I-Space Research Institute ye-Russian Academy of Sciences (IKI RAS), ngokusho kwe-TASS, icacise izinhlelo zokuqaliswa kwe-Venera-D mission, okuhloswe ngayo ukuhlola iplanethi yesibili yesimiso sonozungezilanga.
Le phrojekthi ihilela ukuxazulula izinkinga eziningi zesayensi. Lolu ucwaningo olunzulu lomkhathi, indawo engaphezulu, isakhiwo sangaphakathi kanye ne-plasma ezungezile yeVenus.
I-architecture eyisisekelo ihlinzeka ngokudalwa kwezimoto ezijikelezayo nezihlala phansi. Owokuqala kuzodingeka afunde amandla, ubunjalo be-superrotation yomkhathi weVenus, ukwakheka okuqondile kanye nokwakheka kwamafu, ukusatshalaliswa kanye nemvelo ye-absorber engaziwa yemisebe ye-ultraviolet, ukukhishwa kwamanzi ebusweni ebusuku, njll. .
Ngokuqondene nemodyuli yokufika, kuzodingeka ifunde ukwakheka kwenhlabathi ekujuleni kwamasentimitha ambalwa, izinqubo zokusebenzisana kwezinto ezingaphezulu nomkhathi nomkhathi ngokwawo, kanye nomsebenzi wokuzamazama komhlaba.
Ukuze kuxazululwe ngokugcwele izinkinga zesayensi, ithuba lokufaka izimoto ezisizayo ku-mission zacwaningwa, ikakhulukazi, ama-satellites amabili amancane, okwakuhlongozwa ukuba kwethulwe endaweni ye-Lagrange amaphuzu L1 kanye ne-L2 yesistimu ye-Venus-Sun. Kodwa-ke, manje sekwaziwa ukuthi kunqunywe ukuthi kushiywe lawa ma-subsatellites.
βAmasathelayithi angaphansi abeyingxenye yohlelo olwandisiwe lweVenera-D. Ekuqaleni, sasihlele ukwethula amadivaysi amabili noma ngaphezulu afanayo ezindaweni ezimbili ezifanayo emzileni weVenus, okwakufanele afunde uhlobo lokusebenzisana phakathi komoya welanga, i-ionosphere kanye ne-magnetosphere yeVenus,β kusho i-Institute of Space. Ucwaningo lwe-Russian Academy of Sciences.
Ukwethulwa kwamadivayisi ngaphakathi kohlaka lwephrojekthi ye-Venera-D okwamanje kuhlelwe ngaphambi kuka-2029.
Imithombo:
Source: 3dnews.ru