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Questions for Astronomy Physics Exam2

From Sergio <invalid@invalid.com>
Newsgroups sci.physics
Subject Questions for Astronomy Physics Exam2
Date 2016-07-22 21:08 -0500
Organization Aioe.org NNTP Server
Message-ID <nmujj8$2p7$2@gioia.aioe.org> (permalink)

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  answers should be easy for physics Dudes, answers can be found near 
published link

Astronomy I:  Practice Questions  for EXAM 2



   1. Which of the following types of electromagnetic radiation has

       a wavelength adjacent to but longer than visible light?

       a.  radio

       b.  infrared

       c.  X ray

       d.  ultraviolet

       e.  gamma ray



   2. The energy of a photon is

       a.  proportional to the wavelength and inversely proportional

           to the frequency.

       b.  proportional to the wavelength and proportional to the

           frequency.

       c.  inversely proportional to the wavelength and inversely

           proportional to the frequency.

       d.  inversely proportional to the wavelength and proportional

           to the frequency.



   3. Radio waves have

       a.  high energy and long wavelength.

       b.  low energy and long wavelength.

       c.  low energy and short wavelength.

       d.  high energy and short wavelength.



   4. If Star A is hotter than Star B, and Star A is emitting most

       of its light at a wavelength corresponding to yellow light,

       which of the following statements is true?

       a.  Star B will emit most of its light at a wavelength longer

           than yellow

       b.  Star B will emit most of its light at a wavelength shorter

           than yellow

       c.  Star B will emit most of its light at the same wavelength

           as Star A

       d.  more information is required to answer this question



   5. If two stars have the same surface area but one has 3 times

       the temperature of the other, how many times more energy is

       radiated by the more luminous star?

       a.  3

       b.  9

       c.  12

       d.  27

       e.  81



   6. Star A is radiating two times as much energy as Star B, but it

       is two times the distance from us. Which star will appear

       brighter, and by how much?

       a.  Star A will be 2 times brighter

       b.  Star B will be 2 times brighter

       c.  Star A will be 4 times brighter

       d.  Star B will be 4 times brighter

       e.  they will both have the same observed brightness





   7. Which one of the following types of spectrum always occurs

       with an absorption (dark line) spectrum?

       a.  bright line

       b.  emission line

       c.  continuous



   8. Spectral lines unique to each type of atom are caused by

       a.  each atom having a unique set of protons.

       b.  the unique sets of electron orbits.

       c.  the neutron-electron interaction being unique for each

           atom.

       d.  each type of photon emitted by the atom being unique.

       e.  none of the above; spectral lines are not unique to each

           type of atom.



   9. A star has an absorption spectrum showing many lines

       corresponding to silicon. Before it reaches an observer, the

       light from this star passes through a cool gas cloud

       containing a large amount of silicon. What will the observer

       detect?

       a.  an absorption spectrum with many silicon lines

       b.  an absorption and emission spectrum with lines

           corresponding to silicon

       c.  an emission spectrum of many silicon lines

       d.  a continuous spectrum



   10. Consider a cloud of (cool) gas between a star and an observer

       to be moving away from a source of continuous radiation (and

       towards the observer). Suppose the atoms in the gas have two

       energy levels separated by an energy corresponding to 5000 Angstroms.

       The observer will see a spectrum with absorption at a

       wavelength

       a.  less than 5000 Angstroms.

       b.  equal to 5000 Angstroms.

       c.  greater than 5000 Angstroms.

       d.  no absorption will take place.



   11. If an electron moves from a lower energy level to the next

       higher energy level, then

       a.  the atom has become excited.

       b.  the atom has become ionized.

       c.  the atom's light will be blue shifted.

       d.  the atom's light will be red shifted.



   12. The degree of ionization of an atom (i.e. the number of

       electrons lost) depends on

       a.  the level of the ground state.

       b.  the temperature of the gas.

       c.  the energy difference between the ground state and the

           first excited state.

       d.  the distance to the observer.



   13. Which of the following types of light can only be observed

       from space?

       a.  visible

       b.  radio

       c.  infrared

       d.  gamma ray



14. The greater the __________ the greater the light gathering
        power. (Pick the ONE most correct choice.)
                 a. objective focal length
                 b. resolution
                 c. objective thickness
                 d. objective area
                 e. magnification

15. The greater the __________ the greater the resolution of a
        telescope. (Pick the ONE most correct choice.)
                 a. objective focal length
                 b. eyepiece focal length
                 c. objective diameter
                 d. objective thickness
                 e. magnification

16. For which of the following types of telescopes is
       interferometry commonly used?
                 a. X-ray detector
                 b. ultraviolet telescope in orbit
                 c. visible telescope
                 d. multiple radio telescope dishes

17. If telescope A has a mirror twice the diameter of telescope B, the 
light gathering power of telescope A will be __________
        times that of B?
                 a. 2
                 b. 4
                 c. 8
                 d. 16

18. Which one of the following is a primary reason astronomers desire to 
have telescopes above the Earth's atmosphere?
                 a. the magnification will be improved
                 b. observations may be made in wavelengths that can not 
be seen from the surface of the Earth.
                 c. observations may be made in the radio region of the 
spectrum
                 d. the resolving power will be better in space because 
it no longer depends on the telescope diameter as is the case for
                      telescopes on the Earth's surface

19. Seeing refers to
                 a. the lack of clouds in the atmosphere.
                 b. how far a telescope can see.
                 c. the faintest object observable through a telescope.
                 d. the smearing of an image caused by atmospheric motions
                 e. the appearance of an image caused by the variation of
                      refraction with color

20.  Radio telescopes are large because of the small amount of energy 
carried by radio waves and
             a. because bigger is always better
             b. because the short wavelength radio waves already have 
such a high resolution
             c. because a bigger telescope is needed to increase the 
resolution with the long wavelength radio waves
             d. because they are cheap to construct





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Questions for Astronomy Physics Exam2 Sergio <invalid@invalid.com> - 2016-07-22 21:08 -0500
  Re: Questions for Astronomy Physics Exam2 benj <benj@nobody.net> - 2016-07-23 17:34 -0400
    Re: Questions for Astronomy Physics Exam2 Sergio <invalid@invalid.com> - 2016-07-23 17:59 -0500

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