Hydrogen Emission Spectrum

How many lines are in the emission spectrum of hydrogen?
Where do these lines come from?
What are the Lyman, Balmer, Paschen, Brackett, Pfund and Humphreys Series?
Find the answers to these questions and more in AUS-e-TUTE's new hydrogen emission spectrum resources.
AUS-e-TUTE Members should log-in to access the new tutorial, game, test and exam (with worked solutions of course!)
If you are not an AUS-e-TUTE member you can access a "free-to-view" Hydrogen Emission Spectrum tutorial at https://www.ausetute.com.au/hspectrum.html

Bohr Model of an Atom

What is the Bohr model of the atom?
What is a planetary model of an atom?
What evidence is there that supports Bohr's model of the atom?

I'm glad you asked these questions!

AUS-e-TUTE has just added a new tutorial, game, test and exam on the topic of Bohr's Model of the Atom.
AUS-e-TUTE Members should log-in to the Members ONLY area to access these new learning resources: http://www.ausetute.com.au/index.html
If you are not an AUS-e-TUTE Member, this tutorial is currently available to view for free for evaluation purposes at http://www.ausetute.com.au/bohrmodel.html

The man who proved the moon isn’t cheese

Meet Emeritus Professor Ross Taylor AC, the Australian who analyzed the first moon rock samples in 1969, in Volume 46 Number 4 of the ANUreporter,

"With emission spectroscopy you can put a tiny amount of material into the flame and quickly identify any of 70 different elements from the spectral lines they produce. But those 70 elements could produce 100,000 possible lines," he says.
At 11.45am on 28 July, Taylor received the first samples. By 4pm, he delivered preliminary results to a press conference - significantly faster than the usual scientific process and with much more at stake.
The high-speed analysis had not been without hiccups. Taylor almost missed one of the most significant traits of the moon's chemistry, its significantly lower sodium levels than Earth.
The moon is also rich in chromium, which has a spectral line that almost perfectly disguised the low sodium result. Only moments before the press conference Taylor realised the mistake and corrected it.
"It would have ruined my reputation," he says.

Reference:
The man who proved the moon isn't cheese

Further Reading:
http://www.ausetute.com.au/emissions.html 
http://www.ausetute.com.au/flametest.html

Suggested Study Questions
1/ What is an emission spectrum?
2/ How can you produce the emission spectrum of metallic elements at school?
3/ How is the emission spectrum of an element used to confirm the existence of energy levels in atomic structure?
4/ What is a flame test?
5/ How does a flame test differ from emission spectroscopy?
6/ How is a flame test similar to emission spectroscopy?
7/ "With emission spectroscopy you can put a tiny amount of material into the flame and quickly identify any of 70 different elements from the spectral lines they produce." 
Explain how emission spectroscopy can be used to identify different elements.
8/ "But those 70 elements could produce 100,000 possible lines,"
Explain how such a huge number of lines can be produced from what seems like a much smaller number of elements.
9/ "The moon is also rich in chromium, which has a spectral line that almost perfectly disguised the low sodium result"
Explain how a chromium spectral line could disguise the low sodium result.
10/ Imagine you have helped Emeritus Professor Ross Taylor AC analyse these moon rock samples. Produce a scientific poster to communicate the results of this experiment to your class.

Uranium Glass

Uranium compounds have been used to colour glass since ancient times. A mosaic found in a Roman villa dated to about 79 AD used yellow glass containing 1% uranium oxide. Between 1880 and the 1920s, uranium glass was quite popular, not only because of its interesting yellow-green colour, but because it fluoresces in ultra-violet light as shown in the image of a vase below.
The image on the left hand side shows the vase under normal daylight, while the image on the right shows the same vase in the dark exposed to UV light.

