B
    d	                 @   sn  d Z ddlZddlmZ G dd deZeddd	d
ddddZeddejee	d d
ej
ee	d dddZedddej ee	d d
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d(dddZed)d*d+d#ddddZed,d-d.d
d/dddZed0d1d2d#d3dddZed4d5d6d
d7dddZdS )8z
Astronomical and physics constants in SI units.  See :mod:`astropy.constants`
for a complete listing of constants defined in Astropy.
    N   )Constantc               @   s   e Zd ZdZi Ze ZdS )IAU2012zIAU 2012N)__name__
__module____qualname__Zdefault_reference	_registrysetZ_has_incompatible_units r
   r
   f/work/yifan.wang/ringdown/master-ringdown-env/lib/python3.7/site-packages/astropy/constants/iau2012.pyr      s   r   auzAstronomical Unitg  6-]jABmg        zIAU 2012 Resolution B2si)systempcZParsecg߼xV42?zDerived from aukpcZ
Kiloparsecg     @@L_bol0z.Luminosity for absolute bolometric magnitude 0g_u(
SVEWzIAU 2015 Resolution B 2L_sunzSolar luminosityg*n|#sEgJ-Dz(Allen's Astrophysical Quantities 4th Ed.M_sunz
Solar massg 9FZkgg52DER_sunzSolar radiusg   NAg     d@M_jupzJupiter massgtEER_jupzJupiter equatorial radiusg   Ag     @@M_earthz
Earth massgPXEg@xDR_earthzEarth equatorial radiusg    TXAg      ?)__doc__numpynpZconstantr   r   r   valuetanradiansZuncertaintyr   r   r   r   r   r   r   r   r   r   r
   r
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   r   <module>   s<   	
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