The James M. DuPont Meteorite Collection - E. Anders, E. "On the Chemical Evolution of carbonaceous chondrites." Geochim. Cosmochim. Acta 26, 1085-1114, (1962). 23. K. Tomeoka and P. R. Buseck, "Matrix mineralogy of the Orgueil C1 carbonaceous chondrite." Geochim. Cosmochim. Acta 52, 1627-1640, (1988). 24. R.N. Clayton, "Carbon isotope abundances in meteoritic carbonates." Science, 140, 192-193, (1963). 25. P. Ehrenfreund, D. P. Glavin, O. Botta, G. Cooper and J. Bada, "Extraterrestrial amino acids in Orgueil and Ivuna: Tracing the parent body of CI type carbonaceous chondrites." Proc. Natl. A cad. Acad. Sci., 98, 2138-2141 (2001). 26. M. Berthelot, "Sur la Matiere charboneuse des meteorites." Compt. Rend. Acad. Sci., 67, 849, 1868. 27. K.A. Kvenvolden. J. G. Lawless, K. Pering,

The James M. DuPont Meteorite Collection - limonite-Fe203" Theremaining nH20). 13.9% found was tobecomprised elemental of Sulfur, andinsolublerganic atter"kerogen"). studies showed o m ( Other 22'23 thatOrgueil alsocontains several minormineral species including:ammonium salts,anhydrite-CaSO4; calcite-CaCo3; serpentine-(Mg6Si4Ol0(OH)8+FezSiO trevorite-NiFe204; pyrrhotite-(Fe,Ni)0.9S; olivine-(Mg2SiO4+Fe2SiO4); and pyroxene-(Mg Ca silicates). Fe 22"23 Claytonfound 24 theOrgueil carbonates tohave - +60%0 hich 813C w clearly established tobeof extraterrestrial them origin. he values f-7 to-9 %0 T 513C o forthe_-alanine intheOrgueil meteorite falloutside also therange fterrestrial o values (typically20to-30%0)

The James M. DuPont Meteorite Collection - C isotopic composition of these carbonates [5], our results imply that there was only minimal isotopic fractionation of the atmosphere on Mars, at least within the last 1.39 Ga. Finally, the similarity of this carbonate formation age to the 1.3-Ga crystallization age for some of the other SNC meteorites could be indicative of a particularly active phase of magmatism and hydrothermal activity on Mars at that time. Although this can only be regarded as speculative at this point, it does raise some interesting possibilities regarding the magmatic history of this planet. References: [1] Jagoutz E. et al. (1994) Meteoritics, 29, 478-479. [2] Nyquist L. E. et al. (1995) LPS XXVI, 1065-1066. [3] Mittlefehldt D. W. (1994) Meteoritics, 29, 214-221. [4] Treiman A. H. (1995)

The James M. DuPont Meteorite Collection -with the weathering grade and the terrestrial age of the meteorite. The CO2 release in this temperature region correlates with the H2O release indicating that the carbonate-containing compound could have been formed through the adsorption of atmospheric CO2 onto the surface of the finely-crystalline oxyhydroxides and subsequently incorporated into the crystal structure. Between 500 degrees C and 1000 degrees C the CO2 release is strongly determined by the contamination with carbonates directly transferred from the ground to the meteorite. This contamination is not simply related to the degree of weathering, but also depends on local soil type. The amount of released H2O and CO2 appears to have a maximum at intermediate positions.

The James M. DuPont Meteorite Collection - contains such materials. Carr et al. [8] and Grady et al. [9] reported releases of CO2 from SNC meteorites and Semarkona (LL3.0) respectively after treatment with acid and attributed this to carbonate, a result corroborated by subsequent petrologic investigations [10,11]. The latter is particularly relevant since it is an unequilibrated ordinary chondrite. The delta18O of the putative carbonates in Parnallee (+26.9 to +3 1.1 per mil for calcite, +26.0 to +31.4 per mil for dolomite) is up to 20 per mil heavier than values determined previously in unequilibrated ordinary chondrites [12] but falls within the range of data reported for CI, CM, and CR meteorites by Wright et al. [13]. The delta17O of the calcite was found to fall between +18.6 and 29.0 per mil. Taken

