Oxygen
Electrolysis of water
Submitted by KingElz on 8 June 2008 - 3:21pm.I have a few questions for the electrolysis of water.
If 4 Litres of water is used and lets say for example a 9 volt battery is used. How much hydrogen and oxygen will be produced per second in terms of molecules?
Also if salt is added to the water to speed up the process, how much salt would be needed and would the products from the electrolysis change?
Please answer
Thank you
error in units
Submitted by Christopher Crawford on 16 January 2008 - 1:26pm.- The periodic table and the elements
- Actinium
- Aluminium
- Americium
- Antimony
- Argon
- Arsenic
- Astatine
- Barium
- Berkelium
- Beryllium
- Bismuth
- Bohrium
- Boron
- Bromine
- Cadmium
- Caesium
- Calcium
- Californium
- Carbon
- Cerium
- Chlorine
- Chromium
- Cobalt
- Copernicium
- Copper
- Curium
- Darmstadtium
- Dubnium
- Dysprosium
- Einsteinium
- Erbium
- Europium
- Fermium
- Fluorine
- Francium
- Gadolinium
- Gallium
- Germanium
- Gold
- Hafnium
- Hassium
- Helium
- Holmium
- Hydrogen
- Indium
- Iodine
- Iridium
- Iron
- Krypton
- Lanthanum
- Lawrencium
- Lead
- Lithium
- Lutetium
- Magnesium
- Manganese
- Meitnerium
- Mendelevium
- Mercury
- Molybdenum
- Neodymium
- Neon
- Neptunium
- Nickel
- Niobium
- Nitrogen
- Nobelium
- Osmium
- Oxygen
- Palladium
- Phosphorus
- Platinum
- Plutonium
- Polonium
- Potassium
- Praseodymium
- Promethium
- Protactinium
- Radium
- Radon
- Rhenium
- Rhodium
- Roentgenium
- Rubidium
- Ruthenium
- Rutherfordium
- Samarium
- Scandium
- Seaborgium
- Selenium
- Silicon
- Silver
- Sodium
- Strontium
- Sulphur
- Tantalum
- Technetium
- Tellurium
- Terbium
- Thallium
- Thorium
- Thulium
- Tin
- Titanium
- Tungsten
- Unbibium
- Unbiennium
- Unbihexium
- Unbinilium
- Unbioctium
- Unbipentium
- Unbiquadium
- Unbiseptium
- Unbitrium
- Unbiunium
- Unhexbium
- Unhexhexium
- Unhexnilium
- Unhexpentium
- Unhexquadium
- Unhexseptium
- Unhextrium
- Unhexunium
- Unpentbium
- Unpentennium
- Unpenthexium
- Unpentnilium
- Unpentoctium
- Unpentpentium
- Unpentquadium
- Unpentseptium
- Unpenttrium
- Unpentunium
- Unquadbium
- Unquadennium
- Unquadhexium
- Unquadnilium
- Unquadoctium
- Unquadpentium
- Unquadquadium
- Unquadseptium
- Unquadtrium
- Unquadunium
- Untribium
- Untriennium
- Untrihexium
- Untrinilium
- Untrioctium
- Untripentium
- Untriquadium
- Untriseptium
- Untritrium
- Untriunium
- Ununennium
- Ununhexium
- Ununoctium
- Ununpentium
- Ununquadium
- Ununseptium
- Ununtrium
- Uranium
- Vanadium
- Xenon
- Ytterbium
- Yttrium
- Zinc
- Zirconium
The units of resistivity don't come out right.
10^-8 Ohm * m
or
m Ohm * cm
the 'm' should be a 'mu', but unfortunately they both look the same in the latin alphabet.

isotopic abundance
Submitted by KhadijahA on 15 August 2007 - 7:59pm.Oxygen(atomic mass 15.9994 amu) has 3 isotopes with masses 15.9949 amu, 16.9993 amu, and 17.9992 amu. The abundance of the last isotope is .204%. Estimate the abundance of the other two isotopes.
I just need to know how to solve it bcuz im confused! thanks
The Great Global Warming Swindle
Submitted by Anonymous on 10 March 2007 - 4:57pm.Here in the UK, Channel 4 just screened an interesting documentary: The Great Global Warming Swindle. Good viewing and challenges what seems to have become the accepted view that global warming is caused by man-made CO2 emissions.

