qu.1.topic=fill in blanks@ qu.1.1.mode=Blanks@ qu.1.1.name=StellarParameters-2@ qu.1.1.editing=useHTML@ qu.1.1.question=
Astronomers learn about the surface tempertures of stars from their <1> spectra. They look at the particular spectral lines present and their relative strengths and assign the star a spectral type. The spectral sequence is 0, B, <2>, F, G, <3>, M. A very hot blue star could have a spectral type of <4>. The spectral type of the sun is <5>. A star with a surface temperature of 3000 K could have a spectral type of <6>.
Spectal type information could appear on the <7> of the HR Diagram with the O stars on the far <8>. The other axis contains information on the intrinsic energy production of the star in the form of luminosity or absolute magnitude. Very large stars could be found on the <9> of the HR Diagam. This diagram will be very important for discussing how stars change throughout their lives which will be represented as a path on the HR Diagram.
@ qu.1.1.blank.1=absorption, emission, continuous, blackbody@ qu.1.1.blank.2=A,K,X,P@ qu.1.1.blank.3=K,A,P,X@ qu.1.1.blank.4=O2, A5, F5, K1, M3@ qu.1.1.blank.5=G2, F5, K1, M3, A5@ qu.1.1.blank.6=M3, G2, F5, B1, A5@ qu.1.1.blank.7=x-axis, y-axis@ qu.1.1.blank.8=left, right@ qu.1.1.blank.9=upper right, lower right, upper left, lower left@ qu.1.1.grader.1=menu@ qu.1.1.grader.2=menu@ qu.1.1.grader.3=menu@ qu.1.1.grader.4=menu@ qu.1.1.grader.5=menu@ qu.1.1.grader.6=menu@ qu.1.1.grader.7=menu@ qu.1.1.grader.8=menu@ qu.1.1.grader.9=menu@ qu.1.2.mode=Blanks@ qu.1.2.name=StellarParameters-2@ qu.1.2.editing=useHTML@ qu.1.2.question=Astronomers learn about the surface tempertures of stars from their <1> spectra. They look at the particular spectral lines present and their relative strengths and assign the star a spectral type. The spectral sequence is 0, <2>, A, F, <3>, K, M. A very cool red star could have a spectral type of <4>. A star with a surface temperature of over 30000 K could have a spectral type of <5>. The spectral type of the sun is <6>.
Spectal type information could appear on the <7> of the HR Diagram with the M stars on the far <8>. The other axis contains information on the intrinsic energy production of the star in the form of luminosity or absolute magnitude. Very small stars could be found on the <9> of the HR Diagam. This diagram will be very important for discussing how stars change throughout their lives which will be represented as a path on the HR Diagram.
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