# Constants

AstroBase.Constants.astronomical_unitMethod
astronomical_unit([[T=Float64], unit=KiloMeter()])

Return the astronomical unit $au$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.drift_rateMethod
drift_rate([T=Float64,] TDB, TCB)

Return the rate of drift between TDB and TCB $L_B$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.drift_rateMethod
drift_rate([T=Float64,] TCG, TCB)

Return the rate of drift between TCG and TCB $L_C$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.drift_rateMethod
drift_rate([T=Float64,] TT, TCG)

Return the rate of drift between TT and TCG $L_G$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.earth_rotation_angle_j2000Method
earth_rotation_angle_j2000([T=Float64])

Return the Earth rotation angle at J2000.0 $\theta_0$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.earth_rotation_rateMethod
earth_rotation_rate([T=Float64])

Return the rate of advance of Earth rotation angle $d\theta/dUT1$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.equatorial_radius_earthMethod
equatorial_radius_earth([[T=Float64], unit=KiloMeter()])

Return the equatorial radius of Earth $a\_E$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.gaussian_gravitational_constMethod
gaussian_gravitational_const([T=Float64])

Return the Gaussian gravitational constant $k$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.geocentric_gravitational_constMethod
geocentric_gravitational_const([[[T=Float64], scale=TDB], unit=KiloMeter()])

Return the geocentric gravitational constant $GM_E$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.geoid_potentialMethod
geoid_potential([T=Float64])

Return the geoid potential and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.gravitational_constMethod
gravitational_const([[T=Float64], unit=KiloMeter()])

Return the gravitational constant $G$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.heliocentric_gravitational_constMethod
heliocentric_gravitational_const([[[T=Float64], scale=TDB], unit=KiloMeter()])

Return the heliocentric gravitational constant $GM_S$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.j2_factor_earthMethod
j2_factor_earth([T=Float64])

Return $J_2$ dynamical form factor of Earth and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.j2_rate_earthMethod
j2_rate_earth([T=Float64])

Return the time rate of change in $J_2$ of Earth and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_ceresMethod
mass_ratio_ceres([T=Float64])

Return the ratio of the mass of Ceres to the mass of the Sun $M_{Ceres}/M_S$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_erisMethod
mass_ratio_eris([T=Float64])

Return the ratio of the mass of the Sun to the mass of Eris $M_S/M_{Eris}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_jupiterMethod
mass_ratio_jupiter([T=Float64])

Return the ratio of the mass of the Sun to the mass of Jupiter $M_S/M_{J}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_marsMethod
mass_ratio_mars([T=Float64])

Return the ratio of the mass of the Sun to the mass of Mars $M_S/M_{Ma}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_mercuryMethod
mass_ratio_mercury([T=Float64])

Return the ratio of the mass of the Sun to the mass of Mercury $M_S/M_{Me}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_moonMethod
mass_ratio_moon([T=Float64])

Return the ratio of the mass of the Moon to the mass of Earth $M_M/M_E$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_neptuneMethod
mass_ratio_neptune([T=Float64])

Return the ratio of the mass of the Sun to the mass of Neptune $M_S/M_{N}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_pallasMethod
mass_ratio_pallas([T=Float64])

Return the ratio of the mass of Pallas to the mass of the Sun $M_{Pallas}/M_S$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_plutoMethod
mass_ratio_pluto([T=Float64])

Return the ratio of the mass of the Sun to the mass of Pluto $M_S/M_{P}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_saturnMethod
mass_ratio_saturn([T=Float64])

Return the ratio of the mass of the Sun to the mass of Saturn $M_S/M_{Sa}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_uranusMethod
mass_ratio_uranus([T=Float64])

Return the ratio of the mass of the Sun to the mass of Uranus $M_S/M_{U}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_venusMethod
mass_ratio_venus([T=Float64])

Return the ratio of the mass of the Sun to the mass of Venus $M_S/M_{Ve}$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mass_ratio_vestaMethod
mass_ratio_vesta([T=Float64])

Return the ratio of the mass of Vesta to the mass of the Sun $M_{Vesta}/M_S$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.mean_angular_velocity_earthMethod
mean_angular_velocity_earth([T=Float64])

Return nominal mean angular velocity of Earth $\omega$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.obliquity_j2000Method
obliquity_j2000([T=Float64])

Return the ratio of the mass of the Moon to the mass of Earth $M_M/M_E$ and the associated uncertainty.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.speed_of_lightMethod
speed_of_light([[T=Float64], unit=KiloMeter()])

Return the speed of light $c$.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source
AstroBase.Constants.tdb0Method
tdb0([T=Float64])

Return TDB–TCB at T0.

Reference

• Luzum, Brian, et al. "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy." Celestial Mechanics and Dynamical Astronomy 110.4 (2011): 293.
source