Recap 3-a


 

 

 

1.   An object that absorbs and re-emits all energy that hits it without any reflections is a

       __________________.

 

2. The blackbody radiation from a hot object is (bluer/redder) __________________. than the

      blackbody radiation from a cooler object.

 

3. The hotter the object, the _______________ the wavelength of the peak range of blackbody

      radiation emitted.

 

4. Planck’s Law states that the amount of energy carried by a photon is directly proportional to

       its ___________________.

 

5. The total amount of energy at all wavelengths emitted by a blackbody, per square meter per

      second, is proportional to the ____________ power of the its absolute temperature.

 

6. A plot of a brightness spectrum displays the brightness of radiation received from a source at

      various ______________ or ___________________.

 

7. Electromagnetic radiation from blackbodies, ionized gas, and line emissions from atoms and

      molecules can all be generated by ________________ mechanisms.

 

8. Hot, ionized gases are called ______________.

 

9. Wavelengths of 21.11 cm are associated with line emissions from ________________

       _______________.

 

10. Because blackbody curves do not cross, if you know the brightness of a blackbody at a given

      frequency, you also know its _________________.

 

1. blackbody 2. bluer 3. shorter 4 frequency 5. fourth 6. wavelengths, frequencies 7. thermal 8. plasmas 9. neutral hydrogen 10. temperature

 

 



Basics of Radio Astronomy