Examine this table. What might a planet's composition be if the planet formed in a region of the solar nebula where the temperature was about 1050 K? O metal oxides O metallic iron and nickel O silicates O feldspars O troilite (FeS) O H₂O ice O ammonia-water ice O methane-water ice O argon-neon ice Temperature (K) 1500 1300 1200 1000 680 175 150 120 65 Condensate Metal oxides Metallic iron and nickel Silicates Feldspars Trolite (FeS) Water ice Ammonia-water ice Methane-water ice Argon-neon ice Object; Estimated Temperature of Formation (K) Mercury, 1400 Venus: 900 Earth, 600 Mars: 450 Jovian; 175 Pluto: 65
Examine this table. What might a planet's composition be if the planet formed in a region of the solar nebula where the temperature was about 1050 K? O metal oxides O metallic iron and nickel O silicates O feldspars O troilite (FeS) O H₂O ice O ammonia-water ice O methane-water ice O argon-neon ice Temperature (K) 1500 1300 1200 1000 680 175 150 120 65 Condensate Metal oxides Metallic iron and nickel Silicates Feldspars Trolite (FeS) Water ice Ammonia-water ice Methane-water ice Argon-neon ice Object; Estimated Temperature of Formation (K) Mercury, 1400 Venus: 900 Earth, 600 Mars: 450 Jovian; 175 Pluto: 65
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Transcribed Image Text:Examine this table. What might a planet's composition be if the planet formed in a region of the solar nebula where the temperature was about 1050 K?
O metal oxides
O metallic iron and nickel
O silicates
O feldspars
O troilite (FeS)
O H₂O ice
O ammonia-water ice
O methane-water ice
O argon-neon ice
Temperature
(K)
1500
1300
1200
1000
680
175
150
120
65
Condensate
Metal oxides
Metallic iron and nickel
Silicates
Feldspars
Troilite (FeS)
Water ice
Ammonia-water ice
Methane-water ice
Argon-neon ice
Object; Estimated
Temperature of
Formation (K)
Mercury, 1400
Venus; 900
Earth; 600
Mars; 450
Jovian; 175
Pluto; 65
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