The James M. DuPont Meteorite Collection - of Mars from the heavy bombardment era. New O isotope data on CI olivine grains show that they form two distinct populations, an iron-poor forsteritic population lying on the CAI line and an iron-rich population lying, with considerable scatter, on the Terrestrial or MM material fractionation lines [4] in the vicinity of delta(18)O = +6 per mil. Oxygen-isotope data for carbonates found in MMs show they are highly fractionated and lie between delta(18)O = 20 per mil and 30 per mil where, unfortunately, (17)O data are not available [5]. Assuming that the MM carbonates lie on the MM fraction line, and noting that ranges of fractionation lines are defined by their extremes, the newly considered data gives an MM fraction line extending to delta(18)O = 30 and

Pabegi #1 gagrzeleba =D.

The Carbon Collective and it’s a movement, a community and a network of environmentally-friendly folks just like you who want to do something to make the earth a healthier place. The idea behind it is simple: the more friends that join, better results for the planet, and more income for you! It’s an easy & fun way to reduce HUGE quantities of carbon through the power of friendship alone, and it’s totally free of charge for everyone!

"60 seconds with... " Video Statement by Chris Davies on the carbone capture and storage, one of the climate packages that were voted this week (6-12/10/2008) in the Enviroment Commitee at the European Parliament. [60 Seconds] [Statements] [Language EN] 081009-ALDESTATEMENT-Chris_Davies-on-carbone_capture

Alien Zlog and his side kick Asbo are back and on the look out for our carbon footprints. They find the ‘higher ups’ frown upon the footprints of the ‘lower downs’, especially when they are ‘h...

NASA's Phoenix Mars Lander has detected snow falling from Martian clouds. Spacecraft soil experiments also have provided evidence of past interaction between minerals and liquid water, processes that occur on Earth.

A laser instrument designed to gather knowledge of how the atmosphere and surface interact on Mars has detected snow from clouds about 4 kilometers (2.5 miles) above the spacecraft's landing site. Data show the snow vaporizing before reaching the ground.

"Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University, Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be looking for signs that the snow may even reach the ground."

Phoenix experiments also yielded clues pointing to calcium carbonate, the main composition of chalk, and particles that could be clay. Most carbonates and clays on Earth form only in the presence of liquid water.

"We are still collecting data and have lots of analysis ahead, but we are making good progress on the big questions we set out for ourselves," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Since landing on May 25, Phoenix already has confirmed that a hard subsurface layer at its far-northern site contains water-ice. Determining whether that ice ever thaws would help answer whether the environment there has been favorable for life, a key aim of the mission.

The evidence for calcium carbonate in soil samples from trenches dug by the Phoenix robotic arm comes from two laboratory instruments called the Thermal and Evolved Gas Analyzer, or TEGA, and the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer, or MECA.

"We have found carbonate," said William Boynton of the University of Arizona, lead scientist for the TEGA. "This points toward episodes of interaction with water in the past."

The TEGA evidence for calcium carbonate came from a high-temperature release of carbon dioxide from soil samples. The temperature of the release matches a temperature known to decompose calcium carbonate and release carbon dioxide gas, which was identified by the instrument's mass spectrometer.

The MECA evidence came from a buffering effect characteristic of calcium carbonate assessed in wet chemistry analysis of the soil. The measured concentration of calcium was exactly what would be expected for a solution buffered by calcium carbonate.

Both TEGA, and the microscopy part of MECA, have turned up hints of a clay-like substance. "We are seeing smooth-surfaced, platy particles with the atomic-force microscope, not inconsistent with the appearance of clay particles," said Michael Hecht, MECA lead scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The Phoenix mission, originally planned for three months on Mars, now is in its fifth month. However, it faces a decline in solar energy that is expected to curtail and then end the lander's activities before the end of the year. Before power ceases, the Phoenix team will attempt to activate a microphone on the lander to possibly capture sounds on Mars.

"For nearly three months after landing, the sun never went below the horizon at our landing site," said Barry Goldstein, JPL Phoenix project manager. "Now it is gone for more than four hours each night, and the output from our solar panels is dropping each week. Before the end of October, there won't be enough energy to keep using the robotic arm."