Hydrogen oxygen alloy
Submitted by WebElements on 29 October 2006 - 2:57pm.Researchers at the Carnegie Institution of Washington (Washington DC, USA) have managed to make a remarkable alloy of hydrogen and oxygen from water! They used X-rays to dissociate water at high pressure to form a solid mixture, that is, an alloy, of molecular oxygen (O2) and molecular hydrogen (H2).
The researchers placed some water under an extremely high pressure, about 170,000 atmospheres (17 Gigapascals), using a diamond anvil and then beamed high-energy X-rays at the water. Nearly all the water molecules split and reformed as a solid alloy of O2 and H2. The X-rays are key to cleaving the O—H bonds in water. Without it, the water remains as a high-pressure form of ice known as ice VII. Ice VII is one of at least 15 kinds of ice that exist under various high pressure and variable temperature conditions.

Record ozone loss over South Pole
Submitted by WebElements on 2 October 2006 - 9:28pm.Ozone measurements made by the European Space Agency Envisat satellite reveal the ozone loss of 40 million tons by 2 October in 2006 and that this exceeds the record ozone loss of about 39 million tons for the whole of 2000. The size of this year's ozone hole is 28 million square km.

The Ozone layer is a protective layer found about 25 kilometres above us mostly in the stratospheric stratum of the atmosphere that acts as a sunlight filter shielding life on Earth from harmful ultraviolet rays. Over the last few years the effective thickness of the ozone layer declined, increasing the risk of skin cancers, cataracts and harm to marine life. The thinning of the ozone layer is caused by the presence of pollutants in the atmosphere originating from, for instance, chlorofluorocarbons (CFCs), which have still not vanished from the air although banned under the 1987 Montreal Protocol.
"Such significant ozone loss requires very low temperatures in the stratosphere combined with sunlight. This year’s extreme loss of ozone can be explained by the temperatures above Antarctica reaching the lowest recorded in the area since 1979," European Space Agency Atmospheric Engineer Claus Zehner said.
Background Information
Ozone (O3) is another allotrope of oxygen. It is bent with a O-O-O angle of about 123° It is formed from electrical discharges or ultraviolet light acting on O2. It is an important component of the atmosphere (in total amounting to the equivalent of a layer about 3 mm thick at ordinary pressures and temperatures) which is vital in preventing harmful ultraviolet rays of the sun from reaching the earth's surface. Aerosols in the atmosphere have a detrimental effect on the ozone layer. Large holes in the ozone layer are forming over the polar regions and these are increasing in size annually. Paradoxically, ozone is toxic! Undiluted ozone is bluish in colour. Liquid ozone is bluish-black, and solid ozone is violet-black.
For chemical robots
IUPAC Name: ozone
Canonical SMILES: [O-][O+]=O
InChI: InChI=1/O3/c1-3-2
Links
- European Space Agency
- European Space Ozone story (2 October 2006)
- WebElements oxygen page

Hydrophobic Water
Submitted by David Bradley on 3 November 2005 - 7:44pm.That old truism about mixing oil and water can apply to water and water, according to researchers at Pacific Northwest National Laboratory in Washington State.
Read about his and more in the latest issue of Reactive Reports chemistry news

Special interests threat to ozone layer?
Submitted by WebElements on 26 March 2004 - 7:44pm.The BBC report here that special interests in a number of developed countries wish to to be allowed to continue using a bromine containing gas, methyl bromide, for various purposes such as crop fumigation. Methyl bromide is known to destroy ozone, O3, (an allotrope of oxygen, O2) and this is being debated at an international meeting in Canada. The Montreal Protocol does allow continued use of ozone-destroying gases for purposes agreed to be "critical", but is this really critical?

Water on Mars
Submitted by WebElements on 26 March 2004 - 7:44pm.A NASA press release claims that the Opportunity rover "has demonstrated some rocks on Mars probably formed as deposits at the bottom of a body of gently flowing saltwater." "Bedding patterns in some finely layered rocks indicate the sand-sized grains of sediment that eventually bonded together were shaped into ripples by water at least five centimeters (two inches) deep, possibly much deeper, and flowing at a speed of 10 to 50 centimeters (four to 20 inches) per second," said Dr. John Grotzinger, rover science-team member from the Massachusetts Institute of Technology, Cambridge, Mass.

Oxygen and Carbon Found in Atmosphere of an Extrasolar Planet
Submitted by WebElements on 3 February 2004 - 7:44pm.The Hubble telescope has identified oxygen and carbon in the atmosphere of an extrasolar planet for the first time. Here are the details. The oxygen and carbon are evaporating from a "hot jupiter" planet HD 209458b, orbiting a star lying 150 light-years from Earth. HD 209458b is only 4.3 million miles from its Sun-like star, completing an orbit in less than 4 days. This is not a sign of life!
