An avalanche-like emission of red hot dust and gases typically refers to a volcanic eruption or an explosive event in which a large amount of volcanic material is ejected rapidly. This phenomenon can occur when magma rises to the surface, causing the surrounding rock to fragment and release superheated gases and ash. The resultant flow of hot material can travel down the slopes of a volcano, resembling an avalanche due to its speed and destructive power. Such eruptions can pose significant hazards to nearby communities and ecosystems.
A cloud of hot gas and dust in space is typically referred to as a nebula. Nebulae are vast regions of interstellar material where new stars are born or where dying stars expel their outer layers. These clouds can vary in size, shape, and composition, creating beautiful and diverse astronomical structures.
A planet is formed out of hot gases revolving around the Sun.
That is molten lava flowing on a cushion of hot gases, typically seen in volcanic eruptions.
pyroclastic flow. It is a fast-moving mixture of hot gases, ash, and volcanic rocks that can travel down the sides of a volcano at great speeds, reaching temperatures of hundreds of degrees Celsius. Pyroclastic flows are extremely dangerous and can cause widespread destruction in their path.
its pretty much selfexplanitory, its fluids (liquids and or gases) that are hot.
An "Active" volcano.
Hot clouds of dust and reactive gases
star is made up of hot gases star is made up up of hot gases
A nebula is a region of interstellar gas and dust. Emission nebulae are clouds of ionized gas that allow red, blue, and violet light through. Generally, these nebulae appear reddish. Reflection nebulae are clouds of dust that simply reflect light from nearby stars. The dust particles of reflection nebulae usually only scatter blue light, so the appearance is blue. Other types of nebulae don't reflect light. Dark nebulae such as the Horsehead Nebula are so dense that they block light from other sources, such as background emission nebulae, reflection nebulae, or other stars.
All hot solids or dense enough gases emit black body radiation. Gases that are not very dense are are cold absorb particular wavelengths while gases that are not dense but are hot produce their characteristic emission spectrum.
S. C. Saxena has written: 'Thermal accommodation and adsorption coefficients of gases' -- subject(s): Absorption and adsorption, Accommodation coefficient, Gases 'Dust removal from hot and compressed gas streams by fibrous- and granular-bed filters' -- subject(s): Cleaning, Dust, Filters and filtration, Gases, Removal
An emission nebula is created when hot, young stars emit high-energy ultraviolet radiation, which ionizes the surrounding gas, causing it to glow. Additionally, the gas and dust clouds within the nebula act as the raw material required for the formation of such structures in space.
The glowing clouds that you see in pictures from space are called emission nebulas. A emission nebula is a cloud of hot, glowing cloud of gas and dust in space. These nebulas absorb the light of nearby stars and reach very high temperatures. The high temperature causes them to glow. Emission nebulas are often found in regions of space where new stars are forming.
A cloud of hot gas and dust in space is typically referred to as a nebula. Nebulae are vast regions of interstellar material where new stars are born or where dying stars expel their outer layers. These clouds can vary in size, shape, and composition, creating beautiful and diverse astronomical structures.
Hot dust storms are common in Thar because of low pressure and hot dry wind .
it is a hot gas
In a fusion reactor the hot gases or plasma are contained within a magnetic field.