Thola izindlela zokubona umgodi omnyama. Zihlukanise ngo-"-" emigqeni eminingi.
Context:Ukuba khona komgodi omnyama kungacatshangwa ngokusebenzelana kwawo nenye into nangemisebe kagesi efana nokukhanya okubonakalayo. Noma yiluphi udaba oluwela emgodini omnyama lungakha idiski elingaphandle elifudunyezwa ukungqubuzana, libe ama-quasar, ezinye zezinto ezikhanyayo kunazo zonke endaweni yonke. Izinkanyezi ezidlula eduze kakhulu nomgodi omnyama omkhulu kakhulu zingase ziqhekeke zibe imisebe ekhanya ngokukhazimulayo ngaphambi kokuba "zigwinywe". Uma kunezinye izinkanyezi ezizungeza umgodi omnyama, imijikelezo yazo inganquma isisindo nendawo yomgodi omnyama. Ukuhlola okunjalo kungasetshenziselwa ukukhipha ezinye izindlela ezinjengezinkanyezi ze-neutron. Ngale ndlela, izazi zezinkanyezi ziye zathola izinkanyezi eziningi ezingase zibe izimbobo ezimnyama ezisezinhlelweni zezinkanyezi ezimbili futhi zathola ukuthi umthombo womsakazo owaziwa ngokuthi iSagittarius A*, osenkabeni yomthala i-Milky Way, uqukethe imbobo emnyama enkulu kakhulu enesisindo esicishe sibe yizigidi ezingu - 4,3 ezinesisindo selanga.
Umgodi omnyama ungabonwa ngezindlela ezilandelayo: - I-disc yokwanda evuthwa ukungqubuzana lapho into iwela emgodini omnyama.