Tellurium
What do diphtheria, isotopes and garlic breath have in common?
This week’s element is tellurium, which has the symbol Te and the atomic number, 52. Its name comes from the Latin, tellus, for “earth”. Despite its name, this lustrous, pale grey metalloid is quite rare on earth, rarer than it is elsewhere in the universe, in fact. The reason for its comparative rarity is attributed to the formation of H2Te, a volatile gas that was lost to space during the early formation of earth.
Tellurium is used in a number of industrial and commercial applications. It is alloyed with stainless steel and copper to improve their machinability and tellurium is used as a semiconductor, cadmium telluride is used in solar panels because it has the highest efficiency for electricity generation, tellurium speeds the curing of rubber and renders it less susceptible to aging and to the softening effects of oil, and tellurium oxide, TeO, is used in some rewritable CDs and DVDs.
When I was a microbiologist, one of the many types of growth media that I used to diagnose human pathogens was an agar made with serum and potassium tellurite (K2TeO3). This agar is used specifically to diagnose the human respiratory pathogen, Corynebacterium diphtheriae. Tellurite agar is a selective medium because tellurium inhibits growth of a variety of bacteria, and it is a differential medium because Corynebacterium will reduce tellurite to metallic tellurium, producing characteristic black or brownish-black colonies on the otherwise pale straw-coloured and transparent agar.
In humans and other animals, tellurium has no known biological role, but the body does metabolise it to create the volatile gaseous compound, dimethyl telluride, (CH3)2Te, which is excreted in sweat and exhaled, and is the source of a charmingly potent “garlic breath”, similar to what happens with selenium ingestion. (Which makes me wonder why don’t any of these elements make people smell minty or fruity? Why must we always smell like a litter box?) I should point out that taking vitamin C can reduce these odoriferous effects.
Tellurium can be toxic if ingested in high enough quantities. *
Chemically speaking, the discovery of tellurium caused the inventor of the periodic table of elements, Dmitri Mendeleev, a lot of headaches. This is because tellurium has an atomic mass of 127.6 whilst the element that comes after it, iodine, is lighter with an atomic weight of 126.9. Mendeleev concluded that the atomic mass for one of these two elements must be wrong because tellurium clearly preceded iodine in the periodic table. After 50 years of headbanging frustration and effort by a number of chemists to accurately determine the atomic mass of these two elements, the concept of chemical isotopes was discovered. Isotopes are variant forms of an element that maintain the element’s characteristic number of protons, but contain variable numbers of neutrons. As it turns out, the most common isotopes of tellurium have atomic masses of 128 and 130, whilst iodine’s most common isotope has an atomic mass of 127. Thus, tellurium has an average atomic mass of 127.6 whilst iodine has an average atomic mass of 126.9.
Here’s our favourite chemistry professor telling us more about tellurium:
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* [added 1430 on 2 March 2012] Tellurium is “[h]ighly toxic, may be fatal if inhaled, swallowed or absorbed through skin. Avoid any skin contact. Effects of contact or inhalation may be delayed.”. Sodium tellurite is also toxic: “The material is both an oral and dermal toxic hazard. The material is toxic by ingestion. Oral ingestion of tellurium compounds is generally regarded as extremely toxic. The probable oral lethal dose is 5-50 mg/kg or between 7 drops and 1 teaspoonful for a 70 kg (150 pound) person. Tellurium compounds are regarded as super toxic for skin exposures.”
Source: http://www.guardian.co.uk/science/grrlscientist/2012/mar/02/1
Rare Element on Earth Discovered in Ancient Starlight

A photo of an ultra pure tellurium crystal. Astronomers have discovered the material in deep space by analyzing light from three ancient stars. CREDIT: MIT
Light from three ancient stars at the edge of the Milky Way indicates that the stars contain tellurium, a brittle, superconducting element that is rare on Earth.
The cosmic discovery, which also spotted traces of other heavy elements, supports the theory that these elements were synthesized in the rapidly collapsing cores of rare supernovas (stellar explosions).
“You can make iron and nickel in any ordinary supernova, anywhere in the universe,” said Anna Frebel, an astrophysicist at the Massachusetts Institute of Technology and a member of the research team. “But these heavy elements seem to only be made in specialized supernovas.”
According to the theory, heavy atoms form during rapid nuclear fusion at the heart of some supernovas. Called r-process, it sets in when a supernova core collapses, bombarding atomic nuclei with a fierce onslaught of neutrons. The result is the production of atoms heavier than iron, which then get hurled into space, enriching the cloud of gas and dust that eventually collapses to form another star.