Why does uranium glass glow green in the dark like this?
Well, it has nothing to do with the radioactivity of uranium isotopes. The green glow does not occur because of changes within the nucleus of uranium atoms, it occurs because of changes in the energy of electrons surrounding the nucleus.
A ground state electron in a uranium atom absorbs the energy of a photon  of ultra-violet light causing the electron to jump to a higher energy level known as the excited state. This new excited state electron configuration is not stable, so, the electron falls back down to to the ground state energy level, which is a lower energy state, by losing energy which it does by emitting a photon of light. Some of the energy of the original photon used to excite an electron is dispersed as molecular vibration and heat, so the energy of the photon emitted when the excited electron falls back to the ground state is less than the energy originally absorbed.
That is: E = hν/λ
where E = energy, h = Planck's constant, ν = speed of light , λ = wavelength of light
If the speed of light is a constant, then E ∝ 1/λ or Eλ = a constant
in other words, the more energy the photon of light has the shorter its wavelength is.
In the case of uranium glass, the absorbed photon of ultra-violet light has a wavelength of about 300 nm, while the emitted photon of green light has a wavelength of about 550 nm.
The wavelength of the emitted photon of light corresponds to the green part of the visible spectrum.
The emission of visible light in this way is known as fluorescence.

Further Reading:
Isotopes
Radioactivity: Properties and Uses
Emission Spectra
Flame Tests

Suggested Study Questions

1. Uranium is found in nature as one of three isotopes, uranium-234, uranium-235 and uranium-238. Explain how atoms of each isotope are:
• the same
• different
2. Atoms of neptunium-234, neptunium-235 and neptunium-238 have been synthesized. Explain the similarities and differences between each of the following pairs of atoms:
   • neptunium-234 and uranium-234
   • neptunium-235 and uranium-235
   • neptunium-238 and uranium-238
3. The value for Planck's constant is 6.626 070 040 x 10^-34 J s and the speed of light is given as 300 000 000 m / s. Calculate the energy of each of the following photons of light:
• ultra-violet light, λ = 300 nm
• green light, λ = 550 nm
4. Using the results of question 3, compare the energy of the photons used to excite uranium atoms and the energy of the photons emitted by uranium atoms and explain the difference.
5. Explain why the same wavelength of light is always emitted when these uranium atoms are exposed to ultra-violet light.
6. Would you expect the uranium glass to fluoresce if it is exposed to infra-red light rather than to ultra-violet light? Explain your answer.
7. Optical brighteners are often used in laundry detergents to make your old, yellowy-looking white clothes look whiter. Typically these compounds absorb ultra-violet light with a wavelength of around 300 nm and emit light with a wavelength of around 450 nm.
   • What colour is the light emitted?
   • What is the energy of the emitted light?
   • Why is the energy of the light emitted not the same as the energy absorbed when the incoming photon hits the "optical brightening compound"?
   • Would you expect a laundry detergent containing "optical brightening compounds" to glow in the dark when exposed to UV light? Explain your answer.

Argon Hydride in Space

Almost 1,000 years ago, the Chinese recorded a bright new object in the night sky. This is believed to be a star that exploded. The remnant of that exploded star is now called the Crab Nebula and it is about 6,500 light years from Earth.
Europe launched its Herschel Space Observatory in 2009, and in 2012 Astronomers used it to study the emission lines from Crab Nebula. What the scientists found were 2 bright emission lines from an area of shining dust. It was only by consulting databases of the known properties of different molecules that the scientists could finally identify these emission lines as coming from a very special molecule, argon hydride.
Argon hydride is special because it is the first time that molecules of a Noble Gas (Group 18) element have been found in space. On Earth, the naturally occurring Noble Gas (Group 18) elements are monatomic gases. Atoms of Noble Gas elements have a full valence shell of electrons so they tend not to react with other atoms.
Something really interesting must be happening in the Crab Nebula for argon hydride to be formed naturally. The researchers believe that the argon formed when the original star exploded. The intense energy of the explosion stripped electrons off the argon atoms, ionising them. Ionised argon atoms then reacted with hydrogen molecules to form argon hydride molecules.

