answersLogoWhite

0

A spectrum that contains only certain colors, or wavelengths, is called a line spectrum. For every element, the emitted light contains only certain wavelentghs, giving each element a unique line spectrum.

They exist for atomic fingerprinting, which is useful in identifying elements. They are also used in sodium-vapor lmaps, which are widely used for street lighting. They are also used in "neon" lights.

User Avatar

Wiki User

15y ago

What else can I help you with?

Continue Learning about Earth Science

How are the elements identified from bright light line spectra?

Elements are identified from bright light line spectra by analyzing the unique pattern of emission lines produced when the element is heated. Each element emits a specific set of wavelengths of light, resulting in a distinct spectral fingerprint that can be compared to known spectra to determine the element present. This technique is known as spectroscopy and is commonly used in chemistry and astronomy.


Where can you find an IR Spectra for Potassium Oxalate monohydrate and what is the spectra number?

Best guess would be the Sadtler spectra; no idea what the number would be.


What are some ways that you know cold clouds of gas exist in space?

Cold clouds of gas in space can be detected by studying their emission lines in the radio wavelength spectrum. They also often exhibit absorption features in the spectra of background light sources. Additionally, their presence can be inferred from their effects on the surrounding environment, such as blocking or scattering light.


What is the maximum time difference that can exist between two locations on Earth?

The maximum time difference between two locations on Earth is 24 hours, which occurs when they are on opposite sides of the International Date Line.


Characteristic series of frequencies of electromagnetic radiation substances emit?

Each substance emits a unique characteristic series of frequencies of electromagnetic radiation when it is heated or excited. These frequencies correspond to specific energy transitions within the atoms or molecules of the substance. By studying these emission spectra, scientists can identify the composition of the substance and gain insights into its structure and properties.

Related Questions

When was Line Spectra created?

Line Spectra was created in 2006.


The line spectra of atoms provides experimental evidence for?

The line spectra of atoms provide experimental evidence for the quantization of energy levels in atoms. This supports the idea that electrons can only exist in specific energy levels within an atom's electron shells. The specific wavelengths of light emitted or absorbed by atoms in their line spectra confirm the discrete nature of energy levels and the transitions between them.


What are the differences between line spectra and continuous spectra in terms of their characteristics and properties?

Line spectra are composed of distinct, discrete lines of light at specific wavelengths, while continuous spectra consist of a continuous range of wavelengths without distinct lines. Line spectra are produced by excited atoms emitting light at specific energy levels, while continuous spectra are emitted by hot, dense objects like stars. Line spectra are unique to each element and can be used to identify elements, while continuous spectra are characteristic of hot, dense objects emitting thermal radiation.


How can forensic scientists use emission line spectra and absorption spectra?

Forensic scientists can use emission line spectra and absorption spectra to analyze trace evidence, such as glass fragments or paint chips, found at a crime scene. By comparing the spectra of the collected samples with reference spectra, scientists can identify the chemical composition of the evidence and link it to potential sources or suspects.


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


Bohr postulated that elements have unique line spectra because?

Bohr postulated that elements have unique line spectra because the electrons in an atom can only occupy certain energy levels. When an electron moves between energy levels, it emits or absorbs energy in the form of light. Each element has a distinct arrangement of electrons, leading to unique line spectra.


What experimental evidence led to bohr to believe that electrons can posses only specific amounts of energy?

The observation of discrete emission spectra from elements provided the experimental evidence for Bohr's model. The only way to explain these spectra was through quantization of electron energy levels in atoms. This led Bohr to propose that electrons could only exist in specific orbits with quantized energy levels.


How do we know that the elements that exist on earth are the same throughout the universe?

Because we can see their spectra in starlight from the rest of the universe.


What causes spectra lines?

Absorption of energy at atom energy levels cause the line spectrum.


Bohr found experimental evidence for his atomic model by studying?

The electron cloud


What has the author Kenneth Bruce McBeath written?

Kenneth Bruce McBeath has written: 'Rapid variations of Balmer line strengths in the spectra of Be stars' -- subject(s): Spectra, B stars


Why was the study of line spectra useful in the discovery of new elements?

The study of line spectra was useful in the discovery of new elements because each element has a unique line spectrum that can help identify and distinguish it from others. By examining the line spectra of unknown substances, scientists could match their patterns with known elements, revealing the presence of new elements with distinct spectral signatures. This technique played a crucial role in the discovery and characterization of many new elements in the periodic table.