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A gaseous substance exhibits a line spectrum, whereas a liquid or a solid substance exhibits a continuous spectrum. Give a qualitative explanation for these phenomena.

Short Answer

Expert verified
In summary, a gaseous substance exhibits a line spectrum because its isolated atoms or molecules possess clearly defined energy levels, leading to absorption or emission of radiation at specific wavelengths. In contrast, a liquid or solid substance exhibits a continuous spectrum due to the close proximity and interactions between atoms or molecules, causing a broadening and distribution of energy levels, resulting in a wide range of wavelengths being absorbed or emitted.

Step by step solution

01

Understanding the line spectrum of a gaseous substance

Gaseous substances are composed of individual atoms or molecules that are isolated from each other, allowing free movement throughout the gas. When electromagnetic radiation (such as light) interacts with these atoms or molecules, the electrons within the atoms can absorb energy and transition to higher energy levels. This absorption occurs at specific wavelengths corresponding to the energy difference between the initial and final energy levels of the electrons. As the electron transitions back to its ground state, it emits radiation at the same specific wavelengths. This results in the characteristic sharp and discrete lines observed in the emission or absorption spectra of gaseous substances, known as line spectra.
02

Understanding the continuous spectrum of a liquid or solid substance

In contrast to gaseous substances, the atoms or molecules in a liquid or solid substance are much closer together, resulting in various interactions between them. These interactions can cause the energy levels of the atoms or molecules to be influenced by their surrounding environment, leading to a distribution, or "smearing," of the energy levels. Additionally, vibrational and rotational energy states may also be populated, leading to even more possible energy transitions. Therefore, when electromagnetic radiation interacts with a liquid or solid substance, it can be absorbed or emitted at a wide range of wavelengths, creating a continuous spectrum.
03

Qualitative explanation

In summary, when a gaseous substance interacts with electromagnetic radiation, its isolated atoms or molecules possess clearly defined energy levels, leading to the absorption or emission of radiation at specific wavelengths, resulting in a line spectrum. However, in a liquid or solid substance, the close proximity and interactions between atoms or molecules cause a broadening and distribution of energy levels, which leads to a wide range of wavelengths being absorbed or emitted, creating a continuous spectrum.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Atomic Absorption and Emission
Exploring the interaction of light with atoms leads us into the fascinating world of atomic absorption and emission. As students of science, we recognize that each atom is a tiny universe of negatively charged electrons orbiting a nucleus of positively charged protons and neutral neutrons. The intriguing dance of electrons within their atomic realms is governed by quantum rules.

Now, when light waves, which are packets of energy known as photons, encounter these orbiting electrons, a very specific exchange occurs. If the energy of a photon matches the gap between two energy levels in an atom, the electron can absorb the photon, leap to a higher energy orbit – an excited state – and the atom becomes ‘excited’. The absorption of light at particular wavelengths is a clue we use to identify the presence of specific elements in a substance (like in stars or distant galaxies).

What rises must fall, and the excited electron soon yearns for the comfort of its ground state. As it returns, that exact amount of energy it absorbed is now released as a photon, leading to what we call emission. Different elements have unique energy gaps; hence, they absorb and emit light at different wavelengths. That’s why each element has its own 'fingerprint' of spectral lines, whether in the lab or in the vastness of space.
Energy Levels in Atoms
To understand how electrons behave, we need to delve into the concept of energy levels within atoms. Picture energy levels as steps on an invisible staircase within an atom. Electrons can only exist on these steps, not in between. These steps are like discrete energy zones, and electrons can move up or down these levels, but they can't just hang out on the staircase landing.

When it comes to atomic spectra, the position of these energy levels is crucial. Every time electrons transition between these levels, they must absorb or emit energy that precisely matches the difference between the steps. This is the cornerstone of why we see distinct lines in an atomic spectrum.

These energy levels are not haphazardly arranged; they are quantized and follow specific rules and limits set by the principles of quantum mechanics. This explains the distinctive lines in a spectrum, as electrons emit photons of very specific energies – it's like they are emitting notes on a music scale, where each note is tied to a specific jump between the energy levels.
Gaseous vs Solid State Spectroscopy
Spectroscopy, the study of the interaction between light and matter, wonderfully showcases the difference between gaseous and solid state substances. When we perform spectroscopy on gases, we mostly see atoms or molecules in the role of lone rangers. They roam freely, with their energy levels unperturbed by neighbors. This independence is why gases exhibit line spectra – those neat, sharp lines each representing a specific energy transition of an atom or molecule.

In contrast, solid-state spectroscopy is akin to observing a tightly knit crowd. Atoms and molecules are squeezed together in close quarters, constantly nudging and influencing each other. These interactions lead to a broadening of their energy levels, enabling continuous energy transitions over a range of wavelengths. This is why solids produce a continuous spectrum, with all colors blending together rather than showing distinct lines.

Differences Beyond the Phase

But there’s more to the story. Solids and liquids also have vibrational and rotational energy states, adding layers of complexity to their spectra. The combination of all these factors results in a rainbow of possibilities when light is absorbed or emitted – a stark contrast to the clear-cut line spectra of their gaseous counterparts.

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Most popular questions from this chapter

Wave number ( \(\mathrm{v}\) ) are the reciprocals of wavelengths, \(\lambda\) and are given by the expression \(\bar{v}=1 / \lambda\). For the hydrogen atom, the Bohr theory predicts that the wave number for the emission line associated with an electronic transition from the energy level having principal quantum number \(\mathrm{n}_{2}\) to that with principal quantum number \(\mathrm{n}_{1}\) is \(\bar{v}=R_{H}\left[\left(1 / n_{1}^{2}\right)-\left(1 / n_{2}^{2}\right)\right]\) where \(\mathrm{R}_{\mathrm{H}}\) is the Rydberg constant. In what region of the electromagnetic spectrum would there appear a spectral line resulting from the transition from the tenth to the fifth electronic level in hydrogen?

The sodium D-lines, two very distinct lines of yellow light emitted by heated sodium metal, are often used in the calibration of spectrometers. The wavelength of one of these lines is \(5890 \AA\). How much energy does an electron emit (or absorb) in undergoing the electronic transition associated with this line?

To measure the wavelength of lines in atomic emission and absorption spectra, one uses a spectroscope. Two lines in the yellow emission spectra of hot Na metal, the so-called sodium-D lines, are used to calibrate this instrument. If the wavelength of one of these lines is \(5890 \AA\), find the energy of the electronic transition associated with this line, \(\mathrm{h}=6.62 \times 10^{-27}\) erg-sec.

Show that in the Balmer series that the frequencies of successive lines tend toward a limiting value of \(\mathrm{cR} / 4\), where \(\mathrm{R}\) is the Rydberg constant and \(\mathrm{c}\) the speed of light.

The first two lines in the Lyman series for hydrogen are \(1215.56 \AA\) and \(1025.83 \AA\). These lines lie in the ultraviolet region of the spectrum. For each of these lines calculate the following: (a) the corresponding energy in ergs; (b) the corresponding energy in \(\mathrm{Kcal} / \mathrm{mole} ;\) (c) the frequency in \(\mathrm{sec}^{-1}\)

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