Machadka Cilmi-baarista Hawada Sare ee Akadeemiyada Sayniska ee Ruushka (IKI RAS) ayaa sheegaysa in ka-qaybgalayaasha mashruuca ExoMars-2016 ay daabaceen natiijooyinkii ugu horreeyay ee falanqaynta xogta laga helay aaladaha Trace Gas Orbiter (TGO).
Aan ku xasuusino in ExoMars ay tahay mashruuc wadajir ah oo Roscosmos ah iyo Wakaaladda Hawada Yurub, oo lagu fuliyay laba marxaladood. Marxaladda koowaad - 2016 - moduleka orbital TGO iyo Schiaparelli lander waxay aadeen Meeraha Cas. Midka kowaad wuxuu si guul leh u ururiyaa macluumaadka sayniska, iyo kan labaad, hoogay, shil.
TGO-da waxaa ku jira dhismaha ACS ee Ruushka iyo aaladda Belgian NOMAD, oo ku shaqeysa kala duwanaanshaha infrared ee spectrum electromagnetic. spectrometer-yadan waxa loogu talagalay in lagu duubo qaybo yaryar oo jawiga ka kooban yahay - gaas kuwaas oo xooggoodu aanay dhaafin dhawr qaybood halkii bilyan ama xataa trillion, iyo sidoo kale boodhka iyo hawada hawada.
Mid ka mid ah yoolalka ugu muhiimsan ee howlgalka TGO waa in la ogaado methane, taas oo muujin karta nolosha Mars ama ugu yaraan dhaqdhaqaaqa volcano socda. Jawiga meeraha cas, molecules methane, haddii ay muuqdaan, waa in lagu baabi'iyaa shucaaca ultraviolet ee qorraxda laba ilaa saddex qarni gudahood. Sidaa darteed, diiwaangelinta molecules methane waxay muujin kartaa dhaqdhaqaaq dhawaan (nafley ama volcano) meeraha.
Nasiib darro, weli suurtagal ma ahayn in la ogaado methane jawiga Martian. "ACS spectrometers, iyo sidoo kale spectrometers ee dhismaha NOMAD ee Yurub, kama aysan helin methane Mars intii lagu jiray cabbirada laga bilaabo Abriil ilaa Agoosto 2018. Indho-indhaynta waxa lagu sameeyay qaabka qorrax-madoobaadka dhammaan latitudes,β ayay tiri daabacaadda IKI RAS.
Si kastaba ha ahaatee, tani macnaheedu maaha in aanu jirin methane gabi ahaanba jawiga meeraha cas. Xogta la helay ayaa dejisay xadka sare ee feejignaantiisa: methane ku jira jawiga Mars ma noqon karo wax ka badan 50 qaybood trillion. Macluumaad dheeraad ah oo ku saabsan daraasadda ayaa laga heli karaa halkan.
Source: 3dnews.ru