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Wednesday, December 14, 2011

Astronomy

1.

Quiz2 - Q1

 
The Sun is a fairly normal star.
Student ResponseValueCorrect Answer
True100%True
Score:5/5
 

2.

Quiz2 - Q2

 
At very large distances from the Sun, its corona turns into the solar wind.
Student ResponseValueCorrect Answer
True100%True
Score:5/5
 

3.

Quiz2 - Q3

 
The Sun's density is about the same as Saturn's.
Student ResponseValueCorrect Answer
True0%False
Score:0/5
 

4.

Quiz2 - Q4

 
The energy of the Sun starts as radiation, but is actually transported to its surface by convection, where it is radiated off into space at last.
Student ResponseValueCorrect Answer
True100%True
Score:5/5
 

5.

Quiz2 - Q5

 
The light we see from the Sun comes from which layer?
 Student ResponseValueCorrect AnswerFeedback
troposphere  
chromosphere  
ionosphere  
Student Response photosphere100%Student Response   
corona  
Score:5/5
 

6.

Quiz2 - Q6

 
How many planet Earths could fit inside the Sun?
 Student ResponseValueCorrect AnswerFeedback
110  
1000  
Student Response a little over a million100%Student Response   
ten billion  
ten trillion  
Score:5/5
 

7.

Quiz2 - Q7

 
From inside out, which is in the correct order for the structure of the Sun?
 Student ResponseValueCorrect AnswerFeedback
core, convective zone, radiative zone  
Student Response photosphere, radiative zone, corona0%  
radiative zone, convective zone, chromosphereStudent Response   
core, chromosphere, photosphere  
convective zone, radiative zone, granulation  
Score:0/5
 

8.

Quiz2 - Q8

 
The vibrations of the Sun reveal information about
 Student ResponseValueCorrect AnswerFeedback
the temperature of the core of the Sun.  
the structure of the atmosphere of the Sun.  
the production of energy in the Sun.  
Student Response the interior structure of the Sun.100%Student Response   
the magnetic field of the Sun.  
Score:5/5
 

9.

Quiz2 - Q9

 
The outward pressure of hot gas in the Sun
 Student ResponseValueCorrect AnswerFeedback
Student Response is balanced by the inward gravitational pressure.100%Student Response   
is increasing the Sun's diameter.  
is cooling the photosphere.  
is responsible for variations in the sunspot cycle.  
weakens the magnetic field.  
Score:5/5
 

10.

Quiz2 - Q10

 
Which is the net result of the proton-proton chain?

 Student ResponseValueCorrect AnswerFeedback
Student Response 4 protons = 1 helium 4 + a positron + a neutrino + gamma rays0%  
2 protons = deuterium + a positron + an antineutrino + X-rays  
4 protons = 2 helium 2 + 2 positrons + ultraviolet radiation  
4 protons = 1 helium 4 + 2 neutrinos + gamma raysStudent Response   
6 protons = 2 heliums + 3 positrons + 3 neutrinos + gamma rays  
Score:0/5
 

11.

Quiz2 - Q11

 
Which of these are not associated with the active Sun?
 Student ResponseValueCorrect AnswerFeedback
sunspots  
prominences  
Student Response granulation100%Student Response   
flares  
aurora  
Score:5/5
 

12.

Quiz2 - Q12

 
Suppose a large flare is detected optically. How long until radio interference arrives?
 Student ResponseValueCorrect AnswerFeedback
Student Response simultaneously100%Student Response   
8.5 minutes later  
12 hours later  
no relation between the arrival time  
6 days later  
Score:5/5
 

13.

Quiz2 - Q13

 
We know the Sun rotates differentially by observing sunspots; as with Jupiter the solar equator rotates the fastest.
Student ResponseValueCorrect Answer
True100%True
Score:5/5
 

14.

Quiz2 - Q14

 
The proton-proton chain requires a temperature of 100 million K to get started.
Student ResponseValueCorrect Answer
True0%False
Score:0/5
 

15.

Quiz2 - Q15

 
The solar constant is a measure of
 Student ResponseValueCorrect AnswerFeedback
the energy received by the Sun on Earth's surface.  
Student Response the energy received by the Sun at the location of Earth.100%Student Response   
the energy received by the Sun at any location in the solar system.  
the energy emitted by the Sun at the photosphere.  
the total energy emitted by the Sun in all directions.  
Score:5/5
 

16.

Quiz2 - Q16

 
The luminosity of the Sun is a measure of 
 Student ResponseValueCorrect AnswerFeedback
the energy received by the Sun on Earth's surface.  
the energy received by the Sun at the location of Earth.  
the energy received by the Sun at any location in the solar system.  
the energy emitted by the Sun at the photosphere.  
Student Response the total energy emitted by the Sun in all directions.100%Student Response   
Score:5/5
 

17.

Quiz2 - Q17

 
The above diagram indicates that
tvsD sun.jpg
 Student ResponseValueCorrect AnswerFeedback
the Sun is hottest somewhere between its surface and its core.Student Response   
the Sun is coolest somewhere between its surface and its core.  
the Sun is hotter at its surface than at its core.  
Student Response the Sun is hotter at its core than at its surface.0%  
the Sun has about the same temperature throughout its interior.  
Score:0/5
 

18.

Quiz2 - Q18

 
What two energy transport mechanisms, in order from outside the core to the surface, is found in the Sun? 
 Student ResponseValueCorrect AnswerFeedback
convection, conduction  
Student Response radiative diffusion, convection100%Student Response   
conduction, radiative diffusion  
radiative diffusion, conduction  
conduction, convection  
Score:5/5
 

19.

Quiz2 - Q19

 
From where does most of the solar wind flow?
 Student ResponseValueCorrect AnswerFeedback
granules  
sunspots  
Student Response flares0%  
prominences  
coronal holesStudent Response   
Score:0/5
 

20.

Quiz2 - Q20

 
The numbers of sunspots and their activity peak about every:
 Student ResponseValueCorrect AnswerFeedback
36 days  
6 months  
1 year  
Student Response 11 years100%Student Response   
79 years  
Score:5/5

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