Hydrogen
Might future fuel cells be nickel based?
There seems to be a possibility that nickel compounds might help in the electrolysis of water, the reaction at the centre of hydrogen fuel cells. Researchers at the Joseph Fourier University in Grenoble, and at the French Atomic Energy Commission in Gif-sur-Yvette and attached a nickel compound that mimics hydrogenase enzymes (catalysts) and attached it to the surface of carbon nanotubes. This maximises the catalyst's surface area. The resulting material was tested using a proton-exchange membrane and produced hydrogen from a sulphuric acid solution. The result is only 1% as efficient than commercial platinum catalysts but is stable under typical fuel cell conditions, justifying further study.1
- 1. From Hydrogenases to Noble Metal-Free Catalytic Nanomaterials for H2 Production and Uptake,
, Science, 12/2009, Volume 326, Issue 5958, p.1384 - 1387, (2009)
From Hydrogenases to Noble Metal-Free Catalytic Nanomaterials for H2 Production and Uptake
Abstract: Interconversion of water and hydrogen in unitized regenerative fuel cells is a promising energy storage framework for smoothing out the temporal fluctuations of solar and wind power. However, replacement of presently available platinum catalysts by lower-cost and more abundant materials is a requisite for this technology to become economically viable. Here, we show that the covalent attachment of a nickel bisdiphosphine–based mimic of the active site of hydrogenase enzymes onto multiwalled carbon nanotubes results in a high–surface area cathode material with high catalytic activity under the strongly acidic conditions required in proton exchange membrane technology. Hydrogen evolves from aqueous sulfuric acid solution with very low overvoltages (20 millivolts), and the catalyst exhibits exceptional stability (more than 100,000 turnovers). The same catalyst is also very efficient for hydrogen oxidation in this environment, exhibiting current densities similar to those observed for hydrogenase-based materials.
From Hydrogenases to Noble Metal-Free Catalytic Nanomaterials for H2 Production and Uptake, , Science, 12/2009, Volume 326, Issue 5958, p.1384 - 1387, (2009)A room-temperature titania-nanotube hydrogen sensor able to self-clean photoactively from environmental contamination
Abstract: described is a room-temperature hydrogen sensor comprised of a TiO2-nanotube array able to recover substantially from sensor poisoning through ultraviolet (UV) photocatalytic oxidation of the contaminating agent; in this case, various grades of motor oil. The TiO2 nanotubes comprising the sensor are a mixture of both anatase and rutile phases, having nominal dimensions of 22-nm inner diameter, 13.5-nm wall thickness, and 400-nm length, coated with a 10-nm-thick noncontinuous palladium layer. At 24°C, in response to 1000 ppm of hydrogen, the sensors show a fully reversible change in electrical resistance of approximately 175,000%. Cyclic voltammograms using a 1 N KOH electrolyte under 170 mW/cm2 UV illumination show, for both a clean and an oil-contaminated sensor, anodic current densities of approximately 28 mA/cm2 at 2.5 V. The open circuit oxidation potential shows a shift from 0.5 V to –0.97 V upon UV illumination.
A room-temperature titania-nanotube hydrogen sensor able to self-clean photoactively from environmental contamination, , Journal of Materials Research, 02/2004, Volume 19, Issue 2, p.628?634, (2004)The Group 1 elements
The Group 1 elements other than hydrogen are called the alkali metals. The Group 1 elements are:
The Group 1 metals are all highly reactive silvery metals that are so reactive to air and moisture that they must be stored under an inert atmosphere or oil. They are all soft and can be cut easily with a knife.
Hydrogen is usually placed at the top of the Group but is not a Group 1 metal.
The electronic configuration of the elements all consist of a lone s-electron outside an inner core of electron corresponding to the previous inert gas.
