Based on what you’ve learned from the raisin cake analogy, which two properties of distant galaxies do astronomers have to measu
1 answer:
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Answer:
<h2>Explanation:
<u>Rule</u><u>:</u>
<h3>Speed= Distance/ Time</h3><em>Hope</em><em> </em><em>this</em><em> </em><em>helps</em><em>!</em><em> </em>
Answer:
This represents radiation in ultra-violet region .
Explanation:
Energy of the orbit where n = 3 is given as follows
= -1.511 eV
Energy of the orbit where n = 1 is given as follows
= 13.6 eV
Difference of [tex]E_3 and [tex]E_1 = - 1.511+ 13.6
= 12.089 eV.
The wavelength of light having this energy in nm is given by the expression as follows
Wavelength in nm = 1244 / energy in eV
= 1244 / 12.089
= 102.90 nm
This represents radiation in ultra-violet region .