What is the predominant atomic or molecular mechanism that produces the light we see from emission nebulae?
A) Radio energy from embedded stars excites atoms to high atomic states, and spectral lines are produced as these atoms return to their unexcited states.
B) Radiation from nearby stars heats the gas, and the gas then emits a continuum spectrum appropriate to its temperature.
C) Photons of UV and X radiation from very hot embedded stars accelerate electrons by collision, and these accelerating electrons radiate at all wavelengths.
D) UV light from hot stars ionizes atoms, and the subsequent recombination of electrons with these ions produces spectral lines.
Correct Answer:
Verified
Q6: We see an emission nebula predominantly in:
A)blue
Q7: Hot O and B stars embedded in
Q8: The predominant color of an emission nebula
Q9: What is the characteristic color of an
Q10: What is the dominant spectral emission line
Q12: What process makes an emission nebula glow?
A)electric
Q13: What causes the characteristic red color of
Q14: A large emission nebula contains about how
Q15: A small emission nebula contains about how
Q16: Long-exposure color photographs of the night sky
Unlock this Answer For Free Now!
View this answer and more for free by performing one of the following actions
Scan the QR code to install the App and get 2 free unlocks
Unlock quizzes for free by uploading documents