List of elements by atomic number
| Element name | Element symbol | Atomic number | ||||||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Hydrogen | H | 1 | ||||||||||||||||||||||||||||||
| Helium | He | 2 | ||||||||||||||||||||||||||||||
| Lithium | Li | 3 | ||||||||||||||||||||||||||||||
| Group | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | 1 | 2 | ||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Period | ||||||||||||||||||||||||||||||||
| 1 | 1 H |
2 He | ||||||||||||||||||||||||||||||
| 1 | 3 Li |
4 Be | ||||||||||||||||||||||||||||||
| 2 | 5 B |
6 C |
7 N |
8 O |
9 F |
10 Ne |
11 Na |
12 Mg |
||||||||||||||||||||||||
| 3 | 13 Al |
14 Si |
15 P |
16 S |
17 Cl |
18 Ar |
19 K |
20 Ca |
||||||||||||||||||||||||
| 4 | 21 Sc |
22 Ti |
23 V |
24 Cr |
25 Mn |
26 Fe |
27 Co |
28 Ni |
29 Cu |
30 Zn |
31 Ga |
32 Ge |
33 As |
34 Se |
35 Br |
36 Kr |
37 Rb |
38 Sr |
||||||||||||||
| 5 | 39 Y |
40 Zr |
41 Nb |
42 Mo |
43 Tc |
44 Ru |
45 Rh |
46 Pd |
47 Ag |
48 Cd |
49 In |
50 Sn |
51 Sb |
52 Te |
53 I |
54 Xe |
55 Cs |
56 Ba |
||||||||||||||
| 6 | 57 La |
58 Ce |
59 Pr |
60 Nd |
61 Pm |
62 Sm |
63 Eu |
64 Gd |
65 Tb |
66 Dy |
67 Ho |
68 Er |
69 Tm |
70 Yb |
71 Lu |
72 Hf |
73 Ta |
74 W |
75 Re |
76 Os |
77 Ir |
78 Pt |
79 Au |
80 Hg |
81 Tl |
82 Pb |
83 Bi |
84 Po |
85 At |
86 Rn |
87 Fr |
88 Ra |
| 7 | 89 Ac |
90 Th |
91 Pa |
92 U |
93 Np |
94 Pu |
95 Am |
96 Cm |
97 Bk |
98 Cf |
99 Es |
100 Fm |
101 Md |
102 No |
103 Lr |
104 Rf |
105 Db |
106 Sg |
107 Bh |
108 Hs |
109 Mt |
110 Ds |
111 Rg |
112 Cp |
113 Uut |
114 Uuq |
115 Uup |
116 Uuh |
117 Uus |
118 Uuo |
119 Uue |
120 Ubn |
List of elements sorted by symbol
List of elements sorted by name
Here is a list of the elements sorted by alphabetically by element name.
Sponsoring an element
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| Element | Popularity | Element | Popularity | Element | Popularity |
|---|---|---|---|---|---|
| actinium | 22 | holmium | 14 | rhodium | 21 |
| aluminium | 80 | hydrogen | 100 | rubidium | 25 |
| americium | 18 | indium | 25 | ruthenium | 22 |
| antimony | 26 | iodine | 39 | rutherfordium | 12 |
| argon | 41 | iridium | 23 | samarium | 15 |
| arsenic | 42 | iron | 72 | scandium | 29 |
| astatine | 19 | krypton | 39 | seaborgium | 13 |
| barium | 31 | lanthanum | 18 | selenium | 28 |
| berkelium | 14 | lawrencium | 13 | silicon | 65 |
| beryllium | 45 | lead | 48 | silver | 68 |
| bismuth | 23 | lithium | 64 | sodium | 76 |
| bohrium | 12 | lutetium | 16 | strontium | 26 |
| boron | 54 | magnesium | 63 | sulphur | 57 |
| bromine | 33 | manganese | 35 | tantalum | 22 |
| cadmium | 24 | meitnerium | 12 | technetium | 21 |
| caesium | 27 | mendelevium | 12 | tellurium | 21 |
| calcium | 69 | mercury | 54 | terbium | 14 |
| californium | 17 | molybdenum | 29 | thallium | 21 |
| carbon | 82 | neodymium | 16 | thorium | 16 |
| cerium | 18 | neon | 61 | thulium | 13 |
| chlorine | 57 | neptunium | 16 | tin | 43 |
| chromium | 45 | nickel | 50 | titanium | 62 |
| cobalt | 42 | niobium | 23 | tungsten | 34 |
| copper | 71 | nitrogen | 69 | ununbium | 12 |
| curium | 14 | nobelium | 13 | ununhexium | 14 |
| dubnium | 12 | osmium | 22 | ununnilium | 12 |
| dysprosium | 15 | oxygen | 73 | ununoctium | 22 |
| einsteinium | 18 | palladium | 24 | ununpentium | 5 |
| erbium | 15 | phosphorus | 51 | ununquadium | 15 |
| europium | 17 | platinum | 57 | ununseptium | 5 |
| fermium | 11 | plutonium | 28 | ununtrium | 5 |
| fluorine | 45 | polonium | 19 | roentgenium | 13 |
| francium | 20 | potassium | 65 | uranium | 40 |
