What specific hot object illuminates the ejected shell gas of a planetary nebula?
Answer
The exposed, hot core collapsing into a white dwarf star left behind after the star sheds its outer layers.
Planetary nebulae are formed during the late stages of life for stars similar in mass to the Sun. When the star exhausts its fuel, it expels its outer layers of gas into space. The remaining stellar core contracts intensely, becoming incredibly hot and small—a white dwarf. This exposed white dwarf radiates prodigious amounts of ultraviolet radiation due to its extreme temperature, sometimes exceeding one hundred thousand degrees Celsius. This intense radiation acts as an internal light source, exciting and illuminating the surrounding shell of previously ejected gas, causing the expanding material to glow brightly.

Related Questions
What process involving high-energy ultraviolet radiation makes an emission nebula glow?Why do reflection nebulae often appear distinctly blue to observers or telescopes?How do dark nebulae reveal themselves against a bright background?What are nebulae fundamentally composed of primarily?What specific hot object illuminates the ejected shell gas of a planetary nebula?What distinguishes the visibility mechanism of an emission nebula from a reflection nebula?What element causes the characteristic reddish hue seen in the Orion Nebula?How does long-exposure astrophotography reveal faint emission nebulae structures?Besides the efficiency of interaction, what determines a nebula's perceived brightness?Why might a dark nebula become almost invisible if viewed against the emptiness of deep space?