Kule veki iJuno space probe ifake iifoto ezimbalwa zeJupiter ebomvu iSupor Storm. Isisombululo esiphakamileyo, sithathiwe kufutshane, imifanekiso esondeleyo ye 16.350km isaqhwithi. Ububanzi bayo buphinda-phindwe ngo-1,3 kunobo bomhlaba. Kuqikelelwa ukuba malunga neminyaka eyi-150 ubudala, nangona kunokwenzeka ukuba emva kweenkulungwane ezimbalwa ezalandelayo. Kwaye nangona yaqwalaselwa okokuqala kwi-1830, sele ekuqaleni kwe-1600 indawo encinci ebomvu yabonwa eJupiter. Oku kulandela ukuba inokuba efanayo.
Bakhe I-640km / h imimoya ijika i-anticyclonicOko kukuthi, ngokuchasene neenkqwithela ezininzi. Kwaye iyancipha. Emva kweminyaka yokuqwalaselwa, kuyajongwa ukuba ubukhulu bayo buncipha njani kancinci kancinci. Ngeli xesha akukho mfanekiso ungaphambili-wesithwathwa sakhe. Inkqubo kaJuno, ehamba nge-50km ngomzuzwana, kwaye oko Kukhutshwa ngo-Agasti 5, 2011, isinika le mifanekiso kunye neevidiyo zesaqhwithi, ezo iminyaka emininzi izazi ngeenkwenkwezi ziye zathi.
Ukungaziwa kwesiphango
Imibala yayo ebomvu iseyimfihlakalo. Ngokwezifundo ezenziweyo, amafu eatmosferi angaphezulu kungenzeka ukuba abe nehydrogen sulfide, ammonia, kunye namanzi. Into engacacanga kukuba ezi khompawundi zisabela njani ekugqibeleni zinike lo mbala.
Enye engaziwayo. Kutheni le nto isaqhwithi singadinwa, kwaye siqhubeke nokubetha ngokungapheliyo emva kwamakhulu eminyaka? Izazinzulu ezininzi zikholelwa ekubeni unobangela unokuza nzulu, kwiingcambu zesaqhwithi. Kungenxa yoko le nto kubalulekile ukuba wazi okungaphantsi. Inkqubo yophando lweJuno icwangciselwe indlela yayo elandelayo ngoSeptemba 1.
Le vidiyo ikhawulezayo ilandelayo isibonisa umphezulu weJupiter efakwe kuphando lweJuno.
Imifanekiso efakwe kwiwebhusayithi ye-NASA isimahla kubemi abafuna ukuyihlela kunye nokuphucula. Uninzi lwazo ngenene luphethwe ngabemi bezenzululwazi abaye baphucula imifanekiso kwiwebhu yeJunoCam.
Indlela ende yokuhamba
Iphenyo likaJuno, eliza kuba neminyaka emi-6 ubudala ukusungulwa kwalo, liphethe ukuphanda esi saqhwithi sikhulu. Lixhotyiswe abenzi boluvo ukubona imagnethi, kunye nokufumanisa ubume bomoya Jupiter. I-NASA inethemba lokuqonda ukuba lisebenza njani eli "bala", Utyhile imibuzo engekasonjululwa.
UScott Bolton, uMphandi oyiNtloko Uphengululo lukaJuno kwiSouthWest Research Institute eSan Antonio, eTexas, yanikela le ngxelo: “Ngoku sinemifanekiso ebalaseleyo yesi saqhwithi sidumileyo. Kuya kusithatha ixesha ukuhlalutya idatha, hayi nje kwiJunoCam, kodwa kwizixhobo ezisibhozo zesayensi, ukukhanyisa ukukhanya okwadlulayo, okwangoku kunye nekamva leRed Spot.
Eyona planethi inkulu kwiNkqubo yeLanga, ifakiwe nevidiyo
Ukuba kukho into uJupiter eyahlukileyoKungenxa yokuba yeyona planethi inkulu kuzo zonke iNkqubo yeLanga. Kunye Ububanzi obuphantse bube yi-140.000km, malunga namaxesha ali-11 kuMhlaba, Ikwanazo neentsuku ezimbalwa (ixesha lokujikeleza) phantse nge-10 kusasa, 9:56 am ukuba zichaneke. Ukudityaniswa kwerhasi ubukhulu becala, kwaye ujikeleze ngesantya esiphezulu, kuyenza ingabi ngqukuva ngokupheleleyo, kodwa icaba.
Kwimeko apho nabani na engenakucinga ngobungakanani bayo obukhulu, lo mfanekiso ulandelayo wenza ukuba kube lula ukuthelekisa.
Eminye imifanekiso esinikwe yona ivela kwiwebhu
Kwaye elandelayo, ngokweenkcukacha, amafu kaJupiter. Emangalisayo.
Kule vidiyo ilandelayo, siyaboniswa indlela elandelwa nguJuno kweyona ndawo ikufutshane ithatha indawo yamandla kazibuthe kaJupiter. Isizathu sokuba ingasoloko isondela kufutshane nayo kukuba ayichaphazeleka yimitha, nangona uJuno efumanise ukuba iphindaphindwe kalishumi kunoko bekulindelwe. Kungenxa yoko le nto kwi indawo yayo ekufutshane idlula malunga ne-8.000km kwaye endaweni yoko inqaku layo lingaphezulu kakhulu kude.
Xa uJuno edlula kufutshane neJupiter kwakhona ukuze asinike ingxelo yeefoto zakhe ezintle kunye neziphumo, ukusuka Meteorología en Red Siza kuqaphela ukuba sizisasaze kuye wonke umntu.
Hlala ubukele, kuba ukuba uyithandile, utyelelo olulandelayo lwezithembiso zokwenza uphando!