“…Data on various atomic and nuclear properties and isotopic abundances are gathered frequently by different institutions, and every few years, international working groups release data sets of recommended values for many physical constants [Mohr et al, 2016] as well as atomic and nuclear properties [e.g., Audi et al, 2017;Wang et al, 2017;Meija et al, 2016a]. In this technical note, recent relevant data are gathered in order to calculate heat production rates for the six geologically most important heat-producing nuclides 26 Al, 40 K, 60 Fe, However, in b 2 ; b 1 , and (electron capture, ec) decays, a part E m of the energy is carried away by a neutrino or antineutrino, whose interaction with matter is almost nil and which therefore does not contribute to heat production or to driving chemical processes such as radiolysis; indeed, although this paper focuses on heat, the core issue really is how much of the decay energy causes any effect in matter, and so the following considerations concerning heat energy and power apply also to chemical reactions.…”