Function solar_mass_param_f (o2scl_const)¶
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template<class fp_t>
fp_t o2scl_const::solar_mass_param_f(size_t system = o2scl_mks) Solar mass times gravitational constant ( \( \mathrm{m}^3 / \mathrm{s}^2 \) in MKS and \( \mathrm{cm}^3 / \mathrm{s}^2 \) in CGS; IAU 2015 value, see https://arxiv.org/abs/1510.07674)
Note that this value differs slightly in Barycentric Coordinate Time and Barycentric Dynamical Time. This is the IAU’s nominal value.