| .. _astropy-constants: |
|
|
| ******************************* |
| 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 metadata describing their provenance and uncertainties. |
|
|
| Getting Started |
| =============== |
|
|
| To use the constants in International System of Units (SI 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 of the constants you |
| need, you can 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 conveniently 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 2014 |
|
|
| >>> print(const.c.to('km/s')) |
| 299792.458 km / s |
|
|
| >>> print(const.c.to('pc/yr')) |
| 0.306601393788 pc / yr |
|
|
| You can then use them in conjunction with unit and other nonconstant |
| `~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)) |
| 0.3675671602160826 N |
|
|
| It is possible to convert most constants to Centimeter-Gram-Second (CGS) units |
| using, for example:: |
|
|
| >>> const.c.cgs |
| <Quantity 2.99792458e+10 cm / s> |
|
|
| 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 |
| <Quantity 4.8032045057134676e-08 Fr> |
|
|
| .. _astropy-constants-prior: |
|
|
| Collections of Constants (and Prior Versions) |
| ============================================= |
|
|
| Constants are organized into version modules. The constants for |
| ``astropy`` 1.3 can be accessed in the ``astropyconst13`` module. |
| For example: |
|
|
| >>> from astropy.constants import astropyconst13 as const |
| >>> print(const.e) |
| Name = Electron charge |
| Value = 1.602176565e-19 |
| Uncertainty = 3.5e-27 |
| Unit = C |
| Reference = CODATA 2010 |
|
|
| Physical CODATA constants are in modules with names like ``codata2010`` or |
| ``codata2014``: |
|
|
| >>> from astropy.constants import codata2010 as const |
| >>> print(const.h) |
| Name = Planck constant |
| Value = 6.62606957e-34 |
| Uncertainty = 2.9e-41 |
| Unit = J s |
| Reference = CODATA 2010 |
|
|
| Astronomical constants defined (primarily) by the International Astronomical |
| Union (IAU) are collected in modules with names like ``iau2012`` or ``iau2015``: |
|
|
| >>> from astropy.constants import iau2012 as const |
| >>> print(const.L_sun) |
| Name = Solar luminosity |
| Value = 3.846e+26 |
| Uncertainty = 5e+22 |
| Unit = W |
| Reference = Allen's Astrophysical Quantities 4th Ed. |
| |
| >>> from astropy.constants import iau2015 as const |
| >>> print(const.L_sun) |
| Name = Nominal solar luminosity |
| Value = 3.828e+26 |
| Uncertainty = 0.0 |
| Unit = W |
| Reference = IAU 2015 Resolution B 3 |
| |
| The astronomical and physical constants are combined into modules with |
| names like ``astropyconst13`` and ``astropyconst20``. To temporarily set |
| constants to an older version (e.g., for regression testing), a context |
| manager is available as follows: |
| |
| >>> from astropy import constants as const |
| >>> with const.set_enabled_constants('astropyconst13'): |
| ... print(const.h) |
| Name = Planck constant |
| Value = 6.62606957e-34 |
| Uncertainty = 2.9e-41 |
| Unit = J s |
| Reference = CODATA 2010 |
| >>> print(const.h) |
| Name = Planck constant |
| Value = 6.62607004e-34 |
| Uncertainty = 8.1e-42 |
| Unit = J s |
| Reference = CODATA 2014 |
| |
| .. warning:: |
| |
| Units such as ``u.M_sun`` will use the current version of the |
| corresponding constant. When using prior versions of the constants, |
| quantities should be constructed with constants instead of units. |
| |
| .. note that if this section gets too long, it should be moved to a separate |
| doc page - see the top of performance.inc.rst for the instructions on how to |
| do that |
| .. include:: performance.inc.rst |
| |
| Reference/API |
| ============= |
| |
| .. automodapi:: astropy.constants |
| |