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How does atomic spectrum differ from solar spectrum?
Atomic spectrum is produced when atoms emit or absorb light at specific energies, creating distinct lines or bands. Solar spectrum is the continuous spectrum of light emitted by the Sun, containing all wavelengths of light. Solar spectrum is produced by many elements and compounds in the Sun's atmosphere, creating a broad, continuous range of colors.
What are the characteristics of the nitrogen spectrum?
The nitrogen spectrum consists of lines that are mainly in the ultraviolet region of the electromagnetic spectrum. These lines are produced when nitrogen atoms are excited and emit light. The spectrum is characterized by distinct lines at specific wavelengths, which can be used to identify nitrogen in various substances.
Is an atomic emission spectrum a continuous range of colors?
No, an atomic emission spectrum is not a continuous range of colors. It consists of discrete lines of specific wavelengths corresponding to the emission of light from excited atoms when they return to lower energy levels. Each element has a unique atomic emission spectrum due to its unique arrangement of electrons.
What are the characteristics of the nitrogen emission spectrum?
The nitrogen emission spectrum is characterized by a series of distinct lines of light that are emitted when nitrogen atoms are excited. These lines are specific to the energy levels of nitrogen atoms and can be used to identify the presence of nitrogen in a sample.
Which type of spectrum is produced when white light from the Sun passes through a prism?
A continuous spectrum is produced when white light from the Sun passes through a prism. This spectrum contains all the colors of the rainbow without any distinct lines or bands.
How does atomic spectrum differ from solar spectrum?
Atomic spectrum is produced when atoms emit or absorb light at specific energies, creating distinct lines or bands. Solar spectrum is the continuous spectrum of light emitted by the Sun, containing all wavelengths of light. Solar spectrum is produced by many elements and compounds in the Sun's atmosphere, creating a broad, continuous range of colors.
What type of spectrum is produced when the light emitted directly from a hot dense object passes through a prism?
A continuous spectrum is produced when light emitted directly from a hot dense object passes through a prism. This spectrum shows a rainbow of colors with no distinct lines, indicating that all wavelengths of light are present. This type of spectrum is characteristic of a blackbody radiation emission.
What are the characteristics of the nitrogen spectrum?
The nitrogen spectrum consists of lines that are mainly in the ultraviolet region of the electromagnetic spectrum. These lines are produced when nitrogen atoms are excited and emit light. The spectrum is characterized by distinct lines at specific wavelengths, which can be used to identify nitrogen in various substances.
What do you call a light spectrum that is not continuous?
A light spectrum that is not continuous is called a discrete or discontinuous spectrum. This means that instead of a smooth progression of colors, there are distinct individual colors or wavelengths present in the spectrum.
What is the difference between the spectrum of the light bulb and the spectra of gas tubes?
The spectrum of a light bulb is continuous, meaning it covers a broad range of wavelengths with no distinct lines. Gas tubes emit light at specific wavelengths called emission lines, producing a line spectrum with discrete colored lines. This difference is due to the way light is generated in each source.
Is an atomic emission spectrum a continuous range of colors?
No, an atomic emission spectrum is not a continuous range of colors. It consists of discrete lines of specific wavelengths corresponding to the emission of light from excited atoms when they return to lower energy levels. Each element has a unique atomic emission spectrum due to its unique arrangement of electrons.
The lines in the bright line spectrum of an atom are due to what?
The atomic line spectrum comes from the emission of atoms of different elements that are in an excited state. Each element has its own unique atomic emission spectrum.
How does the spectrum of helium differ from the spectrum of white light from the Sun?
The spectrum of helium consists of distinct lines at specific wavelengths, known as emission lines, due to the transition of electrons between energy levels. In contrast, the spectrum of white light from the Sun is continuous, with all visible wavelengths present. The presence of absorption lines in the solar spectrum, caused by elements in the Sun's atmosphere absorbing specific wavelengths, further distinguishes it from the discrete emission lines of helium.
How does the color of the flame correspond to the distinct lines in its spectrum?
The color in the flame is the representation of a specific line in the spectrum.
What are the characteristics of the nitrogen emission spectrum?
The nitrogen emission spectrum is characterized by a series of distinct lines of light that are emitted when nitrogen atoms are excited. These lines are specific to the energy levels of nitrogen atoms and can be used to identify the presence of nitrogen in a sample.
Which type of spectrum is produced when white light from the Sun passes through a prism?
A continuous spectrum is produced when white light from the Sun passes through a prism. This spectrum contains all the colors of the rainbow without any distinct lines or bands.
What you observe if light from argon gas were passed through a prism?
If light from argon gas were passed through a prism, you would observe it splitting into its different wavelengths or colors, creating a spectrum. The spectrum produced would consist of a few distinct lines corresponding to the specific wavelengths of light emitted by the excited argon atoms. This pattern of lines is known as an emission spectrum and can be used to identify the presence of argon gas.