| gadolinium | 16 | praseodymium | 16 | vanadium | 31 |
| gallium | 30 | promethium | 13 | xenon | 30 |
| germanium | 30 | protactinium | 13 | ytterbium | 15 |
| gold | 76 | radium | 25 | yttrium | 21 |
| hafnium | 18 | radon | 25 | zinc | 53 |
| hassium | 11 | rhenium | 20 | zirconium | 27 |
| helium | 58 |
Element 112 (Uub) to become Copernicium, Cp
CoperniciumIn honour of scientist and astronomer Nicolaus Copernicus (1473-1543), the discovering team around Professor Sigurd Hofmann suggested the name copernicium with the element symbol Cp for the new element 112, discovered at the GSI Helmholtzzentrum für Schwerionenforschung (Center for Heavy Ion Research) in Darmstadt. It was Copernicus who discovered that the Earth orbits the Sun, thus paving the way for our modern view of the world. Thirteen years ago, element 112 was discovered by an international team of scientists at the GSI accelerator facility. A few weeks ago, the International Union of Pure and Applied Chemistry, IUPAC, officially confirmed their discovery. In around six months, IUPAC will officially endorse the new element's name. This period is set to allow the scientific community to discuss the suggested name copernicium before the IUPAC naming.
"After IUPAC officially recognized our discovery, we – that is all scientists involved in the discovery – agreed on proposing the name copernicium for the new element 112. We would like to honor an outstanding scientist, who changed our view of the world", says Sigurd Hofmann, head of the discovering team.
Copernicus was born 1473 in Torun; he died 1543 in Frombork, Poland. Working in the field of astronomy, he realized that the planets circle the Sun. His discovery refuted the then accepted belief that the Earth was the center of the universe. His finding was pivotal for the discovery of the gravitational force, which is responsible for the motion of the planets. It also led to the conclusion that the stars are incredibly far away and the universe inconceivably large, as the size and position of the stars does not change even though the Earth is moving. Furthermore, the new world view inspired by Copernicus had an impact on the human self-concept in theology and philosophy: humankind could no longer be seen as the center of the world.
With its planets revolving around the Sun on different orbits, the solar system is also a model for other physical systems. The structure of an atom is like a microcosm: its electrons orbit the atomic nucleus like the planets orbit the Sun. Exactly 112 electrons circle the atomic nucleus in an atom of the new element "copernicium".
Element 112 is the heaviest element in the periodic table, 277 times heavier than hydrogen. It is produced by a nuclear fusion, when bombarding zinc ions onto a lead target. As the element already decays after a split second, its existence can only be proved with the help of extremely fast and sensitive analysis methods. Twenty-one scientists from Germany, Finland, Russia and Slovakia have been involved in the experiments that led to the discovery of element 112.
Since 1981, GSI accelerator experiments have yielded the discovery of six chemical elements, which carry the atomic numbers 107 to 112. The discovering teams at GSI already named five of them: element 107 is called bohrium, element 108 hassium, element 109 meitnerium, element 110 darmstadtium, and element 111 is named roentgenium.
WebElements: the periodic table on the WWW [http://www.webelements.com/]
Copyright 1993-2011 Mark Winter [The University of Sheffield and WebElements Ltd, UK]. All rights reserved.