And if the theory is right, some of those atoms ought to end up in stars like those analyzed by Frebel and the rest of her team. [Supernova Photos from Star Explosions]
To analyze the chemical composition of the three stars at the Milky Way’s edge, the researchers studied data gathered by the Hubble Space Telescope’s spectrograph, an instrument that splits incoming starlight into a spectrum of wavelengths. If an element is present in a star, the atoms of that element absorb starlight at specific wavelengths, leaving telltale dips in signal in the spectrograph’s data.
The scientists detected dips in the ultraviolet region of the spectrum at a wavelength that matched tellurium’s light absorption, signifying the presence of the rare element in the 12-billion-year-old stars. Furthermore, the abundance of tellurium relative to that of other heavy elements, such as barium and strontium, was the same in all three stars. According to Frebel, the matching ratios support the theory that a rare type of supernova may have created the elements in the bottom half of the periodic table, including tellurium.
The finding helps flesh out one chapter in the cosmic history of the elements, an ongoing effort of astronomers and nuclear physicists to understand the formation of the 94 naturally occurring types of matter.
According to Jennifer Johnson, an associate professor of astronomy at Ohio State University who was not involved in the new research, tellurium has been a “tough” element to detect because it absorbs light in the ultraviolet spectrum. UV signals tend to be flooded by sunlight and are impossible for ground-based telescopes to spot.
“If you look at the periodic table, tellurium is right in the middle of these elements that are hard for us to measure,” Johnson said in a statement. “If we need to understand how [the r-process] works in the universe, we really have to measure this part of the periodic table. It’s really cool that they got this element in this sea of unknown-ness.”
Frebel and her colleagues are attempting to fill in other spots in the periodic table, too, by looking for signs of other heavy elements in starlight. “There are still quite a few holes,” she said. “Every now and then, we can add an element, and it adds another data point that makes our work easier.”
The researchers have published their findings online in Astrophysical Journal Letters.
This story was provided by SPACE.com, a sister site to LiveScience
Source: http://www.livescience.com/18614-rare-earth-element-tellurium-ancient-stars.html
Supply Threats Persist For Thin-Film Solar Materials Due To Competition
One year ago, a report from the U.S. Department of Energy (DOE) on the global supply of essential PV module materials predicted possible disruptions for thin-film manufacturing.
The availability of indium, gallium and tellurium was examined in the context of current and future production needs, and the DOE found cause for concern. Indium and tellurium were pegged as especially vulnerable to supply tightness and price volatility, according to both the report and several market analysts at the time.
(See “New Government Report Identifies Supply Risks For Thin-Film PV Materials” in the February 2011 issue of Solar Industry.)
Now, the DOE has released the latest edition of its Critical Materials Strategy. Have the worries over thin-film PV materials supply eased? According to the DOE, the general supply-demand picture for indium, gallium and tellurium has “improved slightly,” but the situation is not entirely reassuring. The three metals are still highlighted (alongside neodymium and dysprosium) as clean-energy materials that face a “significant risk of supply chain bottlenecks in the next two decades.”
The report attributes the slight improvement primarily to decreased demand for the three thin-film materials: Although PV deployment is expected to grow, the requirements of the materials per module are expected to shrink.
For copper indium gallium diselenide (CIGS) modules, manufacturers are shifting to compositions with higher proportions of gallium and lower concentrations of indium, the DOE says. The result is a “partial trade-off in the potential for supply risk between the two elements.” At the same time, CIGS’ market share assumption has been reduced under the DOE’s new calculations, lowering projected demand for both indium and gallium.
Cadmium telluride (CdTe) thin-film modules currently account for approximately 10% of the PV market, according to the report. Declining silicon prices may threaten this slice of the market, but high tellurium costs and the increasing need for CdTe manufacturers to compete for supply with non-PV companies requiring tellurium continue to cause supply headaches.
“The cost of tellurium is a critical issue for CdTe solar cell makers, and the industry is working to lower material use and increasing recovery of new scrap to reduce reliance on primary tellurium,” the DOE says in the report.
Although short-term supply of tellurium appears adequate, future capacity increases may be insufficient to supply both CdTe manufacturing and the multitude of other manufacturing sectors that use tellurium. Under one scenario modeled in the report, tellurium supply would need to increase 50% more than its projected 2015 total in order to meet expected demand.
