Category Chemistry/Nanotechnology

Artificial Photosynthesis Steps into the Light

1. Scientists at Rice University and the University of Houston created a catalyst from three elements – iron, manganese and phosphorus – and then coated it evenly onto an array of titanium dioxide nanorods to create a highly efficient photoanode for artificial photosynthesis. Click on the image for a larger version. Courtesy of the Whitmire Research Group 2. A photo shows an array of titanium dioxide nanorods with an even coating of an iron, manganese and phosphorus catalyst. The combination developed by scientists at Rice University and the University of Houston is a highly efficient photoanode for artificial photosynthesis. Click on the image for a larger version. Courtesy of the Whitmire Research Group

1. Scientists at Rice University and the University of Houston created a catalyst from three elements – iron, manganese and phosphorus – and then coated it evenly onto an array of titanium dioxide nanorods to create a highly efficient photoanode for artificial photosynthesis. Click on the image for a larger version. Courtesy of the Whitmire Research Group. 2. (inset) Array of titanium dioxide nanorods with an even coating of an iron, manganese and phosphorus catalyst. The combination developed by scientists at Rice University and the University of Houston is a highly efficient photoanode for artificial photosynthesis.

Lab turns transition metals into practical catalyst for solar, other applications...

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Astronomers Identify Purest, most Massive Brown Dwarf

An artist's impression of the new pure and massive brown dwarf. Credit: John Pinfield

An artist’s impression of the new pure and massive brown dwarf. Credit: John Pinfield

An international team has identified a record breaking brown dwarf (a star too small for nuclear fusion) with the ‘purest’ composition and the highest mass yet known. The object, SDSS J0104+1535, is a member of the so-called halo – the outermost reaches – of our Galaxy, made up of the most ancient stars. Brown dwarfs are intermediate between planets and fully-fledged stars. Their mass is too small for full nuclear fusion of hydrogen to helium (with a consequent release of energy) to take place, but they are usually significantly more massive than planets.

Located 750 light years away in the constellation of Pisces, SDSS J0104+1535 is made of gas that is around 250 times purer than the Sun, so consists of ...

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Chemists ID Catalytic ‘Key’ for converting CO2 to Methanol

Brookhaven scientists identified how a zinc/copper (Zn/Cu) catalyst transforms carbon dioxide (two red and one grey balls) and hydrogen (two white balls) to methanol (one grey, one red, and four white balls), a potential fuel. Under reaction conditions, Zn/Cu transforms to ZnO/Cu, where the interface between the ZnO and Cu provides the active sites that allow the formation of methanol.

Brookhaven scientists identified how a zinc/copper (Zn/Cu) catalyst transforms carbon dioxide (two red and one grey balls) and hydrogen (two white balls) to methanol (one grey, one red, and four white balls), a potential fuel. Under reaction conditions, Zn/Cu transforms to ZnO/Cu, where the interface between the ZnO and Cu provides the active sites that allow the formation of methanol.

Results will guide design of improved catalysts for transforming pollutant to useful chemicals. Capturing CO2 and converting it to useful chemicals such as methanol could reduce both pollution and our dependence on petroleum products. So scientists are intensely interested in the catalysts that facilitate such chemical conversions...

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Tracing Aromatic Molecules in the early Universe

In this study, astronomers used data from the Keck and Spitzer telescopes to trace the star forming and dusty regions of galaxies at about 10 billion years ago. The picture in the background shows the GOODS field, one of the five regions in the sky that was observed for this study. Credit: Mario De Leo-Winkler with images from the Spitzer Space Telescope, NASA, ESA and the Hubble Heritage team.

In this study, astronomers used data from the Keck and Spitzer telescopes to trace the star forming and dusty regions of galaxies at about 10 billion years ago. The picture in the background shows the GOODS field, one of the five regions in the sky that was observed for this study. Credit: Mario De Leo-Winkler with images from the Spitzer Space Telescope, NASA, ESA and the Hubble Heritage team.

A molecule found in car engine exhaust fumes that is thought to have contributed to the origin of life on Earth has made astronomers heavily underestimate the amount of stars that were forming in the early Universe, a University of California, Riverside-led study has found. That molecule is called polycyclic aromatic hydrocarbon (PAH). On Earth it is also found in coal and tar...

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