We investigate the variation of the gravitational constant G over the history of the Universe by modeling the effects on the evolution and asteroseismology of the low-mass star KIC 7970740, which is one of the oldest (∼ 11 Gyr) and best-observed solar-like oscillators in the Galaxy. From these data we findĠ/G = (1.2 ± 2.6) × 10 −12 yr −1 , that is, no evidence for any variation in G. We also find a Bayesian asteroseismic estimate of the age of the Universe as well as astrophysical S-factors for five nuclear reactions obtained through a 12-dimensional stellar evolution Markov chain Monte Carlo simulation.