Astronomical system of units
Reference
measured.astronomical
Defines units and constants of use in the field of astronomy, which requires measuring extremely large distances, masses, and periods of time.
The astronomical system of units is a tridimensional system, in that it defines units of length, mass and time. The associated astronomical constants also fix the different frames of reference that are needed to report observations.
Attributes: Units of length
AstronomicalUnit (Unit): A unit representing the average distance between the Earth
and the Sun; it is now defined precisely as 149,597,870,700 meters
LightYear (Unit): The distance light travels through a vacuum in one `JulianYear`
Spat (Unit): An obsolete unit of astronomical distance equaling 1 trillion meters
Parsec (Unit): A measure of large astronomical distances defined in terms of
[trigonometry and parallax][1]
[1]: https://en.wikipedia.org/wiki/Parsec
Siriometer (Unit): An obsolete unit of astronomical distance equaling 1 million AU
Attributes: Units of time
Day (Unit): Uses the same definition of `Day` as the SI system
SiderealDay (Unit): The `Time` it takes the Earth to make one rotation with respect
to distant stars, approximately 86164.0905 seconds, a few minutes shorter than
the SI Day.
JulianYear (Unit): defined as 365.25 days of 84,600 SI `Second`
Attributes: Units of mass
SolarMass (Unit): The mass of the Sun
EarthMass (Unit): The mass of the Earth
JupiterMass (Unit): The mass of Jupiter
Attributes: Units for astrophotometry
Jansky (Unit): A unit of spectral flux density
Crab (Unit): A unit for measuring the intensity of astromonical X-ray sources, based
on the intensity of the Crab Nebula
Attributes: Hubble's Law
H0 (Quantity): Today's estimate of the Hubble Parameter representing the observed
expansion rate of the universe
HubbleTime (Unit): An approximation of the age of the universe, if the expansion
rate had been linear
HubbleLength (Unit): The distance at which galaxies are receding from us at the
speed of light
HubbleVolume (Unit): The sphere within which galaxies are receding from us below
the speed of light