I-Space Research Institute ye-Academy yaseRashiya yeSayensi (IKI RAS) ibhengeza ukupapashwa kwengxelo kwisigaba sesibini somsebenzi weengcali ngaphakathi kwesakhelo seprojekthi yeVenera-D.
Injongo ephambili ye-mission yeVenera-D luphando olubanzi lweplanethi yesibini yenkqubo yelanga. Kule nto kucetywayo ukusebenzisa iimodyuli ze-orbital kunye nokuhlalisa. Ukongeza kwicala laseRashiya, i-US National Aeronautics and Space Administration (NASA) ithatha inxaxheba kule projekthi.
Ngoko ke, kuxelwa ukuba ingxelo epapashiweyo ibizwa ngokuba yi "Venera-D": Ukwandisa i-horizons yokuqonda kwethu imozulu kunye ne-geology yeplanethi yomhlaba ngokusebenzisa uphononongo olubanzi lweVenus.
Uxwebhu lubonisa ingcamango yeprojekthi, ebandakanya ukufunda umoya, umphezulu, isakhiwo sangaphakathi kunye neplasma ejikelezileyo yeVenus. Ukongeza, imisebenzi ephambili yenzululwazi iyaqulunqwa.
Imodyuli ye-orbital iya kufuneka ifunde i-dynamics, ubunjani be-superrotation ye-atmosphere yeVenus, isakhiwo esithe nkqo kunye nokwakhiwa kwe-atmosphere kunye namafu, ukuhanjiswa kunye nendalo ye-absorber engaziwayo yemitha ye-ultraviolet, njl.
Kucetywa ukuba kufakwe isikhululo esincinci, esihlala ixesha elide kwi-lander. Ezi modyuli ziya kufunda ukubunjwa komhlaba kubunzulu beesentimitha ezininzi, iinkqubo zokusebenzisana kwezinto ezingaphezulu kunye neatmosfera, kunye nomoya ngokwawo. Ubomi bezixhobo zokuhlalisa kufuneka zibe ziiyure ezi-2-3, kwaye isikhululo esihlala ixesha elide kufuneka sibe ubuncinane iintsuku ezingama-60.
Ukuqaliswa kweVenera-D kunokuqhutyelwa kwi-Vostochny cosmodrome usebenzisa i-Angara-A5 yokuqalisa imoto kwixesha elivela kwi-2026 ukuya kwi-2031.
umthombo: 3dnews.ru