Indium and gallium have also experienced increased popularity in non-PV manufacturing uses, such as semiconductor applications, flat-panel displays, and coatings for smartphones and tablet computers. The DOE forecasts that as a result, supplies may run short by 2015 unless production of these materials is increased – or non-PV demand lessens.
Of the two metals, gallium poses more cause for concern, as the DOE has adjusted its assumptions of future gallium use under CIGS manufacturers’ expected manufacturing modifications.
“These higher estimates [of gallium requirements] are driven largely by the assumption that gallium will increasingly be substituted for indium in CIGS composition,” the DOE explains. This change points to the benefits of reducing material intensity in other aspects of PV manufacturing, such as reducing cell thickness and improving processing efficiency.
Overall, indium, gallium and tellurium all receive moderate scores (2 or 3 on a scale of 1 to 4) from the DOE with regard to both their importance to clean energy and short- and medium-term supply risk.
In order to help mitigate possible supply disruptions that could threaten the manufacturing and deployment of PV, as well as other types of clean energy, the agency has developed a three-pronged approach.
“First, diversified global supply chains are essential,” the DOE stresses in the report. “To manage supply risk, multiple sources of materials are required. This means taking steps to facilitate extraction, processing and manufacturing here in the United States, as well as encouraging other nations to expedite alternative supplies.”
The second strategy relies on developing alternatives to materials whose supply may be constrained. For PV, one DOE research program focuses on advancements in thin-film formulations such as copper-zinc-tin and sulfide-selenide. Another initiative funds research and development into PV inks based on earth-abundant materials such as zinc, sulfur and copper.
“Several projects also seek to use iron pyrite – also known as fool’s gold – to develop prototype solar cells,” the DOE notes in the report. “Pyrite is non-toxic, inexpensive, and is the most abundant sulfide mineral in the Earth’s crust.”
Finally, improving recycling and reuse mechanisms can reduce demand for new materials, the DOE says, adding that these strategies also can help improve the sustainability of manufacturing processes.
Source: http://www.aer-online.com/e107_plugins/content/content.php?content.9408
Photo: Enbridge Inc.’s 5 MW Tilbury solar project in Ontario uses First Solar’s cadmium telluride thin-film modules. Photo credit: Enbridge
Supply Threats Persist For Thin-Film Solar Materials Due To Competition
One year ago, a report from the U.S. Department of Energy (DOE) on the global supply of essential PV module materials predicted possible disruptions for thin-film manufacturing.
The availability of indium, gallium and tellurium was examined in the context of current and future production needs, and the DOE found cause for concern. Indium and tellurium were pegged as especially vulnerable to supply tightness and price volatility, according to both the report and several market analysts at the time.
Now, the DOE has released the latest edition of its Critical Materials Strategy. Have the worries over thin-film PV materials supply eased? According to the DOE, the general supply-demand picture for indium, gallium and tellurium has “improved slightly,” but the situation is not entirely reassuring. The three metals are still highlighted (alongside neodymium and dysprosium) as clean-energy materials that face a “significant risk of supply chain bottlenecks in the next two decades.”
The report attributes the slight improvement primarily to decreased demand for the three thin-film materials: Although PV deployment is expected to grow, the requirements of the materials per module are expected to shrink.
For copper indium gallium diselenide (CIGS) modules, manufacturers are shifting to compositions with higher proportions of gallium and lower concentrations of indium, the DOE says. The result is a “partial trade-off in the potential for supply risk between the two elements.” At the same time, CIGS’ market share assumption has been reduced under the DOE’s new calculations, lowering projected demand for both indium and gallium.
Cadmium telluride (CdTe) thin-film modules currently account for approximately 10% of the PV market, according to the report. Declining silicon prices may threaten this slice of the market, but high tellurium costs and the increasing need for CdTe manufacturers to compete for supply with non-PV companies requiring tellurium continue to cause supply headaches.
“The cost of tellurium is a critical issue for CdTe solar cell makers, and the industry is working to lower material use and increasing recovery of new scrap to reduce reliance on primary tellurium,” the DOE says in the report.
Although short-term supply of tellurium appears adequate, future capacity increases may be insufficient to supply both CdTe manufacturing and the multitude of other manufacturing sectors that use tellurium. Under one scenario modeled in the report, tellurium supply would need to increase 50% more than its projected 2015 total in order to meet expected demand.
