Author Archives: Maged

The Life Saving Reaction: Chapter II

As chemistry students we usually have to defend our choice of studying chemistry against the ceaseless attacks from friends and relatives. Therefore, beside boosting the food production and saving many lives, the Haber-Bosch process is a strong argument for how chemists can change the world. Simply the Haber-Bosch process produces ammonia from gaseous nitrogen and hydrogen under high temperature and pressure (500oC, 200 atm) . Since ammonia is the key component in chemical fertilizers, the Haber-Bosch process is responsible for the annual production of the food that keeps around 7 billion people alive nowadays.

But the story of the life saving reaction does not end here, a recent modification to the Haber-Bosch process is about to write a new chapter.

In may 2017, researchers from Waseda University and Nippon Shokubai Co. Ltd. achieved a highly efficient ammonia synthesis at low temperature, with the highest yield ever reported. In the paper that was published in Chemical Science, R. Manabe et al. used an Ru catalyst and applied electric field to achieve the reported synthesis. Although the activity of Ru catalyst for ammonia synthesis in mild conditions was reported in 1972, the rate of the reaction was very slow due to the high activation energy. Here is where the finding of the paper becomes interesting.

In the presence of an electric field and hydrogen or a compound containing hydrogen to carry the ions through the reaction, the activation energy can be significantly reduced. Instead of N2 and H2 dissociation followed by N-H bonds formation, protons add up to the N2 molecule and facilitates the N-N bond cleavage. In other words, in the presence of an electric field the reaction proceeds in an associative mechanism rather than a dissociative mechanism. The addition of the proton to the N2 molecule is an example of proton hopping, in which the proton keeps jumping from one molecule to an other.

Figure (1): The steps of the associative of mechanism in the presence of an electric field

As demonstrated in the figure (1), N2 first binds to the Ru catalyst through one N atom. A proton hops non binding N. Another proton hops to the binding N, and the nonbinding N associates to the metal center. The formation of N2H molecule in an electric field releases the energy that supports the endothermic cleavage of the N-N bond. However, the figure does not include the dissociation of the H2 molecule which is catalysed by the Ru. When ammonia is produced in acidic conditions, an ammonium ion is produced which carries out the hopping process which is the first step in the figure.

This news is significant for many reasons. First, the production of ammonia consumes more the 1% of the world’s produced energy. Saving this energy would have significant economic and environmental applications. Second, the use of ammonia as hydrogen carrier for Hydrogen fuel is currently studied, and low-energy synthesis of ammonia might be required soon. Finally but most importantly, you can have a crushing argument for how chemistry can change the world!

 

 

Pack Your Things, We are Going to Mars

Who said that we are going?

Around a year ago, the South African-born billionaire, Elon Musk, announced his plan for the colonilization of  Mars in a live video that went viral. Musk planned to land on Mars in the next decade and get it ready to host life by 2030. Since then, many have questioned the feasibility of the plan, including an esteemed astronaut who hypothesized that the project would stop as soon as Musk realizes the investment is not rewarding.

Are we even close?

According to researchers from the University of Lisbon and the University of Porto, we are. In their paper that was published on 18 October 2017, in the Journal Plasma Sources Science and Technology, Vasco Guerra et al. argue that Mars has nearly ideal conditions for CO2 dissociation to O2 and CO in Plasmas. As a result, production of O2 in Mars from CO2, which constitutes 95.9% of the Martian atmosphere, is possible.

Wait…what?

This is an illustration of a plasma lamp. When current is passed through plasma, amazing colours are observed. Uploaded by Joshua_Willson to Pixabay.com April 26, 2017

Basically, plasma is a state of matter where positive gas ions are surrounded by free negatively charged electrons. It can have interesting applications, such as plasma lamps. This state does not necessarily require high temperaturet. For example, non equilibrium low temperature plasma is a very interesting field of study and it is the type that Guerro describes as “the best media for CO2 dissociation”. There are several studies about how plasma assists the dissociation of pure COin the presence of a catalyst, usually TiO2. First, plasma supplies energy to drive the highly endothermic dissociation of CO2 through electron direct impact, in which an electron from the plasma transfers its energy to the CO2 molecule by collision, which aids the break of the C=O bond. Second, plasma adjusts the particles to the catalyst’s interface. Third, low temperature hinders the reverse reactions.

