Answer: C
Step-by-step explanation:
From the information about dependence of planetesimal composition on distance from the Sun and the existence of the frost line resulted in two main types of planets in our Solar System: the inner rocky planets and the outer gas giants. We have learned that planetesimal formation through accretion, and the types of materials that condensed at that distance from the Sun.
the most likely way the gas Giants are formed includes;
1) Metals: this metals can be, iron, nickel, aluminum. They condense at Temperature= 1,600 K and comprise only 0.2% of the nebula.
2) Rocks: which are silicon-based minerals that condense at Temperature =500-1,300 K and comprises only 0.4% of the nebula.
3) Ices: contains hydrogen compounds like methane (CH4), ammonia (NH3), water (H2O) that condense at 150 K Temperature and make up 1.4% of the nebula.
4) Light gases: these light gases includes, hydrogen and helium that never condensed in the disk (98% of the disk which are gravitationally attracted.