| http://www.w3.org/ns/prov#value | - In a planetary or solar gravitationalpotential K = exp(2GM/rc02) > 1 (M is a local mass distribution, r is the radial distance from the center ofM) while K = 1 in ???empty??? or free asymptotic space (Puthoff, 1999a, 2002a, b; Puthoff et al., 2002).
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