Reference
M. J. Barlow, B. M. Swinyard, P. J. Owen, J. Cernicharo, H. L. Gomez, R. J. Ivison, O. Krause, T. L. Lim, M. Matsuura, S. Miller, G. Olofsson, E. T. Polehampton. Detection of a Noble Gas Molecular Ion, 36ArH , in the Crab Nebula. Science, 2013; 342 (6164): 1343 DOI: 10.1126/science.1243582

Further Reading
http://ausetute.com.au/trendec.html
http://ausetute.com.au/trendie.html
http://ausetute.com.au/massconv.html
http://ausetute.com.au/members/emissions.html

Suggested Study Questions:

1. 1 light year is approximately 9.5 x 10¹⁵ metres. How far from Earth is the Crab Nebula in kilometres?
2. 1 astronomic unit (1 AU) is approximately 1.5 x 10¹¹ metres. What is the distance between Earth and the Crab Nebula in astronomic units?
3. What sort of instrument can be used to observe the emission lines of hot gases?
4. Explain how these emission lines are produced.
5. Give the electron configuration of an atom of argon.
6. With reference to the electron configuration of argon, explain why compounds of argon are not found naturally on Earth.
7. Write an equation to show the loss of an electron from a gaseous argon atom.
8. Explain how the hydride ion can be formed from a hydrogen atom.
9. Give a likely molecular formula for a molecule of argon hydride.
10. Is argon hydride most likely to an ionic compound or a covalent compound? Explain your answer.

Chemistry in Eclipses

The 14th November 2012 excites students of physics and those interested in astronomy. This is the date of a total eclipse of the sun. The area of totality will pass over northern Australia, from east of Darwin in the Northern Territory to the Cape York Peninsula of Far North Queensland, turning morning into darkness. The rest of Australia will see a partial eclipse.

But why would chemists get excited about a solar eclipse?

The story begins more than 200 years ago ...

Gaps in the Solar Spectrum?

In 1802 an English Chemist, William Hyde Wollaston, was the first person to record the appearance of a number of dark lines in the emission spectrum of light from the sun.

In 1814, German physicist Joseph von Fraunhofer began measuring the wavelengths of over 570 of these lines.

Fingerprinting the Sun

Robert Gustave Kirchhoff and Robert Bunsen, developed a better prism-based spectroscope and observed that the spectral lines emitted by a gas occurred at the same wavelength as the absorption lines observed when incandescent light from Bunsen's burner shone through the same gas heated at the same temperature.

Then Kirchhoff,  proposed the laws of spectroscopy which bear his name:

1. A hot solid object produces light with a continuous spectrum
2. A hot tenuous gas produces light with spectral lines at discrete wavelengths (an emission spectrum)
3. A hot solid object surrounded by a cooler tenuous gas produces light with an almost continuous spectrum with gaps at discrete wavelengths (an absorption spectrum)

A star, like the sun, will create an absorption line spectrum because the continuous spectrum emitted by the dense, opaque gas that makes up most of the star passes through the cooler, transparent atmosphere of the star.

In 1859, Kirchhoff  demonstrated that all pure substances display their own characteristic spectrum, so it is possible to use the spectrum of elements to identify elements in a mixture, just like each person's fingerprints are unique and can be used to identify them. He proposed  that the lines in the solar spectrum are caused by the absorption of light by elements in the solar atmosphere and set out to identify the elements present in our sun.

New Element Discovered

On the 18th August 1868 there was a total solar eclipse. In India, French astronomer Pierre Janssen observed this eclipse using a spectroscope. He recorded a bright yellow line with a wavelength of 587.49 nm in the spectrum of the solar prominences. The same result was also recorded by British astronomer Norman Lockyer. This line could not be due to sodium, because although sodium produces a bright yellow line (actually more than 1), the wavelength of sodium's 'line' is about 589.3 nm. Lockyer proposed that this line was due to a new element which he called helium after the greek word 'helios' meaning 'sun'.

About 10 years later, Scottish chemist William Ramsay isolated helium on earth ...... but that's another story.

