******************************* Constants (`astropy.constants`) ******************************* .. currentmodule:: astropy.constants Introduction ============ `astropy.constants` contains a number of physical constants useful in Astronomy. Constants are `~astropy.units.Quantity` objects with additional meta-data describing their provenance and uncertainties. Getting Started =============== To use the constants in S.I. units, you can import the constants directly from the `astropy.constants` sub-package:: >>> from astropy.constants import G or, if you want to avoid having to explicitly import all the constants you need, you can simply do: >>> from astropy import constants as const and then subsequently use for example ``const.G``. Constants are fully-fledged `~astropy.units.Quantity` objects, so you can easily convert them to different units for example:: >>> print(const.c) Name = Speed of light in vacuum Value = 299792458.0 Uncertainty = 0.0 Unit = m / s Reference = CODATA 2010 >>> print(const.c.to('km/s')) 299792.458 km / s >>> print(const.c.to('pc/yr')) # doctest: +FLOAT_CMP 0.306601393788 pc / yr and you can use them in conjunction with unit and other non-constant `~astropy.units.Quantity` objects:: >>> from astropy import units as u >>> F = (const.G * 3. * const.M_sun * 100 * u.kg) / (2.2 * u.au) ** 2 >>> print(F.to(u.N)) # doctest: +FLOAT_CMP 0.367669392028 N It is possible to convert most constants to cgs using e.g.:: >>> const.c.cgs However, some constants are defined with different physical dimensions in cgs and cannot be directly converted. Because of this ambiguity, such constants cannot be used in expressions without specifying a system:: >>> 100 * const.e Traceback (most recent call last): ... TypeError: Constant u'e' does not have physically compatible units across all systems of units and cannot be combined with other values without specifying a system (eg. e.emu) >>> 100 * const.e.esu # doctest: +FLOAT_CMP Reference/API ============= .. automodapi:: astropy.constants