The two main types of bright nebulae are emission nebulae, which emit light from ionized gases, and reflection nebulae, which reflect light from nearby stars. Emission nebulae are usually red or pink in color, while reflection nebulae appear blue due to scattering of light.
Reflection nebulae reflect light from nearby stars, appearing blue due to scattering of light by interstellar dust. Emission nebulae emit light themselves, typically due to ionized gases within the nebula that are excited by nearby hot stars.
Emission nebulae appear red when they surround blue stars because the blue stars emit high-energy ultraviolet radiation which ionizes the hydrogen gas in the nebula, causing it to emit red light through a process called hydrogen-alpha emission. This red light is more prominent than the blue light emitted by the stars, giving the nebula its red color.
Dark reflecting nebulae appear dark because they are dense clouds of gas and dust blocking the light from stars behind them. Light reflecting nebulae, on the other hand, appear bright because they reflect the light of nearby stars, often due to the presence of reflective dust particles.
The most abundant gas in emission nebulae in the Milky Way is hydrogen. Emission nebulae are commonly made up of ionized hydrogen gas that emits light as it recombines with electrons. This creates the vibrant pink and red colors often seen in these nebulae.
The two main types of bright nebulae are emission nebulae, which emit light from ionized gases, and reflection nebulae, which reflect light from nearby stars. Emission nebulae are usually red or pink in color, while reflection nebulae appear blue due to scattering of light.
Reflection nebulae reflect light from nearby stars, appearing blue due to scattering of light by interstellar dust. Emission nebulae emit light themselves, typically due to ionized gases within the nebula that are excited by nearby hot stars.
Emission nebulae appear red when they surround blue stars because the blue stars emit high-energy ultraviolet radiation which ionizes the hydrogen gas in the nebula, causing it to emit red light through a process called hydrogen-alpha emission. This red light is more prominent than the blue light emitted by the stars, giving the nebula its red color.
Dark reflecting nebulae appear dark because they are dense clouds of gas and dust blocking the light from stars behind them. Light reflecting nebulae, on the other hand, appear bright because they reflect the light of nearby stars, often due to the presence of reflective dust particles.
The most abundant gas in emission nebulae in the Milky Way is hydrogen. Emission nebulae are commonly made up of ionized hydrogen gas that emits light as it recombines with electrons. This creates the vibrant pink and red colors often seen in these nebulae.
Emission nebulae can emit photons of many wavelengths, but the predominant color is red. They can also emit blue and pink colors (which are also part of the Balmer series of the hydrogen atom).
There are mainly four types of nebulae: emission nebulae, reflection nebulae, dark nebulae, and planetary nebulae. Emission nebulae glow due to the energy emitted by nearby stars, reflection nebulae reflect light from nearby stars, dark nebulae are dense clouds that block light, and planetary nebulae are the remnants of dying stars. Each type of nebula differs in its composition, appearance, and the processes that create them.
There are several types of nebulae found in outer space, including emission nebulae, reflection nebulae, dark nebulae, and planetary nebulae. Emission nebulae are clouds of ionized gas that emit light, reflection nebulae reflect light from nearby stars, dark nebulae are dense clouds that block light, and planetary nebulae are the remnants of dying stars.
The emission spectrum of hydrogen primarily includes red, blue, and violet wavelengths of light. These correspond to specific transitions between energy levels in the hydrogen atom.
The common element with bright red, blue, green, and violet emission lines is hydrogen. These emission lines correspond to different electron transitions within the hydrogen atom, resulting in different colors of light being emitted.
Black because if a red light reflects off the blue surface there is no reflection, so the surface looks black.
Well you see color is just the rays from the sun reflecting a certain color and if its blue then its reflecting blue. but heres the tricky part since its just a reflection blue paint and red paint smell the same so the answer is blue paint.