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How absorption spectra can be used in the identification of unknowns?

Each substance has known specific maximum of absorption. Comparing spectra substances can be identified.


What has the author Charles R Cowley written?

Charles R. Cowley has written: 'The theory of stellar spectra' -- subject(s): Spectra, Stars 'An introduction to cosmochemistry' -- subject(s): Astrogeology, Astrophysics, Cosmochemistry 'Line identification studies using traditional techniques and wavelength coincidence statistics' -- subject(s): Abundance, Line spectra, Statistical analysis, Stellar spectra


What is the three criteria for a positive identification on the HAZMAT ID?

Has to be greater than .95 to be accurate Spectra corresponds (same) Physical properties match


What has the author J C McLennan written?

J. C. McLennan has written: 'Report on some sources of helium in the British empire' -- subject(s): Helium, Gases 'On the radioactivity of mineral oils and natural gases' -- subject(s): Radioactivity, Mineral oils, Gases 'On the absorption spectra of mercury, cadmium, zinc, and other metallic vapours' -- subject(s): Spectra, Mercury, Cadmium, Absorption spectra, Zinc 'The radioactivity of lead' -- subject(s): Radioactivity, Lead 'Electric screening in vacuum tubes' -- subject(s): Experiments, Electric discharges through gases, Electrodes


How would it be possible to identify the gases in the other light sources based on their emission spectra?

You can use a spectrometer to analyze the emission spectra of the light from these sources. By comparing the spectral lines to known patterns for different gases, you can identify the gases present. Each gas has a unique set of spectral lines due to the arrangement of its energy levels, making it possible to determine the composition of the gas based on its emission spectrum.


How do different scientists spectra to figure out the composition of a star's outer layer?

The color of the light radiated by the spectra can show the internal composition as well as the gases burning on the outer layer. Red stars are colder and blue stars are hotter.


What has the author Lothar Frommhold written?

Lothar Frommhold has written: 'Collision-induced absorption in gases' -- subject(s): Absorption and adsorption, Gases, Infrared radiation, Molecular spectra 'Collision-induced Absorption in Gases (Cambridge Monographs on Atomic, Molecular and Chemical Physics)'


How can the emission spectra be used to identify the components in a mixture?

Emission spectra can be used to identify components in a mixture by analyzing the unique patterns of light emitted by each component when subjected to energy. By comparing these patterns to known spectra of elements or compounds, scientists can determine the composition of the mixture. Each component will emit specific wavelengths of light that can be matched to known standards, aiding in identification.


Is solar spectra a continuous spectra?

The Sun spectra is considered continuous.


How Many types of Infrared Spectra?

There are three main types of infrared spectra: absorption spectra, emission spectra, and reflection spectra. Absorption spectra are produced when a material absorbs infrared energy, emission spectra are produced when a material emits infrared radiation, and reflection spectra result from the reflection of infrared radiation off a material.


What gases which we can detect if present in infrared spectra would be a strong indicator of life on another planet?

Gases such as oxygen (O₂), methane (CH₄), and carbon dioxide (CO₂) are strong indicators of potential life when detected in infrared spectra. The simultaneous presence of oxygen and methane is particularly intriguing, as these gases can react with each other and would require a continual source of replenishment, typically from biological processes. Additionally, other compounds like ozone (O₃) and nitrous oxide (N₂O) could also suggest biological activity.


What has the author Richard H Tourin written?

Richard H. Tourin has written: 'Spectroscopic gas temperature measurement' -- subject(s): Gases, Plasma spectroscopy, Pyrometry, Spectra