Hydrogen and helium within giant planets are largely in a liquid state because the intense pressure within these planets compresses the gases to high densities, causing them to transition from gaseous to liquid states. The temperatures within giant planets are also high enough to keep hydrogen and helium in a liquid form.
Jupiter is a gas giant composed mostly of hydrogen and helium gases. It doesn't have a solid surface like rocky planets, but rather a dense atmosphere that transitions into a liquid layer deeper inside the planet.
Jupiter, the first gas giant from the sun. It's clouds are made out of simple gases like hydrogen,helium,carbon dioxide,water and methane,along with clouds of ammonia ice and ammonium hydrosulphide. There are winds up to 600km per hour,travelling in opposite directions which create the distinct bands. Saturn is composed entirely of hydrogen. The top layer is made up of ammonia crystals and below are ammonium hydrosulphide or water. Beneath the layer of cloud,the pressure is so intense that gas is compressed into a liquid. Uranus's atmoshere is mostly hydrogen and helium, with small quantities of methane. This allows the planet to be able to absorb the Sun's rays, giving the planets distinct blue colour. Neptune has no solid surface to land on. It may have a tiny core of rock.Neptune's atmosphere is mostly hydrogen and helium with traces of methane.
Jupiter does not have a solid surface or crust like rocky planets such as Earth. Instead, it is composed mainly of hydrogen and helium in its outer layers, with a possible rocky core at its center.
No, water is not the lightest liquid on Earth. Liquid hydrogen and liquid helium are lighter than water because they have lower densities.
The word equation for liquid helium is: Helium gas → Liquid helium.
Helium is colder than hydrogen at the same temperature because helium has a lower boiling point (-268.9 degrees Celsius) compared to hydrogen (-252.9 degrees Celsius).
Gasses and ice . (:
Jupiter is a gas giant composed mostly of hydrogen and helium gases. It doesn't have a solid surface like rocky planets, but rather a dense atmosphere that transitions into a liquid layer deeper inside the planet.
The primary composition of gas giant atmospheres is typically hydrogen and helium, with smaller amounts of methane, ammonia, and water vapor. These planets have thick layers of gas that gradually transition into a liquid or ice layer as you move towards the core.
Saturn and Jupiter
The planet you are referring to is Uranus, the seventh planet from the Sun. It is composed mostly of hydrogen and helium, with a layer of frozen water, ammonia, and methane, along with a liquid nitrogen layer on its surface.
Jupiter, the first gas giant from the sun. It's clouds are made out of simple gases like hydrogen,helium,carbon dioxide,water and methane,along with clouds of ammonia ice and ammonium hydrosulphide. There are winds up to 600km per hour,travelling in opposite directions which create the distinct bands. Saturn is composed entirely of hydrogen. The top layer is made up of ammonia crystals and below are ammonium hydrosulphide or water. Beneath the layer of cloud,the pressure is so intense that gas is compressed into a liquid. Uranus's atmoshere is mostly hydrogen and helium, with small quantities of methane. This allows the planet to be able to absorb the Sun's rays, giving the planets distinct blue colour. Neptune has no solid surface to land on. It may have a tiny core of rock.Neptune's atmosphere is mostly hydrogen and helium with traces of methane.
Jupiter and Saturn are gas giants composed primarily of hydrogen and helium. Uranus and Neptune are ice giants that have a smaller gas component but are primarily composed of water, ammonia, and methane.
Saturn is made out of hydrogen (75%) and helium (25%).
kerosene
liquid nitrogen will not freeze everything. Hydrogen and helium will remain a gas when exposed to liquid nitrogen.
Jupiter does not have a solid surface or crust like rocky planets such as Earth. Instead, it is composed mainly of hydrogen and helium in its outer layers, with a possible rocky core at its center.