Abanye ososayensi bakholelwa ukuthi ilangabi elibizwa ngokuthi yi-ninth planethi ingahle ibe nomgodi omncane omnyama. Into enkulu yesikhala ingatholwa yi-radiation ephumayo evela emaphethelweni ayo ibizwa ngokuthi imisebe ye-hocling.
Ukucinga kobufakazi obucacile bokuba khona kweplanethi ejikeleza kude kakhulu kwe-Orbit Neptune bekungathweswa umqhele ngempumelelo. Iminyaka eminingi yezazi zezinkanyezi zisebenzisa ukuhlukahluka kwezindawo zeplanethi ukubikezela ubukhona bamaplanethi amasha. Uma umjikelezo weplanethi ngokubikezela akuhlanganisi ososayensi bavuselela i-physics (ngokwesibonelo, ngokuthola umbono othuthukisiwe wamandla adonsela phansi). Ngakho-ke ukungakwazi ukukhanya kwesayensi kuchazwe ngokunembile yi-orbiry ye-mercury kuholele ekubonakaleni komqondo ka-Einstein. Ukuziphatha okungaqondakali ku-orbium ye-uranium ekugcineni okuphambene kohlelo lwelanga sekuyisizathu sokuvulwa kwePetune Planet.
Iqembu lezazi zezinkanyezi ngonyaka we-2016 lihlolisise ukuqoqwa kwezinto ezikude kakhulu zohlelo lwelanga. Imizimba emincane ebizwa ngokuthi yizinto zeTransneptunova zitholakala e-Orbit emnyama ngaphandle kweNeptune Arbit. Ezinye zazo zenhlangano ye-trajectory zihlangana. Amathuba okuthi ukuhlanganisa kungenzeka ngengozi - ngaphansi kwe-1%. Leli qiniso lenza ochwepheshe liphakamise ukuthi kungenzeka kube neplanethi enkulu - okuthile okungaphezulu kweNeptune kujikeleze izikhathi ezingaphezu kwezingu-10 ukusuka elangeni ngokuqhathaniswa neNeptune.
Babiza lo mhlaba we-hypothetical kuwena eplanethi yesishiyagalolunye. Umqondo uthi amandla adonsela phansi anjalo angathola lezi zinhlaka ku-orbits yeqembu.
NgoFebhuwari, abacwaningi babeka umcabango wokuthi ubufakazi bokuba khona kweplanethi yesishiyagalolunye kubandakanya neqembu lezinkanyezi lingaba umphumela wezazi zezinkanyezi zithumela isayensi ebukhoma. Ngamanye amagama, lezi zinhlaka zingahlelwa njengeqembu ngenxa yokubonwa kososayensi "onopelene". Eminyakeni emihlanu kamuva, iplanethi yesishiyagalolunye ayikaze itholakale.
Isisusa Esimnyama
Uma iplanethi eyisishiyagalolunye itholakala ngempela endaweni ethile lapho kungaba khona engxenyeni yomjikelezo wakhe owuthatha kude kakhulu nelanga ukuthi izazi zezinkanyezi azikwazi ukuzibona zisebenzisa ubuchwepheshe besimanje. Ososayensi uJames Anvin abamele i-Illinois University kanti uYakub Stolz waseDaurus University wafika esiphethweni esisha - iplanethi yesishiyagalolunye ingaba umgodi omncane omnyama. Lokhu kwengqondo kungachaza ukuthi kungani ama-telescopes engakaze athole into engaqondakali yesikhala.
I-Orbits Anomalies ingahle ibe ngumphumela womthelela womgodi omnyama oyinhloko. Lokhu kuqhathaniswa nezimbobo ezimnyama ezinkulu ezivela ngenxa yokuwa kwenkanyezi kwakhiwa kusuka ku-Plasma eshisayo ezigabeni zokuqala zempilo yempilo yempilo yonke. Izimbobo ezinjalo ezimnyama zingaba namasayizi amancane. Ngokwezibalo ze-astrophysics, into yalolu hlobo ngesisindo esiphindwe kahlanu esiphakeme kunobuningi bomhlaba buhlukaniswa yimisebe yamasentimitha ayi-4.
Umgodi oyisisekelo ubonakaliswa ngemisebe emincane, kepha i-halo kusuka ezinkulu ezimnyama zaba amayunithi amabili noma amathathu ezinkanyezi ezinqwabeleyo inyukele kuyo okuzungezile. Abalobi besifundo bakholelwa: Ukuphela kwendlela yokufakazela ubukhona bomgodi omncane omnyama esikhundleni seplanethi yesishiyagalolunye ukuthola imithombo eshukumisayo yemisebe ye-gamma.
Zezazi zezinkanyezi, kubaluleke kakhulu ukuthola umgodi omncane omnyama onqenqemeni lwesistimu yelanga. Uma unquma indawo yento, khona-ke ukuthunywa okuqondiwe kuzothola ithuba lokusondela ekuvulekeni kwemicimbi futhi kwenziwe ukujikeleza emgodini omnyama. Ososayensi bazokwazi ukubona imvelo enkulu kakhulu. Amandla wezobuchwepheshe we-NASA akuvumela ukuthi udale futhi usebenzise inguqulo yesikhathi eside yezindawo ezintsha zokuhambela umgodi omnyama oseduze - into engaqondakali kuyo yonke indawo.