Ezinye izazinzulu zikholelwa ukuba iplani yesithoba ebizwa ngokuba yi-Nnity ye-Ninet inokuhamba ibe ngumngxunya omnyama omnyama. Into enkulu yendawo inokufunyanwa yi-radiation iphuma kumda wayo obizwa ngokuba yi-radiation ye-hoculation.
Ukukhangela ubungqina obucacileyo bobukho beplanethi ejikelezileyo ngaphaya kwe-orbit neptne ne-neptune yayingathwelwa ngempumelelo. Iminyaka emininzi ye-Astronomers ifaka ikhohluko yeplanethi yeplanethi yokuqikelela ubukho beeplanethi ezintsha. Ukuba umjikelezo weplanethi enesifo sokuqikelela ayihambelani nezazinzulu zeNzululwazi (umzekelo, ngokufumana ithiyori ephuculweyo). Ke ukungakwazi kokukhanya kwesayensi kuchazwe ngokuchanekileyo ngumjikelezo we-mercury kwinkangeleko yethiyori ye-Einstein. Ukuziphatha okungafunekiyo kwi-UNIFT ye-Uranium ngaphezulu kwesiphelo senkqubo yelanga kube sisizathu sokuvulwa kweplanethi yeNeptune.
Iqela labavumisi ngeenkwenkwezi ngo-2016 kuvavanywa ukuqokelelwa kwezinto ezikude zeSolar System. Amaziko amancinci omkhenkce abizwa ngokuba yiTransneptunova izinto zibekwe kwi-orbit emnyama ngaphandle kwe-neptune orbit. Abanye babo bangxamisekileyo benza ingqungquthela. Amathuba okuqhayisa kunokwenzeka ngethuba-ngaphantsi kwe-1%. Le nyaniso yenze ukuba iingcali zibonisa ukuba kunokubakho iplanethi enkulu - into engaphezulu kwe-neptune ijikeleza amaxesha ali-10 ukusuka kwilanga xa kuthelekiswa ne-neptune.
Bayibiza le meko ye-hypothetical kwiplanethi yesithoba. Umbono uthi amandla omoya onjalo unokufumana ezi tno kwi-ororedits yeqela.
NgoFebruwari, abaphandi babeka phambili ingcinga yokuba ubungqina bobukhosi besithoba kubandakanya iQela le-Tno lunokuba sisiphumo see-telescopes zayo. Ngamanye amagama, ezi tnos zinokuhlelwa ngenxa yokuqwalaselwa kwenzululwazi yenzululwazi. Kwiminyaka emihlanu kamva, iPlanethi yesithoba ayizange ifunyanwe.
Inkuthazo emnyama
Ukuba iplanethi yesithoba ikwindawo apho ikhoyo kwicandelo le-orbit yakhe elithathayo kude nelanga kangangokuba izazi ngeenkwenkwezi azinakumbona esebenzisa itekhnoloji yale mihla. Izazinzulu james Avin imele iYunivesithi yaseIncibini kunyeYakub Stolz kwiYunivesithi yaseDaurus yeza kwisiphelo esitsha-iPlanethi yesithoba inokuba ngumngxunya omnyama. Olu hypothesis unokuchaza ukuba kutheni i-telescopes ayikayifumani into engaqondakaliyo.
I-ormits Anomalies ingaba sisiphumo sefuthe lomngxunya omnyama. Oku kuthelekiswa nemingxunya emnyama evelayo ngenxa yokuwa kwenkanyezi yenziwa kwi-plasma eshushu kumanqanaba okuqala kobomi bendalo. Imingxunya emnyama enjalo inokuba ngobukhulu obutsha. Ngokobalo lwe-astrophysics, into yolu hlobo kunye nobunzima bamaxesha amahlanu ngaphezulu kunokuba ubunzima behlabathi buphawulwa yiradius ukuya kuthi ga kwiisentimitha ezi-4 5.
Umngxunya ophambili ophawulwa yimitha encinci, kodwa i-halo ukusuka kwinto emnyama ibe yimicimbi emibini okanye emithathu idlulela kuyo ngeenxa zonke kuyo. Ababhali besi sifundo bakholelwayo: Ekuphela kwendlela yokubonisa ubukho bomngxunya omnyama omncinci endaweni yesithoba kukuchonga imithombo yokuhamba ye-gamma yemitha.
Kwizazinzulu zemvula, kubaluleke kakhulu ukufumanisa umngxunya omnyama omnyama kumda weSolar System. Ukuba ubonakalisa indawo yeSolar System. ukujikeleza kumngxunya omnyama. Izazinzulu ziya kukwazi ukubona imeko engqongqo engqongqo. Izakhono zeTekhnoloji ze-NASA zikuvumela ukuba wenze kwaye uqhubeke nohlobo lwexesha elide lwendawo entsha yokuhamba ukuya kumngxunya omnyama osondeleyo kwindalo yonke.