References:

http://eclipse.aaq.org.au/

http://www.csiro.au/en/Outcomes/Understanding-the-Universe/Tracking-spacecraft/History-of-total-solar-eclipses.aspx

Further Reading:

Emission Spectra 

Suggested Study Questions:

1. speed of light (m/s) = frequency (s^-1) x wavelength (m)
   If the speed of light is 3 x 10⁸ ms^-1 calculate:
• find the frequency of the 'yellow line' in sodium's spectrum
• find the frequency of the yellow line for the new element found in the solar spectrum
2.  speed of light (m/s) = frequency (s^-1) x wavelength (m)
   If the speed of light is 3 x 10⁸ ms^-1 calculate:
• wavelength of blue light with a frequency of 6.9 x 10¹⁴ s^-1
• wavelength of red light with a frequency of 4.6 x 10¹⁴ s^-1
  
3. The energy of light emitted, E, is Planck's constant,h, multiplied by the speed of light divided by the wavelength of light emitted. Write a mathematical equation to represent this.
4. Use your equation above to calculate
   • energy of the blue light in question 2 above
   • energy of the red light in question 2 above
5. Complete the following generalizations:
   • The longer the wavelength of light, the ___________ energy it has
   • The shorter the frequency of light, the _________ energy it has.
6. Compare the wavelength of the 'yellow line' in sodium's spectrum and the yellow line for the 'new element'. Which element has
   • the longest wavelength
   • the shortest frequency
   • the most energy
7. Describe the difference in the spectrum of light from the sun as seen in a spectroscope compared to the spectrum of light from a fluorescent light as seen in a spectroscope.
8. Explain the differences between the two spectrum in question 7 above.

Glow in the Dark Ice

No (chemistry) party is complete without edible "glow in the dark" ice cubes.
To make your ice cubes:

•  open up some tonic water (or a bottle of "bitter lemon")
• pour it into an ice cube mold
• place the mold in the freezer until the tonic water solidifies (freezes)

To make your ice cubes glow in the dark:

• place some ice cubes in a glass of water (or cordial or carbonated beverage)
• place the glass under a UV ("black") light (even strong fluorescent light will work but the effect is not as dramatic!) and turn off the room's lights

Results : your glass of water and ice should glow a nice blue colour.


This is an example of fluorescence, the emission of light by a substance that has absorbed electromagnetic radiation. In the case of the tonic water, there is a compound in the tonic water that absorbs light in the ultraviolet region of the electromagnetic spectrum (wavelength ~ 350 nm), and emits light in the visible region of the electromagnetic spectrum (wavelength ~ 450 nm corresponding to bright blue or cyan).

The compound in the tonic water that fluoresces is known as quinine, with the molecular formula C₂₀H₂₄N₂O₂ and the structural formula shown below:

Quinine occurs naturally in the bark of the cinchona tree which is found in the tropical Andes forests of western South America. Quinine was the first effective treatment for malaria. The first medicinal uses involved drying the bark of the cinchona tree then grinding it into a powder which was then mixed into a drink (often wine), which was then drunk. The effective medicinal ingredient of the bark, quinine, was finally isolated in 1820 by French researchers Pierre  Joseph Pelletier and Joseph Bienaime Caventou.
During World War II, the Axis Powers had control over most of the commercial quinine production centres, so the Allied Powers were cut off from their supply of quinine, a necessary war-time commodity for fighting in the tropics. Then in 1944, the American chemists R.B. Woodward and W.E. Doering succeeded in producing quinine in the laboratory.




Quinine is no longer recommended as a first-line treatment of malaria, instead another plant-derived organic compound is used, artemisinin, but that's a different story.

