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The low-pressure sodium arc discharge lamp was first made practical around 1920 owing to the development of a type of glass that could resist the corrosive effects of sodium vapor. These operated at pressures of less than 1 Pa and produced a near monochromatic light spectrum around the sodium emission lines at 589.0 and 589.56 nanometres ...
the spectrum of light coming from a star with hot dense surface and no low density atmosphere would be which type contunuous upper spectrum on the diagram is spectrum #2
When the light emitted from a source is made to pass through an absorbing material and then examined with a spectrometer, the obtained spectrum is called absorption spectrum. It is the characteristic of the absorbing substance. Absorption spectra is also of three types . 1. continuous absorption spectrum . 2. line absorption spectrum and . 3.
For the Sun, the wavelength at which the maximum energy is emitted is 520 nanometers, which is near the middle of that portion of the electromagnetic spectrum called visible light. Characteristic temperatures of other astronomical objects, and the wavelengths at which they emit most of their power, are listed in Table 5.1.
A Growlight is a special type of light bulb that is used in horticulture. it tries to mimic the light spectrum produced by the sun - as normal light bulbs (incandescent and fluorescent) do not ...
The emission spectrum of a chemical element or chemical compound is the spectrum of frequencies of electromagnetic radiation emitted due to an atom or molecule making a transition from a high energy state to a lower energy state. The photon energy of the emitted photon is equal to the energy difference between the two states. There are many ... See full list on imagine.gsfc.nasa.gov
Emission spectra observed directly from hot, low-density gas. Absorption Line Spectrum:The opposite of emission lines, absorption spectra are often due to cooler gas absorbing photons emitted from a hot source. An absorption line spectrum appears to be a continuum spectrum with emission lines taken out.
A hot, dense gas produces a(n) _____ spectrum, with energy emitted at every wavelength. continuous The upward Lyman series transitions in hydrogen begin with electrons in the ground state (n=1), which is the state of most hydrogen atoms.

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spectrum produced when the light emitted directly from a hot, dense object passes through a prism Emission Spectrum spectrum produced when the light emitted directly form a hot, low-density cloud of gas passes through a prism A Growlight is a special type of light bulb that is used in horticulture. it tries to mimic the light spectrum produced by the sun - as normal light bulbs (incandescent and fluorescent) do not ...
By definition, visible light is the part of the EM spectrum the human eye is the most sensitive to. Visible light (and near-infrared light) is typically absorbed and emitted by electrons in molecules and atoms that move from one energy level to another. This action allows the chemical mechanisms that underlie human vision and plant photosynthesis. The emission spectrum of a chemical element or chemical compound is the spectrum of frequencies of electromagnetic radiation emitted due to an atom or molecule making a transition from a high energy state to a lower energy state. The photon energy of the emitted photon is equal to the energy difference between the two states. There are many ... By definition, visible light is the part of the EM spectrum the human eye is the most sensitive to. Visible light (and near-infrared light) is typically absorbed and emitted by electrons in molecules and atoms that move from one energy level to another. This action allows the chemical mechanisms that underlie human vision and plant photosynthesis. 1) What type of spectrum is produced when the light emitted directly from a hot, dense object passes through a prism? 2) What type of spectrum is produced when the light emitted directly from a low density cloud passes through a prism? 3) Describe in detail the source of light and the path the light must take to produce an absorption spectrum.

A gas of hydrogen atoms will produce an absorption line spectrum if it is between you (your telescope+spectrograph) and a continuum light source, and an emission line spectrum if viewed from a different angle. If you were to observe the star (a source of white light) directly, you would see a continuous spectrum, with no breaks. A continuous source is one that emits light of every wavelength and there are no gaps in the spectrum produced. Hot objects, such as the sun or an old fashioned incandescent light bulb are examples. A discrete source emits light of only certain well defined wavelengths. Emission spectra observed directly from hot, low-density gas. Absorption Line Spectrum:The opposite of emission lines, absorption spectra are often due to cooler gas absorbing photons emitted from a hot source. An absorption line spectrum appears to be a continuum spectrum with emission lines taken out. Continuum spectrum: In this diagram, a dense hot object such as the core of a star acts like a black body radiator. If we were able to view the light from this source directly without any intervening matter then the resultant spectrum would appear to be a continuum as shown bottom left in the Figure 1 above.

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