Indium and gallium have also experienced increased popularity in non-PV manufacturing uses, such as semiconductor applications, flat-panel displays, and coatings for smartphones and tablet computers. The DOE forecasts that as a result, supplies may run short by 2015 unless production of these materials is increased – or non-PV demand lessens.
Of the two metals, gallium poses more cause for concern, as the DOE has adjusted its assumptions of future gallium use under CIGS manufacturers’ expected manufacturing modifications.
“These higher estimates [of gallium requirements] are driven largely by the assumption that gallium will increasingly be substituted for indium in CIGS composition,” the DOE explains. This change points to the benefits of reducing material intensity in other aspects of PV manufacturing, such as reducing cell thickness and improving processing efficiency.
Overall, indium, gallium and tellurium all receive moderate scores (2 or 3 on a scale of 1 to 4) from the DOE with regard to both their importance to clean energy and short- and medium-term supply risk.
In order to help mitigate possible supply disruptions that could threaten the manufacturing and deployment of PV, as well as other types of clean energy, the agency has developed a three-pronged approach.
“First, diversified global supply chains are essential,” the DOE stresses in the report. “To manage supply risk, multiple sources of materials are required. This means taking steps to facilitate extraction, processing and manufacturing here in the United States, as well as encouraging other nations to expedite alternative supplies.”
The second strategy relies on developing alternatives to materials whose supply may be constrained. For PV, one DOE research program focuses on advancements in thin-film formulations such as copper-zinc-tin and sulfide-selenide. Another initiative funds research and development into PV inks based on earth-abundant materials such as zinc, sulfur and copper.
“Several projects also seek to use iron pyrite – also known as fool’s gold – to develop prototype solar cells,” the DOE notes in the report. “Pyrite is non-toxic, inexpensive, and is the most abundant sulfide mineral in the Earth’s crust.”
Finally, improving recycling and reuse mechanisms can reduce demand for new materials, the DOE says, adding that these strategies also can help improve the sustainability of manufacturing processes.
By: SI Staff
Source: http://www.aer-online.com/e107_plugins/content/content.php?content.9408
Photo: Enbridge Inc.’s 5 MW Tilbury solar project in Ontario uses First Solar’s cadmium telluride thin-film modules. Photo credit: Enbridge
Thermoelectrics: Roughing it
(Nanowerk News) Thermoelectric materials convert a temperature gradient into a voltage. Most thermoelectrics, however, are too inefficient for widespread practical application. Still, the possibility that these materials could usefully harness heat waste, such as that generated by combustion engines, makes improving their efficiency an important pursuit in materials science. A team of scientists led by Wooyoung Lee at Yonsei University in Korea has now shown that interface roughening may be an effective way to enhance the thermoelectric properties of core/shell nanowires (“Reduction of Lattice Thermal Conductivity in Single Bi-Te Core/Shell Nanowires with Rough Interface”).
In the ideal thermoelectric, the charge conducts easily from a hot point to a cold one, while heat conduction is low. The ratio between these quantities is contained in the thermoelectric ‘figure of merit’.

Nanowires with a bismuth core encased in a tellurium shell have improved thermoelectric properties when the interface between the core and shell is roughened by impeding the flow of phonons, but not electrons.
As both electrons and vibrational waves in the lattice, known as phonons, contribute to a material’s thermal conductivity, Lee and his colleagues attempted to raise a material’s thermoelectric figure of merit by suppressing the conductivity of phonons without impairing electrical conductivity. This can be achieved by adding defects or nanostructuring a material to make it smaller than the phonon mean-free path — the typical distance a phonon travels before it scatters.
Lee and his team combined both of these tricks to reduce the thermal conductivity of a promising thermoelectric material consisting of a bismuth nanowire core coated with a tellurium shell. The team synthesized the wires by cooling just-prepared bismuth nanowires with liquid nitrogen and then coating them with tellurium using a sputtering technique, giving a core/shell structure with a smooth interface. They also prepared the wires without the cooling step, resulting in a rough interface.
After examining a series of the core/shell nanowires of 160–460 nm in diameter in both the smooth and rough versions, the researchers noticed two trends: the narrowest wires had the lowest thermal conductivity, and wires with rough interfaces had lower thermal conductivity than those with smooth interfaces — in some cases by as much as a factor of five.
According to Lee, roughening of the interface between the bismuth and tellurium reduces the thermal conductivity of phonons more significantly than electron thermal conductivity (see image). “The overall effect is to increase the thermoelectric figure of merit,” says Lee.
Source: Tokyo Institute of Technology
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