Further Reading:
Emission Spectroscopy
Empirical Formula
Relative Molecular Mass (molecular weight, formula mass, formula weight)
Percent Composition
Parts per Million Concentration
Functional Groups


Suggested Study Questions:

1. Draw a diagram to describe what happens when quinine absorbs UV light and emits bright blue/cyan light.
2. Imagine you were to view the light emitted by the tonic water through a spectroscope. Draw a sketch of the emission spectrum you would expect to see.
3. Use the molecular formula for quinine to find its empirical formula.
4. Calculate the relative molecular mass (molecular weight, formula mass, formula weight) of quinine.
5. Calculate the percentage of each element present in quinine.
6. Assume a 1L bottle of tonic water contains 15ppm quinine. Calculate the
   • mass of quinine contained in the bottle
   • moles of quinine in the bottle
   • quinine concentration in mol L^-1
7. Using the structural formula for quinine, identify an aliphatic double bond (that is, a double bond that does not occur in an aromatic ring), an aromatic (benzene) ring, and an hydroxyl group

Lithium for a Longer Life

Lithium is the 25^th most abundant element in the Earth's crust, with approximately 20mg of lithium present in every kilogram of crustal material. It is a soft, silvery-white metal that belongs to Group I (alkali metals). It is so highly reactive that when it is cut in air it will quickly corrode before your eyes. In the presence of water, lithium reacts to form hydrogen gas and lithium hydroxide in aqueous solution. Because it is so reactive, lithium does not occur free in nature, it only appears naturally in compounds.

Lithium-6 and lithium-7 were among the three elements synthesized in the Big Bang according to cosmological theory, the other two elements being hydrogen and helium. Lithium is present in cooler, less massive brown dwarf stars but is destroyed in hotter red dwarf stars, so its presence in the stars' line emission (atomic) spectra can be used to differentiate between these two kinds of stars in the so-called 'lithium test'.

Trace amounts of lithium ions are present in the oceans. The total lithium content of seawater is estimated to be 230 billion tonnes, and is present in concentrations of about 0.2 parts per million.
Lithium is also present in trace amounts in plants and animals. Vertebrates contain lithium in concentrations between 21 and 763 parts per billion.

Lithium salts, such as lithium carbonate, have been to shown to be useful as mood-stabilizing drugs. Therapeutically useful amounts of lithium are between 1.0 and 1.2 millimolar, which is only slightly lower than the toxic amount of 1.5 millimolar.

Scientists at the Friedrich Schiller University Jena have just demonstrated that a regular uptake of lithium could lead to a longer life. The scientists studied the impact of lithium in a concentration that is regularly found in ordinary tap water by analyzing the mortality rate in 18 adjacent Japanese municipalities in relation to the amount of lithium contained in tap water from the respective regions. They found that the mortality rate was considerably lower in those municipalities with more lithium in the drinking water.

Reference
Kim Zarse, Takeshi Terao, Jing Tian, Noboru Iwata, Nobuyoshi Ishii, Michael Ristow. Low-dose lithium uptake promotes longevity in humans and metazoans. European Journal of Nutrition, 2011; DOI: 10.1007/s00394-011-0171-x

Further Reading
Elements and Compounds
Metals and Non-metals
Trends in Group I
Electron Configuration
Naming Ionic Compounds
Writing Ionic Formulae
Parts per Million Concentration
Molarity Concentration
Emission (Atomic) Spectra
Isotopes
Relative Atomic Mass

Study Questions

1. What is the atomic number of lithium?
2. What is the simple electron configuration for an atom of lithium?
3. What is the expected charge on a lithium ion? Explain your answer.
4. Write the formula for each of these compounds:
   
   • lithium hydroxide
   • lithium carbonate
5. Write a balanced chemical equation to represent the reaction between lithium metal and water.
6. For each of the following isotopes of lithium, give the number of protons and the number of neutrons present:
   
   • lithium-6
   • lithium-7
7. Given that the relative atomic mass of lithium is 6.941, and assuming lithium-6 and lithium-7 are the only isotopes of lithium present, calculate the abundance of each isotope.
8. Convert the following to concentrations in molL^-1 (M):
   
   • 0.2ppm
   • 1.2millimolar
   • 1.5millimolar
     
   • 21ppb
   • 763ppb
9. If the total lithium content of seawater is estimated to be 230 billion tonnes, and is present in concentrations of about 0.2 parts per million, what is the mass of seawater present on Earth?
10. In the 'lithium test' for stars, what spectral lines do you expect to see in brown dwarf stars that will not be present in red dwarf stars?