Why mars?

That is exactly Guerro’s argument. Guerro states that the atmospheric pressure of mars, 4.5 Torr, replaces the use of vacuum pumps that are necessary for the process on earth. Moreover, the average Martian atmospheric temperature, -63 oC, enhances the energy transfer from the plasma to the CO2. Also, Guerra mentions that the operation only requires as low as 20 W, which can be achieved on mars. Finally, the Martian atmosphere consists of 95.9% CO2, so O2 should be produced from this abundant source. Guerro says that the byproduct of this reaction, CO, can be used to fuel the return trip. In this way, the CO2 decomposition provides two benefits. Also, look at how beautiful it is:

An illustration of Mars, which is very beautiful. Uploaded by GooKingSword at pixabay.com

 

Personally, I used to think that if we can fix the atmosphere on Mars, then we should be able to fix it on Earth first. However, it turned out that Mars is helpful, but Earth is not. I started packing already…

By: Maged Hassan

Who Touched the Thermostat?

“This cannot be correct; God has the thermostat of the earth” said my 80 years old grandmother, in her last attempt to challenge the scientific consensus that the earth’s climate system is warming. As youthful scientists with scientific mindsets, you probably find her argument ridiculous. However, her argument is not entirely false. The earth has a thermostat, the Weathering Thermostat.

A group of scientists in University College London found the first evidence for the planetary thermostat that controls the temperature of the earth. The lead author, Pogge Von Strandmann, describes this process as a mechanism that prevents the temperature of the earth from going crazy.

The process by-which the earth stabilizes its temperature is simple, and have been known for many years; it is called “Weathering”. In this process, rainwater dissolves CO2 from the atmosphere, and combines it with rocks to form bicarbonates. Later, the bicarbonates drift to the ocean, where they react with calcium to be trapped in the form of limestone. Therefore, this process reduces the concentration of CO2, and the climate system cools down. However, if this reaction is slowed down, the CO2 builds up in the atmosphere, traps the heat that is coming from the sun, and the climate system warms up.

Limestone formations in the Torcal de Antequera. Photographer: Juan Fernández Source: http://www.flickr.com/photos/juanjaen/125055912/in/set-72057594101691764/

Still how does the weathering process control the temperature of the earth?

The weathering reaction is temperature dependent; the rate of the reaction increases as the temperature increases, using more CO2 from the atmosphere. But, at low temperatures, the reaction slows down to let the CO2 trap the heat coming from the sun.

If you already know this, you are probably yawning while thinking what is new?

This process had been hypothesized without real evidence. But according to the new study that was published in June 2017, in the journal Geochemical Perspectives Letters, authors have used Li isotopes to monitor the weathering process during the end of the glacial period. Their findings show a decline in the weathering of silicate rocks during the period when the climate system warmed and the ice age ended.

The team chose the Li isotopes because it is solely related to the weathering of silicate rocks. This enhances the certainty that the lowered concentration of Li isotopes in ocean limestone indicates the decline of the weathering of silicate rocks.

In conclusion, the earth had survived sever climate changes. However, fuel combustion, deforestation, and excessive use of pesticides introduce new challenges to the earth. In my opinion, as temperature rises, new natural reactions will be kinetically and thermodynamically afforded, and will reduce the concentration of CO2 in the atmosphere, exactly as weathering does. On the other hand, in her BBC article, Vivien Cumming argues that by the end of this century temperature will rise 4 celsius degrees, a number that she considers to be insane. As a young scientist and an inhabitant of the earth, your opinion on this subject is very valuable…do you have one yet?

By: Maged Hassan