NASA's Phoenix Mars Lander has detected snow falling from Martian clouds. Spacecraft soil experiments also have provided evidence of past interaction between minerals and liquid water, processes that occur on Earth.

A laser instrument designed to gather knowledge of how the atmosphere and surface interact on Mars has detected snow from clouds about 4 kilometers (2.5 miles) above the spacecraft's landing site. Data show the snow vaporizing before reaching the ground.

"Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University, Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be looking for signs that the snow may even reach the ground."

Phoenix experiments also yielded clues pointing to calcium carbonate, the main composition of chalk, and particles that could be clay. Most carbonates and clays on Earth form only in the presence of liquid water.

"We are still collecting data and have lots of analysis ahead, but we are making good progress on the big questions we set out for ourselves," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Since landing on May 25, Phoenix already has confirmed that a hard subsurface layer at its far-northern site contains water-ice. Determining whether that ice ever thaws would help answer whether the environment there has been favorable for life, a key aim of the mission.

The evidence for calcium carbonate in soil samples from trenches dug by the Phoenix robotic arm comes from two laboratory instruments called the Thermal and Evolved Gas Analyzer, or TEGA, and the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer, or MECA.

"We have found carbonate," said William Boynton of the University of Arizona, lead scientist for the TEGA. "This points toward episodes of interaction with water in the past."

The TEGA evidence for calcium carbonate came from a high-temperature release of carbon dioxide from soil samples. The temperature of the release matches a temperature known to decompose calcium carbonate and release carbon dioxide gas, which was identified by the instrument's mass spectrometer.

The MECA evidence came from a buffering effect characteristic of calcium carbonate assessed in wet chemistry analysis of the soil. The measured concentration of calcium was exactly what would be expected for a solution buffered by calcium carbonate.

Both TEGA, and the microscopy part of MECA, have turned up hints of a clay-like substance. "We are seeing smooth-surfaced, platy particles with the atomic-force microscope, not inconsistent with the appearance of clay particles," said Michael Hecht, MECA lead scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The Phoenix mission, originally planned for three months on Mars, now is in its fifth month. However, it faces a decline in solar energy that is expected to curtail and then end the lander's activities before the end of the year. Before power ceases, the Phoenix team will attempt to activate a microphone on the lander to possibly capture sounds on Mars.

"For nearly three months after landing, the sun never went below the horizon at our landing site," said Barry Goldstein, JPL Phoenix project manager. "Now it is gone for more than four hours each night, and the output from our solar panels is dropping each week. Before the end of October, there won't be enough energy to keep using the robotic arm."

NASA's Phoenix Mars Lander has detected snow falling from Martian clouds. Spacecraft soil experiments also have provided evidence of past interaction between minerals and liquid water, processes that occur on Earth.

A laser instrument designed to gather knowledge of how the atmosphere and surface interact on Mars has detected snow from clouds about 4 kilometers (2.5 miles) above the spacecraft's landing site. Data show the snow vaporizing before reaching the ground.

"Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University, Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be looking for signs that the snow may even reach the ground."

Phoenix experiments also yielded clues pointing to calcium carbonate, the main composition of chalk, and particles that could be clay. Most carbonates and clays on Earth form only in the presence of liquid water.

"We are still collecting data and have lots of analysis ahead, but we are making good progress on the big questions we set out for ourselves," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Since landing on May 25, Phoenix already has confirmed that a hard subsurface layer at its far-northern site contains water-ice. Determining whether that ice ever thaws would help answer whether the environment there has been favorable for life, a key aim of the mission.

The evidence for calcium carbonate in soil samples from trenches dug by the Phoenix robotic arm comes from two laboratory instruments called the Thermal and Evolved Gas Analyzer, or TEGA, and the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer, or MECA.

"We have found carbonate," said William Boynton of the University of Arizona, lead scientist for the TEGA. "This points toward episodes of interaction with water in the past."

