object:

  • Lacc - accretion luminosity
  • Lbol - bolometric luminosity

Mass comparison[]

Mass comparison:

  • ME, MEarth - mass of Earth
  • MJ, M - mass of Jupiter
  • MS, M - mass of the Sun (Sol)

Mass of certain object:

Metallicity comparison[]

Metallicity comparison:

  • [Fe/H] - Iron ratio to Hydrogen, a logarithm representation of the ratio of a star's iron abundance compared to that of the Sun
  • [M/H] - Metallicity ratio.
  • Z - Metallicity
  • ZS, Z - Metallicity of the Sun (Sol)

Orbital parameters[]

Orbital Parameters of a Cosmic Object:

Radius comparison[]

Radius comparison:

  • RE, REarth - Radius compared to Earth
  • RJ, R - Radius compared to Jupiter
  • RS, R - Radius compared to The Sun (Sol)

Spectral comparison[]

Spectral comparison:

Temperature description[]

Temperature description:

  • Teff - Temperature Effect, usually associated with luminous object
  • Tmax - Temperature Maximum, usually associated with non-luminous object
  • Tavg - Temperature Average, usually associated with non-luminous object
  • Tmin - Temperature Minimum, usually associated with non-luminous object
  • K - Kelvin

See also[]

References[]

  1. ^ Ultra-luminous X-ray sources: X-ray binaries in a high/hard state?, Z. Kuncic, R. Soria, C. K. Hung, M. C. Freeland, G. V. Bicknell, 2006
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