Wo àyọkà tó wà nísàlẹ̀ yìí, kó o sì dáhùn ìbéèrè tó wà lẹ́yìn náà ní èdè kan náà tí àyọkà náà wà:  Ìlà: 34He → 12C + γ + 7.2 MeVIn massive stars, heavier elements can also be burned in a contracting core through the neon-burning process and oxygen-burning process. In massive stars, heavier elements can also be burned in a contracting core through the neon-burning process and oxygen-burning process.In massive stars, heavier elements can also be burned in a contracting core through the neon-burning process and oxygen-burning process.In massive stars, heavier elements can also be burned in a contracting core through the neon-burning process and oxygen-burning process.In massive stars, heavier elements can also be burned in a contracting core through the neon-burning process and oxygen-burning process. Ipele ikẹhin ninu ilana nucleosynthesis irawọ jẹ ilana sisun silisiomu ti o fa ni iṣelọpọ ti isotopu iduroṣinṣin irin-56, ilana endothermic ti o jẹ agbara, ati nitorinaa agbara siwaju le ṣee ṣe nikan nipasẹ isubu gravitational. Apẹẹrẹ ti o wa ni isalẹ fihan iye akoko ti o nilo fun irawọ 20 M<unk> lati jẹ gbogbo epo iparun rẹ. Bí ìràwọ̀ tí ó wà ní ìsọ̀rí O-class, yóò jẹ́ ìlọ́po 8 ti radius oòrùn àti ìlọ́po 62,000 ti ìmọ́lẹ̀ oòrùn.  Ìbéèrè: Àwọn ọ̀nà wo la lè gbà fi iná sun àwọn ohun tó wúwo jù lọ nínú ohun èlò kan tó ń dín kù?
ilana sisun neon ati ilana sisun atẹgun