The TEGA evidence for calcium carbonate came from a high-temperature release of carbon dioxide from soil samples. The temperature of the release matches a temperature known to decompose calcium carbonate and release carbon dioxide gas, which was identified by the instrument's mass spectrometer.

The MECA evidence came from a buffering effect characteristic of calcium carbonate assessed in wet chemistry analysis of the soil. The measured concentration of calcium was exactly what would be expected for a solution buffered by calcium carbonate.

Both TEGA, and the microscopy part of MECA, have turned up hints of a clay-like substance. "We are seeing smooth-surfaced, platy particles with the atomic-force microscope, not inconsistent with the appearance of clay particles," said Michael Hecht, MECA lead scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The Phoenix mission, originally planned for three months on Mars, now is in its fifth month. However, it faces a decline in solar energy that is expected to curtail and then end the lander's activities before the end of the year. Before power ceases, the Phoenix team will attempt to activate a microphone on the lander to possibly capture sounds on Mars.

"For nearly three months after landing, the sun never went below the horizon at our landing site," said Barry Goldstein, JPL Phoenix project manager. "Now it is gone for more than four hours each night, and the output from our solar panels is dropping each week. Before the end of October, there won't be enough energy to keep using the robotic arm."

NASA's Phoenix Mars Lander has detected snow falling from Martian clouds. Spacecraft soil experiments also have provided evidence of past interaction between minerals and liquid water, processes that occur on Earth.

A laser instrument designed to gather knowledge of how the atmosphere and surface interact on Mars has detected snow from clouds about 4 kilometers (2.5 miles) above the spacecraft's landing site. Data show the snow vaporizing before reaching the ground.

"Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University, Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be looking for signs that the snow may even reach the ground."

Phoenix experiments also yielded clues pointing to calcium carbonate, the main composition of chalk, and particles that could be clay. Most carbonates and clays on Earth form only in the presence of liquid water.

"We are still collecting data and have lots of analysis ahead, but we are making good progress on the big questions we set out for ourselves," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Since landing on May 25, Phoenix already has confirmed that a hard subsurface layer at its far-northern site contains water-ice. Determining whether that ice ever thaws would help answer whether the environment there has been favorable for life, a key aim of the mission.

The evidence for calcium carbonate in soil samples from trenches dug by the Phoenix robotic arm comes from two laboratory instruments called the Thermal and Evolved Gas Analyzer, or TEGA, and the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer, or MECA.

"We have found carbonate," said William Boynton of the University of Arizona, lead scientist for the TEGA. "This points toward episodes of interaction with water in the past."

The TEGA evidence for calcium carbonate came from a high-temperature release of carbon dioxide from soil samples. The temperature of the release matches a temperature known to decompose calcium carbonate and release carbon dioxide gas, which was identified by the instrument's mass spectrometer.

The MECA evidence came from a buffering effect characteristic of calcium carbonate assessed in wet chemistry analysis of the soil. The measured concentration of calcium was exactly what would be expected for a solution buffered by calcium carbonate.

Both TEGA, and the microscopy part of MECA, have turned up hints of a clay-like substance. "We are seeing smooth-surfaced, platy particles with the atomic-force microscope, not inconsistent with the appearance of clay particles," said Michael Hecht, MECA lead scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The Phoenix mission, originally planned for three months on Mars, now is in its fifth month. However, it faces a decline in solar energy that is expected to curtail and then end the lander's activities before the end of the year. Before power ceases, the Phoenix team will attempt to activate a microphone on the lander to possibly capture sounds on Mars.

"For nearly three months after landing, the sun never went below the horizon at our landing site," said Barry Goldstein, JPL Phoenix project manager. "Now it is gone for more than four hours each night, and the output from our solar panels is dropping each week. Before the end of October, there won't be enough energy to keep using the robotic arm."

Home-brewing Blickman Beer Gun force carbonates a bottle without the sediment. Learn more about how the Blickman Beer Gun works with tips from a master brewer in this free video on beverage making.

Clip du titre THE NEWS de CARBON/SILICON réalisé par CALLICORE. Sortie de l'album de CARBON/SILICON, "THE LAST POST" le 3 Novembre 2008 !

http://carbon-copy-pro.info Join Eric Su Jay Kubassek Mike Dillard & Aaron Parkinson In Carbon Copy Pro or CarbonCopyPro To Make Money Online Real internet home based business opportunity not a scam.

