mainly composed of hydrogen and helium
helium
hydrogen
hydrogen
hydrogen
Gas giants are primarily made up of hydrogen and helium, with small amounts of other gases such as methane and ammonia. They have no solid surface and their atmosphere becomes increasingly dense towards the core.
Mainly hydrogen and helium - which were also the main elements in the early Universe.
The atmosphere of gas giants like Jupiter and Saturn is primarily composed of hydrogen and helium, along with trace amounts of other gases like methane and ammonia. These gases create the thick and colorful cloud layers that are characteristic of these planets.
Saturn is considered one of the gas giants because it consists primarily of a gaseous atmosphere, with a small solid core. The other gas giants are Jupiter, Uranus and Neptune.
Gas giants are planets whose atmosphere is predominantly composed of gases, such as hydrogen and helium. These planets have a small solid core surrounded by thick layers of gas. Examples of gas giants in our solar system include Jupiter and Saturn.
helium, with traces of other gases like methane and ammonia. These planets have thick atmospheres that consist of several layers, each with different compositions and properties. The presence of hydrogen and helium in the atmosphere contributes to the large size and low density of gas giants.
Gas giants have enormous atmospheres, it may be said they consist only of atmosphere. They have a large mass, and they have rings.Gas giants have enormous atmospheres, it may be said they consist only of atmosphere. They have a large mass, and they have rings.Gas giants have enormous atmospheres, it may be said they consist only of atmosphere. They have a large mass, and they have rings.Gas giants have enormous atmospheres, it may be said they consist only of atmosphere. They have a large mass, and they have rings.
Hydrogen. The atmosphere of gas giants like Jupiter and Saturn consists mostly of hydrogen and helium, with small amounts of other gases like methane and ammonia. These gases are present in such large quantities that they give the planets their distinctive appearance and properties.