How Does Electron Transition Calculate Atomic Energy Levels and Ionization?

In summary: Regards,MarkIn summary, the conversation discusses the formula for calculating the energy needed to remove an electron from a hydrogen atom and the energy needed to remove one mole of electrons from one mole of hydrogen atoms. The formula is E = -2.178*10^-18 * Z^2/nhigh^2 - nlow^2, where Z is the atomic number, nhigh is infinity, and nlow is 1. The conversation also mentions using the formula to calculate the value of Z for an ion with a 2 to 1 transition associated with a wavelength of 13.4nm. However, there appears to be an error in the Z equation, which should be written as Z = sqrt(hc*(1/n
  • #1
StephenDoty
265
0
E of nlow to nhigh= -2.178*10^-18 * Z^2/nhigh^2 - nlow^2

find the energy needed to remove an electron completely from a hydrogen atom and the energy needed to remove one mol of electrons from one mol of hydrogen atoms

Z= 1 nhigh= infinity nlow=1

E = 2.178*10^-18 J
one mole of electrons = 2.178*10^-18 * 6.022*10^23 = 1.312*10^6 J/mol
Are these right??

And use the above formula to find the value of Z for an ion whose 2 to 1 transition is associated with a wavelength of 13.4nm.

lamba of 2 to 1= hc/(2.178*10^-18 * Z^2/nhigh^2 - nlow^2)
z=sqrt(hc(nhigh^2-nlow^2)/(13.4*10^-9)(2.178*10^-18))
Z= 4.5
or 5
Is this right??

Thank you guys so much for your help.
Stephen
 
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  • #2
StephenDoty said:
E of nlow to nhigh= -2.178*10^-18 * Z^2/nhigh^2 - nlow^2

Try to use TEX or at least brackets, it doesn't look OK at the moment.
 
  • #3
Hello Stephen,

Looks good on the single hydrogen atom and mole-of-hydrogen question.

But it looks like there's an error somewhere in the Z question. The correct answer is very close to an integer.

I think the problem is with the expressions you are writing. There should be a term

( 1/nhigh^2 - 1/nlow^2 )​

but instead you have

nhigh^2 - nlow^2​

?

Regards,

Mark

p.s. Borek is correct, it's better to at least use brackets (parantheses) to express things properly and avoid confusion.
 
  • #4
Z^2/nhigh^2 - nlow^2
is the same thing as z^2*(1/nhigh^2 - 1/nlow^2)
 
  • #5
Okay, but in your expression

z = sqrt(...)​

it has mysteriously become, literally,

(nhigh^2-nlow^2)​

and that is wrong.

Try keeping it as

(1/nhigh^2 - 1/nlow^2)​

Also, you might find it easier to figure out what the energy is for 13.4 nm, and then work with the energy equation (1st equation of your 1st post).
 

Related to How Does Electron Transition Calculate Atomic Energy Levels and Ionization?

1. What is an electron transition?

An electron transition is the movement of an electron from one energy level to another within an atom. This can happen when the electron absorbs or emits energy, causing it to change its orbit around the nucleus.

2. How is an electron transition related to light?

When an electron transitions between energy levels, it either absorbs or emits energy in the form of electromagnetic radiation, which includes light. This is because the energy levels in an atom are quantized, meaning they can only exist at specific values, and when an electron changes energy levels, it must either gain or lose energy in the form of light.

3. What is the significance of electron transitions?

Electron transitions are significant because they play a crucial role in many phenomena, such as the emission and absorption of light, chemical reactions, and the functioning of electronic devices. They also help scientists understand the structure and behavior of atoms and molecules.

4. How do electron transitions occur?

Electron transitions occur when an electron in an atom moves from a higher energy level to a lower energy level, releasing energy. This can happen spontaneously, or it can be induced by external factors such as light or collisions with other particles.

5. Can electron transitions be observed?

Yes, electron transitions can be observed using spectroscopy techniques, which involve shining light on a sample and analyzing the wavelengths of light that are absorbed or emitted. These observations can provide valuable information about the energy levels and structure of atoms and molecules.

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