reflection nebula- An interstellar cloud of gas and dust that shines because light from nearby bright stars is reflected or scattered toward us. The emission component of the spectrum is due to the gas, the reflection component is due to the dust.
Nebulae glow because they are made up of gas and dust particles that are illuminated by nearby stars. These particles scatter and reflect starlight, creating the glowing appearance. Additionally, some nebulae may also emit light due to processes such as ionization or radiation.
A planetary nebula is a glowing shell of gas and dust formed by a star shedding its outer layers at the end of its life. Despite its name, it has nothing to do with planets. The glowing gas is illuminated by the hot core of the star left behind, known as a white dwarf.
This description is of a nebula. Nebulae are vast regions of interstellar gas and dust, often illuminated by nearby stars or glowing from the energy of newly forming stars within them. The colors and shapes of nebulae can vary depending on the types of gases present and the processes occurring within them.
A nebula is a cloud of gas and dust in space where new stars are formed. These regions are often characterized by the presence of young, hot stars surrounded by glowing gas and dark dust.
The Orion Nebula was not formed from a single supernova or nova event. It is a stellar nursery where new stars are currently being formed. The nebula is created by the glowing gas and dust illuminated by newly formed stars within it.
A glowing cloud of gas is typically a nebula, which is a large cloud of gas and dust in space that emits light due to the presence of energized atoms and molecules. These clouds can be illuminated by nearby stars or by processes such as shockwaves or radiation from massive stars.
Nebula
Nebula
A cloud in outer space consisting of gas or dust and planetry nebula is one of the types also called ring nebula or A planetary nebula is an emission nebula consisting of a glowing shell of gas
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.
in the middle of a nebula lies a glowing neutron star or a white dwarf with highly concentrated mass at extremely high densities.
The spectrum of the Orion Nebula (M42) would show emission lines typical of hot, ionized gas, such as hydrogen-alpha and doubly ionized oxygen. This is because the gas in the nebula is being energized by nearby hot stars, causing it to emit light at specific wavelengths.
The explosion (a supernova) produces a glowing cloud of gas (called a nebula) that slowly expands and dissipates (eg the crab nebula).
Nebulae glow because they are made up of gas and dust particles that are illuminated by nearby stars. These particles scatter and reflect starlight, creating the glowing appearance. Additionally, some nebulae may also emit light due to processes such as ionization or radiation.
A planetary nebula is a glowing shell of gas and dust formed by a star shedding its outer layers at the end of its life. Despite its name, it has nothing to do with planets. The glowing gas is illuminated by the hot core of the star left behind, known as a white dwarf.
This description is of a nebula. Nebulae are vast regions of interstellar gas and dust, often illuminated by nearby stars or glowing from the energy of newly forming stars within them. The colors and shapes of nebulae can vary depending on the types of gases present and the processes occurring within them.
The Horsehead Nebula is a dark nebula located in the constellation Orion. It is a cloud of dust and gas that is backlit by a nearby bright star, giving it the distinctive shape that resembles the head of a horse. The nebula is a popular target for astrophotography due to its striking appearance.