The absorption spectra of ions have been used to identify the presence of the elements in...
The absorption spectra of ions have been used to identify the presence of the elements in the atmospheres of the sun and other stars. What is the energy of a photon (in J) that is absorbed by He+ ions, when an electron is excited from the Bohr orbit with n = 1 to the n = 4 state? The energy of an electron in the nth level is:
Homework Answers
En = -2.178*10^-18J*Z^2/n^2
Z = 2 for He^+
n = 1
E1 = -2.178*10^-18*(2)^2/(1)^2
E1 = -8.712*10^-18J
n = 4
E4 = -2.178*10^-18*(2)^2/(4)^2
E4 = -0.5445*10^-18J
E4-E1 = -0.5445*10^-18-( -8.712*10^-18)
= 8.1675*10^-18J >>>>answer
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The absorption spectra of ions have been used to identify the
presence of the elements in...
The absorption spectra of ions have been used to identify the presence of the elements in...
The absorption spectra of ions have been used to identify the presence of the elements in the atmospheres of the sun and other stars. What is the energy of a photon (in J) that is absorbed by He+ ions, when an electron is excited from the Bohr orbit with n = 1 to the n = 6 state? The energy of an electron in the nth level is? En= -BZ^2/N^2
Simplified. The absorption spectra of ions have been used to identify the presence of the elements...
Simplified. The absorption spectra of ions have been used to identify the presence of the elements in the atmospheres of the sun and other stars. What is the energy of a photon (in J) that is absorbed by He+ ions, when an electron is excited from the Bohr orbit with n = 1 to the n = 8 state? The energy of an electron in the nth level is - BZ2 En =- n? where B = 2.18 x 10-18...
Simplified. The absorption spectra of ions have been used to identify the presence of the elements...
Simplified. The absorption spectra of ions have been used to identify the presence of the elements in the atmospheres of the sun and other stars. What is the energy of a photon (in J) that is absorbed by He ions, when an electron is excited from the Bohr orbit with n = 1 to the n = 6 state? The energy of an electron in the nth level is 2 B2 2 where B = 2.18 x 10-1° J and...
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It is presented without derivation in Equntion 3.3 (3.3) ( )--(2. 178 x10-i, J)를 where n identifies the orbit whose energy is belng caleulated; 2 is the atonie number of the atom or on eketron ion: m, is the mi of the electron; ro is the vacuum permittivity: e is the charge on the electron; and h is Planck's constant....
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Simplified. The absorption spectra of ions have been used to identify the presence of the elements in the atmospheres of the sun and other stars. What is the energy of a photon (in J) that is absorbed by He+ ions, when an electron is excited from the Bohr orbit with n = 1 to the n = 8 state? The energy of an electron in the nth level is - BZ2 En =- n? where B = 2.18 x 10-18...
Simplified. The absorption spectra of ions have been used to identify the presence of the elements in the atmospheres of the sun and other stars. What is the energy of a photon (in J) that is absorbed by He ions, when an electron is excited from the Bohr orbit with n = 1 to the n = 6 state? The energy of an electron in the nth level is 2 B2 2 where B = 2.18 x 10-1° J and...
Laboratory questions: Atomic Emission Spectra This sheet has to be returned with your lab report and placed at the annex section A one electron excited ion (not hydrogen) absorbs a green photon: 2 - 542 nm. The electron, initially at the Bohr energy level n=8, moves to the level n = 14 after the photon absorption. Identify this ion (hint: find the Z value).
05 Question (4 points) When a hydrogen atom absorbs a photon of electromagnetic radiation (EMR), the internal energy of the atom increases and one or more electrons may be energized into an excited state. The release of this extra energy as the excited state electron transitions back to a lower energy state results in the emission of a photon. These energy changes are responsible for the emission spectrum of hydrogen (shown below) and are described by the Bohr equation. AE...
- Explain the trends in the magnitude of your errors for (a) the
H atom and (b) the He^+ ion.
It is presented without derivation in Equntion 3.3 (3.3) ( )--(2. 178 x10-i, J)를 where n identifies the orbit whose energy is belng caleulated; 2 is the atonie number of the atom or on eketron ion: m, is the mi of the electron; ro is the vacuum permittivity: e is the charge on the electron; and h is Planck's constant....
Problem Set 4 Atomic Structure and the Periodic Table Name: Date: Lab Section: General Instructions Complete the following problems. Attach another sheet to give yourself space for problems 8,9,10 as needed. Assignment is due at the end of the lab period unless stated otherwise by instructor. 1.) Energy Levels and Sublevels for the Polyelectronic Atom (a) How many sublevels exist in the energy level (n = 5)? (b) How many orbitals exist in any f-sublevel? (c) What is the maximum...
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