TYPES OF NEBULAE By Raahil Ashraf VIII-A NEBULAE To start A nebula is a giant cloud of dust and gas in space. Some nebulae (more than one nebula) come from the gas and dust thrown out by the explosion of a dying star, such as a supernova. Other nebulae are regions where new stars are beginning to form. TYPES OF NEBULAE Planetary nebulae Nebulae are classified into one of two categories including extragalactic and galactic. Practically nothing is known about extragalactic nebulae, so the focus will be on galactic. Galactic nebulae can be further divided into either planetary or diffuse nebulae. Planetary (regular) nebulae have a distinct shape, where diffuse nebulae are irregular. Diffuse Nebulae are then broken down into dark and luminous. This sounds exactly like it is. Dark nebulae do not emit as much light as the luminous, so they appear as dark, irregular blotches in the sky. Luminous nebulae can either be emission or reflection types. Emission can then be categorized as supernova remnants or H II regions. PLANETARY NEBULAE When a star dies, it doesn't explode into a supernova or collapse into a black hole. Instead, it gently sheds its outer layers, which form a beautiful cloud called a “planetary nebula”, while the dying star's core becomes a white dwarf. DIFFUSE NEBULAE Diffuse nebulae are named for their widespread, fairly thin regions of gas and dust. Diffuse nebulae, like the Orion Nebula, can be regions of star formations if they are large enough. Once all the gas and ions have been used in a diffuse nebula, a group of young, hot stars remains in an open star cluster. Diffuse nebula can be classified as dark or luminous. DARK NEBULAE Dark nebulae are dense regions in space that do not emit light. They look like big black opaque splotches surrounded by the starry night. Dark Nebulae are so dense with dust and particles that no light passes through them. They tend to have irregular shapes, with no definable outer edges. These vast clouds are mostly composed of molecular hydrogen. LUMINOUS NEBULAE Luminous nebulae are made bright by radiation from stars in the vicinity. REFLECTION NEBULAE Reflection nebula are clouds of interstellar dust which might reflect the light of a nearby star or stars. The energy from the nearby stars is insufficient to ionize the gas of the nebula to create an emission nebula, but is enough to give sufficient scattering to make the dust visible. EMISSION NEBULAE An emission nebula is a cloud of high temperature gas. Within this type of nebula, a star energizes the atoms in the cloud with ultraviolet radiation. The process is similar to that of a neon light. This causes the nebula to glow. SUPERNOVA NEBULAE When the pressure drops low enough in a massive star, gravity suddenly takes over and the star collapses in just seconds. This collapse produces the explosion we call a supernova. Supernovae are so powerful they create new atomic nuclei. HII REGIONS NEBULAE HII regions are emission nebulae created when young, massive stars ionise nearby gas clouds with high-energy UV radiation. THANK YOU For listening and reading