Umoya weplanethi yoMhlaba wenziwe ngeegesi ezahlukeneyo, ezinje ngeoksijini, initrogen, iargon, iozone kunye nomphunga wamanzi. Zonke zidlala indima ebaluleke kakhulu kwimozulu yoMhlaba, kwaye ke ngoko kubomi obukhoyo kuye.
Xa sithetha ngotshintsho lwemozulu, ngamanye amaxesha kunokunika imvakalelo yokuba icarbon dioxide yirhasi enobungozi, kwaye kunjalo, kodwa kuphela kwimeko apho abantu bayaqhubeka ukungcolisa njengoko besenza, kuba ephezulu ezikhutshwayo, kokukhona ziya kubamba ubushushu kwaye kuphakame amaqondo obushushu. Ngoku, I-NASA idale ividiyo apho indlela yokuziphatha kwe-CO2 ibonakala khona ekhaya.
Izazinzulu ze-NASA zisebenzise ukuqaphela kwi-Orbiting Carbon Observatory (OCO-2) satellite ukwenza imodeli yokuziphatha kwekhabhoni ukusukela nge-1 kaSeptemba 2014 ukuya ku-31 Agasti 2015. Lo ngumzekelo onokusetyenziselwa ukuqikelela. apho ukugxila kuyakuba phezulu okanye kusezantsi.
Emva kokufunda ukukhutshwa kwe-CO2 amashumi eminyaka, Iingcali ngoku zinokuqokelela yonke le datha ukwenza isisombululo esiphakamileyo sokubonakala kwe-3D evumela nawuphi na umsebenzisi ukuba azi ukuba le gesi iziphatha njani emoyeni.
Ikharbhon diokside isebenza njenge thermostat. Ukuphakama koxinaniso, kokukhona ubushushu buya kubanjiswa ngaphakathi kwiplanethi, kukhawulezisa ukufudumala kwehlabathi. Ke, Kubalulekile ukuqonda ukuba zeziphi ezona ndawo zithatha ezona CO2 kwaye zingakanani.
Ividiyo ibonisa ukunyuka nokuwa kwe-CO2 kwiNyakatho yeNtlabathi unyaka wonke; impembelelo yamazwekazi, iinduli zeentaba, kunye nemisinga yolwandle kwiipateni zemozulu; kunye nefuthe lommandla wefotosinthesisi.
Ngolunye ulwazi, nqakraza apha.