Field Trip to Bahamas, Part 1: Dive
clips of sites around Nassau including
Blue Hole, Shark Wall and Shark Arena

hey ya'll, this is a review of need for speed carbon reviewed by me. enjoy.

All 5 Parts of - Mars Rising-The Search For Life
http://www.youtube.com/view_play_list?p=0215E3B99C9C24BA


PART SIX - Is there life on Mars? Scientists in North America are combing the most barren places on Earth to search out bacteria, amino acids or carbonates that might offer clues. What if Mars has its own independently created life forms which are deadly to humans? Researchers on the Arctic's frigid Devon Island, British Columbia's Pavilion Lake, Chile's Atacama Desert and caves in New Mexico offer compelling chronicles.

William Shatner narrates "Mars Rising"

All 5 Parts of - Mars Rising - The Search For Life http://www.youtube.com/view_play_list?p=0215E3B99C9C24BA


PART SIX - Is there life on Mars? Scientists in North America are combing the most barren places on Earth to search out bacteria, amino acids or carbonates that might offer clues. What if Mars has its own independently created life forms which are deadly to humans? Researchers on the Arctic's frigid Devon Island, British Columbia's Pavilion Lake, Chile's Atacama Desert and caves in New Mexico offer compelling chronicles.

William Shatner narrates "Mars Rising"

All 5 Parts of - Mars Rising - The Search For Life
http://www.youtube.com/view_play_list?p=0215E3B99C9C24BA


PART SIX - Is there life on Mars? Scientists in North America are combing the most barren places on Earth to search out bacteria, amino acids or carbonates that might offer clues. What if Mars has its own independently created life forms which are deadly to humans? Researchers on the Arctic's frigid Devon Island, British Columbia's Pavilion Lake, Chile's Atacama Desert and caves in New Mexico offer compelling chronicles.

William Shatner narrates "Mars Rising"

An inside look at home business at it extreme. This is a money making entreprenuer based look at what it takes to make hundreds of thousands of dollars. This business opportunity is one of a kind. Serious entrepreneurs shold take advantage now!

http://www.WhoisAaronHill.com Is Carbon Copy Pro a Scam? This program doesn't work as well as they would like you to think. The bottom line is, if you don’t know how to effectively market a business, then you will find it very difficult to succeed with this company. Go to: http://www.WhoisAaronHill.com to schedule an interview. A little background on me, I have been involved with several home businesses and mlms in the past 6 years, I was tired of struggling, buying leads, putting out flyers, going to my friends and family and I told myself I was not going to do that any more. Now I have created a system and found a new business model that is working like crazy, and I am teaching all of my students my little known secrets on how to market their business and generate free targeted traffic & free leads to their business every single day. I am currently taking on 10 new students a week, and I do want to let you know that I don’t take on everyone, I do turn people down. So go to ...

Outspoken Brit Ann McLaren gives you the lowdown on Carbon Copy Pro.

Polycarbonate was discovered in 1898 when a German chemist named Einhorn observed the formation of an insoluble, infusible solid, while preparing cyclic carbonates by reacting hydroquinone with phosgene. It wasn't until 1953 that Bayer laboratories produced linear thermoplastic Polycarbonate of high molecular weight. In 1957 Bayer and General Electric announced independent development of polycarbonate and in the summer of 1960 both companies began end use production. Today, approximately 75% of the Polycarbonate market is held by SABIC Innovative Plastics (formerly known as General Electric) and Bayer Material Science.

Polycarbonate plastic is a lightweight, high-performance plastic that possesses a unique balance of toughness, dimensional stability, optical clarity, high heat resistance and excellent electrical resistance. Because of these attributes, polycarbonate is used in a wide variety of common products including electronic media like CDs and DVDs, electronic equipment, automobiles, construction glazing, sports safety equipment and medical devices.

