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Izimbobo ezimnyama ziyizifunda ezisemkhathini ezinamandla adonsela phansi anamandla ngendlela emangalisayo, lapho kungekho lutho, ngisho nokukhanya, okungaphunyuka. Zisuka kumbono ka-Albert Einstein wokuhlobana okujwayelekile futhi ziza ngobukhulu obuhlukahlukene, ngobuningi bazo obunquma amandla nomthelela wazo. Izimbobo ezimnyama zezinkanyezi kwakheka lapho izinkanyezi ezinkulu ziwa, kuyilapho izimbobo ezimnyama ezinkulu kakhulu zitholakala enkabeni yemithala eminingi, kuhlanganise nowethu. Naphezu kwemvelo yabo yokubamba ukukhanya, ososayensi bakwazile ukubona ubukhona babo ngokusebenzisa amandla abo adonsela phansi ezintweni ezizungezile nokukhanya. Muva nje, isithombe sokuqala esiqondile somgodi omnyama omkhulu sithwetshulwe yi-Event Horizon Telescope, siqhubeka nokubekela inselele ukuqonda kwethu kwendawo yonke.
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I-Betelgeuse iyinkanyezi ebomvu eyi-supergiant etholakala kumlaza i-Orion engenye yezinkanyezi ezinkulu nezikhanya kakhulu ezibonakala ziseMhlabeni. Isiseduze nokuphela komjikelezo wayo wokuphila, ngemva kokuqeda uphethiloli wayo oyinhloko we-hydrogen futhi yaqala ukuhlanganisa i-helium ezintweni ezisindayo, futhi kukholakala ukuthi iyisandulela somcimbi omangalisayo we-supernova. Izazi zezinkanyezi zisebenzise amasu ahlukahlukene ukutadisha izici ezingaphezulu ze-Betelgeuse, ukuhlukahluka kwezinga lokushisa, nezinye izici, futhi ngasekupheleni kuka-2019 nasekuqaleni kuka-2020, yaba nesenzakalo esifiphele ngokungavamile. Lokhu kuye kwaholela ekuqageleni ukuthi kungenzeka ukuthi i-supernova, futhi ukutadisha ukuqhuma kwayo ekugcineni kwe-supernova kuzonikeza ukuqonda okubalulekile ngezigaba zokugcina zokuziphendukela kwezinkanyezi.
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