I-Space Research Institute ye-Russian Academy of Sciences (IKI RAS), ngokwe-TASS, icacise izicwangciso zokuphunyezwa kwe-mission ye-Venera-D, ejoliswe ekuhloleni iplanethi yesibini yelanga.
Le projekthi ibandakanya ukusombulula uluhlu olubanzi lweengxaki zenzululwazi. Olu luphononongo olubanzi lwe-atmosfera, umphezulu, isakhiwo sangaphakathi kunye ne-plasma ejikelezayo yeVenus.
Uyilo olusisiseko lubonelela ngokudala i-orbital kunye neenqwelo zokuhlalisa. Eyokuqala kuya kufuneka ifunde i-dynamics, ubume be-superrotation ye-atmosphere yeVenus, isakhiwo esithe nkqo kunye nokubunjwa kwamafu, ukuhanjiswa kunye nendalo ye-absorber engaziwayo yemitha ye-ultraviolet, ukukhutshwa komphezulu kwicala lasebusuku, njl. .
Ngokuphathelele imodyuli yokumisa, kuya kufuneka ifunde ukubunjwa komhlaba kubunzulu beesentimitha ezininzi, iinkqubo zokusebenzisana kwezinto ezingaphezulu kunye nomoya kunye nomoya ngokwawo, kunye nomsebenzi we-seismic.
Ukusombulula ngokupheleleyo iingxaki zenzululwazi, ukubakho kokubandakanya izithuthi ezincedisayo kwi-mission zafundwa, ngokukodwa, ii-satellites ezimbini ezincinci, ezicetywayo ukuba ziqaliswe kwiindawo zeLagrange L1 kunye ne-L2 yenkqubo yeVenus-Sun. Nangona kunjalo, ngoku kuye kwaziwa ukuba kuye kwagqitywa ukuba ziyeke ezi subsatellites.
βIi-subsatellites beziyinxalenye yenkqubo eyandisiweyo yeVenera-D. Ekuqaleni, sicebe ukusungula izixhobo ezimbini okanye ngaphezulu ezifanayo kwiindawo ezimbini ezifanayo kwi-orbit yeVenus, ebekufanele ukuba ifunde ubunjani bobudlelwane phakathi komoya welanga, i-ionosphere kunye nemagnetosphere yeVenus, "latsho iZiko leSithuba. Uphando lwe-Academy yaseRashiya yeSayensi.
Ukuqaliswa kwezixhobo ngaphakathi kwesakhelo seprojekthi yeVenera-D okwangoku kucwangciswe ngaphambi kowama-2029.
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umthombo: 3dnews.ru