The Gellért Baths and Hotel were built in 1918, although there had once been Turkish baths on the site, and in the Middle Ages a hospital. In 1927 the Baths were extended to include the wave pool, and the effervescent bath was added in 1934. With its immaculately preserved Art Nouveau interior, including colourful mosaics, marble columns, stained glass windows and statues, this is without doubt the most beautiful bathing complex in Budapest.
The Gellért Baths were an immediate international success, and were even the scene of an early political scandal. In 1931 a visiting black doctor, Dr. Ramon Costello (who happened to be Cuban), was refused to the Baths on the grounds there were some white American visitors there, and, since there was still racial segregation in America, they objected to his presence. Costello took the matter to the City Council, and they found in his favour.
Water temperatures: 79-100°F (26-38°C). Pools: open air wave pool, thermal pool and children's pool, indoor swimming-effervescent pool and nine medicinal pools.
Water mineral content: thermal water containing nitrates, calcium-magnesium-hydroge n-carbonates and sulphate-chlorides, as well as fluoride ions in significant quantities. Opening times: Weekdays 6.0 a.m. -- 7.0 p.m. Weekends 6.0 a.m. -- 5.0 p.m.

http://spasbudapest.com
http://www.budapestinfo.hu/en

Yeh Hai Jalwa

We asked dozens of everyday people to tell us what they thought a carbon offset was. For more information, visit KeysToGreen.com.

The Dads offer a few suggestions on how to clean up the environmental nightmare that is child rearing. Are carbon offsets a good deal for the minivan and SUV crowd? But what could possibly be funny about global warming? Two words: methane recapture.

try to get seem speed ^_^ hhhh

Note:

Appearance - carbonates are powdery
Cheating test - use acid to test for effeversence

Ugh!! It took us forever to finally get this down. We spent like 3 days on the whole video, but this was all that survived through the smoke and the wreckage.

got the lyrics faster than i thought got the lyrics faster than i thought
Solubility Song: Rules for Solubility (To the Tune of 99 Bottles of Beer)

Potassium, sodium and ammonium salts,
Whatever they may be
Can always be depended on For solubility.

When asked about the nitrates,
The answer's always clear,
They each and all are soluble,
Is all we want to hear.

Most every chloride's soluble,
At least we've always read,
Save silver, mercurous mercury,
And (slightly) chloride of lead.

Every single sulfate,
Is soluble, 'tis said,
'Cept barium and calcium
And strontium and lead.

Hydroxide of metal's won't dissolve,
That is, all but three.
Potassium, sodium and ammonium
Dissolve quit readily.

And then you must remember
That you must not forgit:
Calcium and barium
Dissolve a little bit.

Metallic sulfide will not mix
With water it is true
But if you read the two above
You'll found out which ones do.

The carbonates, insoluble,
It's lucky that it's so,
Or else our marble buildings
Would melt away like snow.

first zero-carbon, zero-waste city in Abu Dhabi. Named Masdar City

Carbon Offset Programs:Travel with a Carbon Offset-Travel Video Alert Have a good trip…and don‘t worry that your flight is spewing tons of carbon dioxide into the atmosphere. Carbon Offset programs are new and making it possible to travel with no carbon footprint. Travel Carbon neutral. More people are flying than ever and the C02 emitted by planes at high altitudes does more harm to the atmosphere than emission from cars, so no one can travel guilt free these days? However, Carbon Offset programs let travelers offset the gas they pass The programs offered on the web and by travel giants like Orbitz and Travelocity calculate how much C02 you‘re responsible for while you’re flying the friendly skies They give you a dollar figure to pay to offset your carbon footprint… and they’ll plant a tree with the money or back a wind power program

If you want to download this video then go to this site: http://www.downloadvideos.co.nr .Magnesium is placed in a cavity in a block of dry ice. The magnesium is ignited and covered by another block of dry ice. The magnesium continues to glow, due to its reaction with carbon dioxide. This demonstration is difficult to set up.

My name is pepsious maximus defender of the carbonates, alegence to the diet pepsicous i need 1,000 pounds instead of 2 chickens and a goat to fight of gasious burpicus .... for maximus day. www.maxyourlife.co.uk

n4s carbon, ingame footage Seen On: WWW.ACEGAMER.BE :: GAMES & BABES ::