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PRACTICE:Physics Unit33: Astrophysics and Cosmology



 Author: physics   Total Marks: 24 mks  Marks Awarded: _____________

User Name: No Login  Start Time: 23年05月02日 09:42  Switch to Whole-Paper Mode

Mark Problem
1#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The appearance of the gre2 ;+ cwmr9jcv ot1o 3:fie0dewat range of brightness among stars is due to

Correct Answer:    

Mark Problem
2#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The absolute luminosity for most stars depends on theva :kq k69ovxj-op82m

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Mark Problem
3#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  Four different main-sequence stars are colored blue, orange, red, and yellob1c x3 r73lhukw. What is their rank frorx1uk h3bl37 cm coolest to hottest?

Correct Answer:    

Mark Problem
4#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  A Hertzsprung-Russell diagram shows stars on a plot oxq n*ulk25 pn-f

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Mark Problem
5#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  A white dwarf star with a mass equal to that of the Sun is abjdop51k) m ms/out the size of

Correct Answer:    

Mark Problem
6#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The Chandrasekhar limit of stellar mass (below wczak+: 7.xm z obsdrxz4:ta3:hich a star will collapse into a white dwarf) is, if :x4mtza.+cr zxd obs3:: k za7the mass of our Sun is M, about

Correct Answer:    

Mark Problem
7#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  Supernovas are thought to always resulj; 5bxe/8ct ivt in

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Mark Problem
8#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  Black holes

Correct Answer:    

Mark Problem
9#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  Pulsars are rapidly spinn+y tap*zw1v( iing

Correct Answer:    

Mark Problem
10#
 
Free-Response ( 1.0 marks) Whole-Paper View Save Problem  
State Einstein's principle of equivalence.-6cktt fa cwt30gl ,/y
Correct Answer:    

Mark Problem
11#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The Schwarzschild radius of a black hole rp3t,zr)b7keasa)*fy-i ( xw is that radial distance from the center of a sphere within which not even light can escape. It was first discovered mathematically by Schwarzschild in 1916 after Einstein published his general relativity theory. It can be calculated from a st-)i3xarkf ps) za*(w7 ,yb retar's mass M as: $R = 2GM/c^2$. Take the radius of both stars A and B as the Schwarzschild radius. If the mass of star A is twice as much as the mass of star B, the average density of star A, compared to star B will be

Correct Answer:    

Mark Problem
12#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  When a distant source emits light of a particul8 w xc p88nadm;f.1krwar wavelength in the visible, and the source is moving away from us, the color of the light apca 88xm8w;fn.d1w rk ppears to us to be shifted toward the

Correct Answer:    

Mark Problem
13#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The cosmic background radiation corresponds to a temperature oa04 u ysdm7wqm+3v h2xf about

Correct Answer:    

Mark Problem
14#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The Sun has apparent brightness at Earth (6(zes/*m2j nb f6fijxg: e 4glf-tdw4$1.5 \times 10^{8} \; km$ away) of B. What would be the apparent brightness of the Sun at Pluto, which is $6.0 \times 10^{9} \; km$ from the Sun?

Correct Answer:    

Mark Problem
15#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  A star has absolute luminosity equal to that ofc2* gn v 8lb).qno eodc.r9ic. the Sun ($1.5 \times 10^{8} \; km$ from the Earth) but is 10 pc away from the Earth. By what factor will it appear dimmer than the Sun?

Correct Answer:    

Mark Problem
16#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The Earth's orbit has a mean rad1xneh m pexb/s-*q *r7 5xt,j1rve8odius of $1.5 \times 10^{8} \; km$. Over a six-month period, the apparent position of a particular star varies by $0.00014^{\circ}$ due to parallax. How distant is the star, in km?

Correct Answer:    

Mark Problem
17#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The Earth's orbit hatvcid-w4q*g kl0kjcb3+onu0 le4 :fh hw 21-ps a mean radius of $1.5 \times 10^{8} \; km$. Over a six-month period, the apparent position of a particular star varies by $0.00014^{\circ}$ due to parallax. How distant is the star, in ly? (1 ly = $9.46 \times 10^{15} \; m$)

Correct Answer:    

Mark Problem
18#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  What is the parallax angle for Proxima Centauri, which is Eau29ol9z a+q63umx8-gx mxfxorth's nearest star at 4.3 lyx 3uoml axx8x9-2 +zo9qgmf6u?

Correct Answer:    

Mark Problem
19#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  The apparent brightness of a star ir9 l;ql o4p e 6wks-)w;usle:ncn4be- s $1.0 \times 10^{-12} \; W/m^{2}$ and the peak wavelength is 600 nm. Estimate its distance from us.

Correct Answer:    

Mark Problem
20#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  It can be shown that the approximate age of the univb.d:ai a166zwrpykm7 dt+(c verse is 1/H, where H is the Hubble constant. Taking H ci pv6a(kmrdt 6adb17y:zw+ . = 20 km/s/Mly, estimate the age of the universe, in years.

Correct Answer:    

Mark Problem
21#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  If a galaxy is moving awayrxl.kwe y 8;o; from us at 1.0% of the speed of light, how far away is it from us?rk o.;l;w y8xe

Correct Answer:    

Mark Problem
22#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  Estimate the speed of a galaxy that is 10 billion light-year qr.xbzv o6(zh7k 0:svs away.

Correct Answer:    

Mark Problem
23#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  Estimate the observed wavelength for the 656 nm line in the spectr bt a tu7zmdy-2hxsmq (1t1;,ium of a star whichs ztu,12dy;txa7mbi- q 1mt(h is 100 million light-years from us.

Correct Answer:    

Mark Problem
24#
 
Single-Choice ( 1.0 marks) Whole-Paper View Save Problem  
  About 1 ms after the Big Bang, the temperxdtq3kq 0*-n iature of the universe was about 1013 K. Whakxti qdqn3-0 *t energy (in eV) does this correspond to?

Correct Answer:    

  • :
  • Total:24 mks Pass:14.4 mks Duration:Unlimited
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