Duba wurin da ke ƙasa sannan ka amsa tambayar daga baya a cikin harshe ɗaya kamar yadda wurin yake:  Passage: A kimanin 1.15 M<unk>, IK Pegasi B ana ɗaukarsa a matsayin babban dwarf fari. Kodayake ba a lura da radius ɗin sa kai tsaye ba, ana iya kimanta shi daga sanannun alaƙar ka'idoji tsakanin taro da radius na fararen dwarfs, yana ba da darajar kusan 0.60% na radius na Sun. (Wani tushe daban ya ba da darajar 0.72%, don haka akwai sauran rashin tabbas a cikin wannan sakamakon.) Don haka wannan tauraron yana tattara taro mafi girma fiye da Rana a cikin girma kusan girman Duniya, yana ba da alamar wannan abu mai tsananin yawa. Babban, yanayin haɗin gwiwar farin dwarf yana haifar da ƙarfin nauyi mai ƙarfi. Masanan taurari suna nuna wannan darajar ta wurin logarithm na goma na ƙarfin nauyi a cikin raka'a cgs, ko log g. Don IK Pegasi B, log g shine 8.95. Ta hanyar kwatanta, log g ga Duniya shine 2.99. Saboda haka nauyi a kan IK Pegasi ya fi sau 900,000 na ƙarfin nauyi a duniya. An kiyasta yawan zafin jiki na IK Pegasi B ya kasance kusan 35,500 ± 1,500 K, yana mai da shi tushen tushen hasken ultraviolet. A cikin yanayi na yau da kullum wannan farin dwarf zai ci gaba da sanyaya fiye da shekaru biliyan, yayin da radius zai kasance ba zai canza ba.  Tambaya: Ta yaya za a iya auna radius na wani farin dwarf?
daga sanannun dangantakar ka'idoji tsakanin taro da radius na fararen dwarfs