Ezinsukwini ezimbalwa ezedlule bekungeyakhe NASA lowo owethula incwadi yabezindaba ememezela ukuthi banezindaba ezinhle abazongitshela zona. Ngemuva kwezinsuku ezimbalwa belindile, i-United States Space Agency igcine isishicilele isitatimende esisha lapho iveze khona ukuthi ithole i- iplanethi lesishiyagalombili elizungeza uKepler 90, inkanyezi efana nelanga lethu elisendaweni yokukhanya eyiminyaka engu-2.545 XNUMX ukusuka eMhlabeni.
Ukubaluleka kwalokhu okutholakele, ngaphezu kokwazi ukuthi iKepler 90 ineplanethi entsha ezungezayo, kutholakala kubuchwepheshe obusetshenzisiwe. Kusengaphambili, ngikutshele ukuthi kulokhu i-NASA icacisile ukuthi ukusebenzisana kwe-google, inkampani enikeze ipulatifomu ye- ukuhlakanipha okufakelwayo ikwazi ukuphatha izigidi zemininingwane yolwazi erekhodwe yi I-Kepler Space Telescope.
IGoogle neNASA bakhombisa ukuthi kunezimfihlo eziningi ongazithola ezinkulungwaneni zedatha eyenziwe yiKepler Space Telescope
Ukungena emininingwaneni ethe xaxa, ngikutshele ukuthi labo ababhekene nokwakhiwa kwalolu hlelo lobuhlakani bokufakelwa bebekhona UChristopher Shallue, Unjiniyela Omkhulu Wesoftware kwaGoogle AI, Andrew Vanderberg, umuntu osebenza ngemuva kwe-NASA's Sagan Center, kanye nesazi sezinkanyezi esivela e-University of Texas (Austin).
Inqubo esetshenziselwe ukuthuthukiswa kohlelo kube yindlela ye- ukufunda imishini, yingakho leli thimba likwazile ukufundisa ikhompyutha ukukhomba amaplanethi emininingwaneni etholwe kusibonakude lapho iqopha ngokuzenzakalela uhlobo oluthile lwesiginali oluhlobene ne-exoplanet, leyo engaphezu kwesimiso sethu sonozungezilanga.
Ngenxa yalo msebenzi onzima, ubuhlakani bokufakelwa bukwazile ukuthola lokho okubhabhadiswe njengo UKepler-90i, i-exoplanet evelele phakathi kokunye ukuzungeza inkanyezi yayo kanye njalo ezinsukwini eziyi-14,4, inezinga lokushisa eliphakathi nendawo elingaba cishe ama-800 degrees Fahrenheit (cishe ama-426.667 degrees Celsius) noma ngokukhula kwalo ngqo ngo-30% kunoMhlaba.
Njengoba kuphawuliwe UPaul Hertz, Umqondisi wamanje we-NASA's Astrophysics Division eWashington:
Njengoba besilindele, kunokutholwa okuthokozisayo phakathi kwedatha yethu egcinwe ku-Kepler, elinde ithuluzi elifanele noma ubuchwepheshe ukuyivula.
Lokhu okutholakele kukhombisa ukuthi idatha yethu izoba yindawo yokugcina amagugu kubacwaningi eminyakeni ezayo.
Ngenxa yalokhu okutholakele, izinsizakusebenza zizoqhubeka nokutshalwa ekwakhiweni kobuhlakani bokufakelwa obukhethekile ekuhlonzweni kwamaplanethi amasha
Akungabazeki ukuthi sibhekene nezindaba ezinhle ngoba, yize kutholakele i-exoplanet entsha, iqiniso ukuthi okulindelwe bekungekuhle kakhulu ekuqaleni, ikakhulukazi ngoba lokhu Akukhona okokuqala ukuthi kusetshenziswe ubuhlakani bokufakelwa ngesisekelo sedatha kaKepler. Lokhu kutholakala kukhombisa ukuthi ukusebenzisa amanethiwekhi we-neural kungaba yithuluzi elihle lezinkanyezi nesayensi jikelele.
Lapho nje kungenzeka ukukhombisa inani leli pulatifomu elingaba nalo ezinkulungwaneni zedatha egcinwe kwaKepler, akumangazi ukuthi iqembu eliphethe ukuthuthukiswa kwale phrojekthi selinqume ukusebenzisa ipulatifomu yalo hlaziya imininingwane iNASA enayo ezinkanyezini ezingaphezu kuka-150.000 ngenqubo yokuthi, noma kungathatha isikhathi eside, ingasinika izimanga eziningi ezinjengalezi.
Asikwazi ukulahleka, ngokusho kweNASA uqobo, ukuthi kuningi maningi amathuba okuthola impilo kwezinye izinhlelo zonozungezilanga kuneKepler-90. Noma kunjalo, ngokwethimba labaphenyi nonjiniyela, sikhuluma ngohlelo lwelanga oluluhlobo oluthile lwenguqulo yesimiso sethu sonozungezilanga ngoba lunamaplanethi womabili amancane engxenyeni yawo yangaphakathi namaplanethi amakhulu kakhulu engxenyeni yawo yangaphandle. Umehluko wangempela phakathi kwesimiso sethu sonozungezilanga neKepler-90 ukuthi lesi samuva sihlangene kakhulu. njengoba iplanethi yayo ekude kakhulu izungeza inkanyezi yayo ebangeni elifana ncamashi nalelo eliphakathi koMhlaba neLanga.