The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol should be calculated using the concept of Bohr’s theory. Concept Introduction: The emission of radiation given by an energized hydrogen atom to the electron falling from a higher-energy orbit to a lower orbit give a quantum of energy in the form of light. Based on electrostatic interaction and law of motion, Bohr derived the following equation. E n = − 2 .18 × 10 − 18 J ( 1 n 2 ) where n gets an integer values such as n = 1, 2, 3 and so on. This is the energy of electron in n th orbital. The electrons are excited thermally when the light is used by an object. As a result, an emission spectrum comes. Line spectra consist of light only at specific, discrete wavelengths. In emission, the electron returns to a lower energy state from n f (the i and f subscripts denote the initial and final energy states). In most cases, the lower energy state corresponds to the ground state but it may be any energy state which is lower than the initial excited state. The difference in the energies between the initial and final states is ΔE = E f − E i This transition results in the photon’s emission with frequency v and energy hv . The following equation is resulted. ΔE = hν = − 2 .18 × 10 − 18 J ( 1 n f 2 − 1 n i 2 ) When n i > n f , a photon is emitted. The term in parentheses is positive, making ΔE negative . As a result, energy is lost to the surroundings. When n i < n f , a photon is absorbed. The term in parentheses is negative, so ΔE is positive. As a result, energy is absorbed from the surroundings. To find: The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol
The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol should be calculated using the concept of Bohr’s theory. Concept Introduction: The emission of radiation given by an energized hydrogen atom to the electron falling from a higher-energy orbit to a lower orbit give a quantum of energy in the form of light. Based on electrostatic interaction and law of motion, Bohr derived the following equation. E n = − 2 .18 × 10 − 18 J ( 1 n 2 ) where n gets an integer values such as n = 1, 2, 3 and so on. This is the energy of electron in n th orbital. The electrons are excited thermally when the light is used by an object. As a result, an emission spectrum comes. Line spectra consist of light only at specific, discrete wavelengths. In emission, the electron returns to a lower energy state from n f (the i and f subscripts denote the initial and final energy states). In most cases, the lower energy state corresponds to the ground state but it may be any energy state which is lower than the initial excited state. The difference in the energies between the initial and final states is ΔE = E f − E i This transition results in the photon’s emission with frequency v and energy hv . The following equation is resulted. ΔE = hν = − 2 .18 × 10 − 18 J ( 1 n f 2 − 1 n i 2 ) When n i > n f , a photon is emitted. The term in parentheses is positive, making ΔE negative . As a result, energy is lost to the surroundings. When n i < n f , a photon is absorbed. The term in parentheses is negative, so ΔE is positive. As a result, energy is absorbed from the surroundings. To find: The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol
Solution Summary: The author explains that the wavelength of light emitted in a transition from the first excited state to the ground state should be calculated using the concept of Bohr's theory.
The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol should be calculated using the concept of Bohr’s theory.
Concept Introduction:
The emission of radiation given by an energized hydrogen atom to the electron falling from a higher-energy orbit to a lower orbit give a quantum of energy in the form of light. Based on electrostatic interaction and law of motion, Bohr derived the following equation.
En=−2.18 × 10−18 J (1n2)
where n gets an integer values such as n = 1, 2, 3 and so on. This is the energy of electron in nth orbital.
The electrons are excited thermally when the light is used by an object. As a result, an emission spectrum comes. Line spectra consist of light only at specific, discrete wavelengths. In emission, the electron returns to a lower energy state from nf (the i and f subscripts denote the initial and final energy states). In most cases, the lower energy state corresponds to the ground state but it may be any energy state which is lower than the initial excited state. The difference in the energies between the initial and final states is
ΔE = Ef− Ei
This transition results in the photon’s emission with frequency v and energy hv. The following equation is resulted.
ΔE = hν =−2.18 × 10−18 J (1nf2−1ni2)
When ni > nf, a photon is emitted. The term in parentheses is positive, making ΔE negative. As a result, energy is lost to the surroundings. When ni < nf, a photon is absorbed. The term in parentheses is negative, so ΔE is positive. As a result, energy is absorbed from the surroundings.
To find: The wavelength of light emitted in a transition from the first excited state in which the ionization energy is 126 kJ/mol to the ground state in which the ionization energy is 412 kJ/mol
5. Compressibility (6 points total). The isothermal compressibility is a measure of how
hard/easy it is to compress an object (how squishy is it?) at constant temperature. It is
др
defined as Br=-()=-(200²)T'
(a) You might wonder why there is a negative sign in this formula. What does it mean when
this quantity is positive and what does it mean when this quantity is negative?
(b) Derive the formula for the isothermal compressibility of an ideal gas (it is very simple!)
(c) Explain under what conditions for the ideal gas the compressibility is higher or lower,
and why that makes sense.
19. (3 pts) in Chapter 7 we will see a reaction of halocyclohexanes that requires that the halogen occupy an axial position with
this in mind, would you expect cis-1-bromo-3-methylcyclohexane or trans-1-bromo-3-methylcyclohexane to be more
reactive in this reaction? Briefly explain your choice using structures to support your answer.
Mere-eries-cecleone)
The tran-i-browse-3-methylcyclohexione
Please help me calculate the undiluted samples ppm concentration.
My calculations were 280.11 ppm. Please see if I did my math correctly using the following standard curve.
Link: https://mnscu-my.sharepoint.com/:x:/g/personal/vi2163ss_go_minnstate_edu/EVSJL_W0qrxMkUjK2J3xMUEBHDu0UM1vPKQ-bc9HTcYXDQ?e=hVuPC4
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, chemistry and related others by exploring similar questions and additional content below.
Author:Steven D. Gammon, Ebbing, Darrell Ebbing, Steven D., Darrell; Gammon, Darrell Ebbing; Steven D. Gammon, Darrell D.; Gammon, Ebbing; Steven D. Gammon; Darrell
Author:Steven D. Gammon, Ebbing, Darrell Ebbing, Steven D., Darrell; Gammon, Darrell Ebbing; Steven D. Gammon, Darrell D.; Gammon, Ebbing; Steven D. Gammon; Darrell
Quantum Numbers, Atomic Orbitals, and Electron Configurations; Author: Professor Dave Explains;https://www.youtube.com/watch?v=Aoi4j8es4gQ;License: Standard YouTube License, CC-BY