Light behaves as both waves and particles called photons. Is this statement true or false?
02 Observing the Universe Online Quiz Questions
Use this free practice quiz with 20 questions to review 02 Observing the Universe, test your knowledge, and prepare for your next test or exam.
As the wavelength of light decreases, what happens to its frequency and the energy of its photons?
- A
Both frequency and photon energy decrease.
- B
Both frequency and photon energy increase.
- C
Frequency increases, but photon energy decreases.
- D
Frequency decreases, but photon energy increases.
Observing an astronomical object in just one wavelength band is enough to give a complete picture of it. Is this statement true or false?
- A
True
- B
False
How does a charge-coupled device (CCD) turn incoming light into digital measurements?
- A
The sensor directs photons to a prism, which stores them as a spectrum.
- B
The sensor records the source’s brightness as a sound signal.
- C
Incoming photons create electrical charges that are read and converted into digital measurements.
- D
The sensor focuses all wavelengths onto one pixel and records their temperature.
A spectrum with dark lines where material between the source and observer has absorbed light is an spectrum.
Which conclusions can astronomers draw from spectra? Select all correct choices.
- A
Characteristic spectral lines can help identify chemical composition.
- B
The overall spectrum can provide clues to temperature and physical conditions.
- C
Shifts in spectral lines can reveal motion along the line of sight.
- D
A spectrum directly gives the object's distance without any other evidence.
For observations at the same wavelength, what is a general benefit of using a telescope with a larger aperture?
- A
It captures fewer photons and generally lowers angular resolution.
- B
It captures more photons and generally improves angular resolution.
- C
It captures more photons but necessarily lowers angular resolution.
- D
It affects the amount of light collected but has no effect on angular resolution.
What instrument separates incoming light into a spectrum and records the result with a detector?
Most visible light and some reach the ground; many ultraviolet, X-ray, and gamma-ray wavelengths do not.
Which statements correctly describe information that different wavelength bands can reveal? Select all correct choices.
- A
Infrared can reveal relatively cool objects and radiation from dust.
- B
Ultraviolet can trace hot stars and gas.
- C
X-rays often reveal extremely hot gas.
- D
Visible light always reveals every region obscured by dust.
What is the name for a record showing how an astronomical source's brightness changes over time?
Why might astronomers place an observatory in space or at a high altitude, and how can combining visible-light and infrared observations of the same nebula provide a fuller picture?
What is a key limitation of combining separated telescopes through interferometry?
- A
It provides the same collecting area as a single dish spanning the separation between telescopes.
- B
It can improve resolution, but does not provide the collecting area of one dish spanning the separation.
- C
It increases collecting area but cannot improve resolution.
- D
It only works for visible light and always requires a single telescope.
Ordinary mirrors are generally used to focus gamma rays in the same way that mirrors focus visible light. Is this statement true or false?
- A
True
- B
False
A visible-light image of a nebula shows stars and glowing gas, but a dusty region is difficult to see. Which wavelength band would best help reveal cooler material and regions obscured by dust?
- A
Ultraviolet
- B
Infrared
- C
X-ray
- D
Gamma-ray
A spectrum contains dark lines at particular wavelengths against a brighter background. What most directly explains those lines?
- A
Atoms or molecules in the source emitted light at those wavelengths.
- B
The source produced a continuous spectrum with no interaction along the line of sight.
- C
Material between the source and observer absorbed light at those wavelengths.
- D
The detector converted those wavelengths into electrical charges.
A telescope camera uses a charge-coupled device (CCD). Which sequence best describes how the CCD turns incoming visible light into image data?
- A
Photons create electrical charges in pixels, which electronics read as digital measurements.
- B
Photons are stored unchanged in the pixels until the image is viewed.
- C
The sensor separates light into spectral lines before measuring it.
- D
The pixels focus incoming light onto the telescope aperture.
An astronomer needs to observe X-rays from a distant source. Where should the telescope be placed to avoid the atmosphere blocking most of the incoming X-rays?
- A
Place the telescope at a high mountain observatory because all X-rays pass through the atmosphere there.
- B
Use a ground-based optical telescope, since mirrors focus X-rays like visible light.
- C
Place the telescope underwater to reduce atmospheric absorption.
- D
Place the telescope in space, above most of the atmosphere.
What is the name for coordinated observations of the same astronomical object in different wavelength bands?
For ideal circular apertures, the diffraction limit is θ≈1.22λ/D. Telescope B observes at three times the wavelength and has twice the aperture diameter of telescope A. What is the ratio θB/θA?