Astronomers want to observe a star-forming region that is deeply embedded in a dense molecular cloud. Visible light cannot penetrate the dust. Which wavelength band is most useful?
AUltraviolet
BInfrared
CX-ray
DGamma-ray
Infrared radiation has longer wavelengths than visible light and is far less scattered by interstellar dust grains. It can penetrate dense dust clouds and reveal the young stars forming within. UV and X-rays have shorter wavelengths than visible light and are absorbed even more strongly by dust. Gamma rays are produced by the most extreme high-energy events, not by nascent star formation.
Question 2 True / False
Earth-based optical telescopes can observe most of the electromagnetic spectrum that reaches Earth's surface, including X-rays and gamma rays.
TTrue
FFalse
Answer: False
Earth's atmosphere is opaque to most non-visible wavelengths. X-rays and gamma rays are absorbed by the upper atmosphere (fortunately for life on Earth), and most ultraviolet is blocked by the ozone layer. Radio waves and some infrared do reach the ground, but most infrared is absorbed by water vapor. X-ray and gamma-ray observatories (like Chandra and Fermi) must be placed in orbit above the atmosphere.
Question 3 Short Answer
Why does the wavelength band used to observe an astronomical object depend on the object's temperature, and what law connects them?
Think about your answer, then reveal below.
Model answer: Wien's displacement law states that a blackbody's peak emission wavelength is inversely proportional to its temperature (λ_max = b/T). Hot objects like neutron star surfaces (millions of K) peak in X-rays; Sun-like stars peak in visible; cool dust and molecular clouds peak in infrared or radio.
This connects directly to blackbody radiation: every object emits a spectrum of radiation, and the peak wavelength shifts to shorter, higher-energy radiation as temperature increases. Knowing an object's likely temperature tells you which telescope to use — and conversely, the wavelength of peak emission tells you the object's temperature.