U e{j @s.dZddlZddlmZddlmZGdddeZedd d d d d ddZeddej e dd ej e ddddZ edddej e dd dej e ddddZ eddddd dddZeddddd dddZed d!d"d#d dddZed$d%ej ejj d&ejj ejj ej ejj d'ejjddZed(d)d*d d dddZed+d,d-d#d dddZed.d/ej ejj d&ejj ejj ej ejj d'ejjddZed0d1d2d d dddZed3d4d5d#d dddZed6d7ej ejj d&ejj ejj ej ejj d'ejjddZed8d9d:d d dddZdS);z Astronomical and physics constants in SI units. See :mod:`astropy.constants` for a complete listing of constants defined in Astropy. N)codata)Constantc@seZdZdZiZeZdS)IAU2015zIAU 2015N)__name__ __module__ __qualname__Zdefault_reference _registrysetZ_has_incompatible_unitsr r X/var/www/html/bwave/python/venv/lib/python3.8/site-packages/astropy/constants/iau2015.pyrsrauzAstronomical Unitg6-]jABmgzIAU 2012 Resolution B2si)systempcZParsecg߼xV42?z2Derived from au + IAU 2015 Resolution B 2 note [4]kpcZ Kiloparsecg@@L_bol0z.Luminosity for absolute bolometric magnitude 0g_u( SVEWzIAU 2015 Resolution B 2L_sunzNominal solar luminositygOMMPsEzIAU 2015 Resolution B 3GM_sunzNominal solar mass parameterg^M(4Dz m3 / (s2)M_sunz Solar massZkgzIAU 2015 Resolution B 3 + R_sunzNominal solar radiusgŻAGM_jupzNominal Jupiter mass parameterg@'K!|CM_jupz Jupiter massR_jupz!Nominal Jupiter equatorial radiusg AGM_earthzNominal Earth mass parameterg@3fBM_earthz Earth massR_earthzNominal Earth equatorial radiusgTXA)__doc__numpynpconfigrZconstantrrr valueradiansZ uncertaintyrrrrrG referencerrrrrrrrr r r r s