Monday, October 08, 2012

Chemists get the blues

Just got back from judging the Chemistry World science writing competition. Makes me feel old, or perhaps just reminds me that I am. Anyway, many congratulations to the winner Chris Sinclair, whose article I believe will appear soon in Chemistry World. Meanwhile, here is my last Crucible column.
__________________________________________________

“Ultramarine blue is a colour illustrious, beautiful, and most perfect, beyond all other colours”, wrote the Italian artist Cennino Cennini in the late fourteenth century. He and his contemporaries adored this mineral pigment for its rich, deep lustre. But they didn’t use it much, at least not unless they had a particularly rich client, because it was so costly. As the name implies, it came from ‘over the seas’ – all the way from what is now Afghanistan, where mines in the remote region of Badakhshan were the only known source of the parent mineral, lapis lazuli, for centuries. Not only was ultramarine expensive to import, but it was laborious to make from the raw material, in a process of grinding and repeated washing that separated the blue colorant from impurities. So ultramarine could cost more than its weight in gold, and painters reserved it for the most precious parts of their altarpieces, especially the robes of the Virgin Mary.

Blue has always been a problem for artists. One of the first synthetic pigments, Egyptian blue (calcium copper silicate), was pale. The best mineral alternative to ultramarine, called azurite (hydrous copper carbonate), was more readily accessible but greenish rather than having ultramarine’s glorious purple-reddish tinge. Around 1704 a misconceived alchemical experiment yielded Prussian blue (iron ferrocyanate), which is blackish, prone to discolour, and decomposes to hydrogen cyanide under mildly acidic conditions. The discovery of cobalt blue (cobalt aluminate) in 1802, followed by a synthetic route to ultramarine in 1826, seemed to solve these problems of hue, stability and cost, but even these ‘artificial’ blues have drawbacks: cobalt is rather toxic, and ultramarine is sensitive to heat, light and acid, which limits its use in some commercial applications.

This is why the identification of a new inorganic blue pigment in 2009 looked so promising. Mas Subramanian and coworkers at Oregon State University found that trivalent manganese ions produce an intense blue colour, with the prized ‘reddish’ shade of ultramarine, when they occupy a trigonal bipyramidal site in metal oxides [1]. The researchers substituted Mn3+ for some indium ions in yttrium indium oxide (YInO3), forming a solid solution of YInO3 and YMnO3, which has a blue colour even though the two oxides themselves are white and black respectively. The depth of the colour varies from pale to virtually black as the manganese content is increased, although it is significantly blue even for only about 2 percent substitution. The researchers found that inserting manganese into other metal oxides with the same coordination geometry also offers strong blues. Meanwhile, similar substitutions of iron (III) and copper (II) generate bright orange and green pigments [2,3]. Those are traditionally less problematic, however, and while the materials may prove to have useful magnetic properties, it’s the blue that has attracted colour manufacturers.

Producing a commercially viable pigment is much more than a matter of finding a strongly coloured substance. It must be durable, for example. Although ultramarine, made industrially from cheap ingredients, is now available in quantities that would have staggered Titian and Michelangelo, it fades in direct sunlight because the sodalite framework is degraded and the sulphur chromophores are released and decompose – a process only recently understood [4]. This rules out many uses for exterior coatings. In contrast, the manganese compound has good thermal, chemical and light stability.

One of the key advantages of the YIn1-xMnxO3 compounds over traditional blues, however, is their strong reflectivity in the near-infrared region. Many other pigments, including cobalt blue and carbon black, have strong absorption bands here. This means that surfaces coated with these pigments heat up when exposed to strong sunlight. Building roofs coloured with such materials become extremely hot and can increase the demand of air conditioning in hot climates; instrument panels and steering wheels of cars may become almost too hot to touch. That’s why there is a big industrial demand for so-called ‘cool’ pigments, which retain their absorbance in the visible region but have low absorbance in the infrared. These can feel noticeably cooler when exposed to sunlight.

This aspect in particular has motivated the Ohio-based pigment company Shepherd Color to start exploring the commercial potential of the new blue pigment. One significant obstacle is the price of the indium oxide (In2O3) used as a starting material. This is high, because it is produced (mostly in China) primarily for the manufacture of the transparent conductive oxide indium titanium oxide for electronic displays and other optoelectronic applications. Those uses demand that the material be made with extremely high purity (around 99.999 percent), which drives up the cost. In principle, the low-purity In2O3 that would suffice for making Yin1-xMnxO3 could be considerably cheaper, but is not currently made at all as there is no market demand.

That’s why Subramanian and colleagues are now trying to find a way of eliminating the indium from their manganese compounds – to find a cheaper host that can place the metal atoms in the same coordination environment. If they succeed, it’s possible that we’ll see yet another revolution in the chemistry of the blues.

1. A. E. Smith et al., J. Am. Chem. Soc. 131, 17084-17086 (2009).
2. A. E. Smith, A. W. Sleight & M. A. Subramanian, Mater. Res. Bull. 46, 1-5 (2011). 1. A. E. Smith et al., J. Am. Chem. Soc. 131, 17084-17086 (2009).
3. P. Jiang, J. Li, A. W. Sleight & M. A. Subramanian, Inorg. Chem. 50, 5858-5860 (2011).
4. E. Del Federico et al., Inorg. Chem. 45, 1270-1276 (2006).

No comments:

Post a Comment

Note: Only a member of this blog may post a comment.