An international team of astrophysicists led by a scientist from the Sternberg Astronomical Institute of the Lomonosov Moscow State University has reported the discovery of a binary solar-type star inside supernova remnant RCW 86. Spectroscopic observation of this star reveals that its atmosphere is polluted by heavy elements ejected during the supernova explosion that produced RCW 86. In particular, it was found that the calcium abundance in the stellar atmosphere exceeds the solar abundance by a factor of six, which hints at the possibility that the supernova might belong to a rare type of calcium-rich supernova, enigmatic objects whose origin is yet not clear. The research results are published in Nature Astronomy on 2017 April, 24.