Meinecke et al. Turbulent amplification of magnetic fields in laboratory laser-produced shock waves, June 2014, Nature Physics.

A supernova is the explosion of a massive star which releases a burst of radiation that can be as bright as 10 billion suns. Such a massive amount of radiation can shine throughout the entire universe for several light-years. Supernovas are triggered either when the fuel within a star ignites or when a star’s core collapses under extreme gravitational forces. Supernovas have already taught us very important lessons about the history of the universe. For example, these explosions have provided solid evidence that the universe is expanding. Supernovas can also tell us a lot about how old stars die and how new stars are born. When a star goes through a supernova explosion, it leaves behind a skeleton made of expanding dust and gas that scientists call a remnant. These star-remnants spread around space. They might end up on earth or other planets, or they could form the energy source of a new star. Since the best way to understand supernovas is to actually explode a star, researchers recently developed a technique to simulate small-scale supernovas in a lab environment. To do this, scientists used lasers that are 60,000 billion times more powerful than a laser pointer. They focused the laser beams on a thin carbon rod inside a gas-filled chamber. The lasers heated the chamber to over 1 million degrees Celsius, which caused the carbon rod to explode and expand out through the low density gas – just like how exploding stars speed through space. The experiment revealed that as the blast passes through the grid, it becomes irregular and turbulent. They also noticed that the magnetic field was dramatically higher within the grid than without, suggesting that the magnetic field was amplified by the generated turbulence. The supernova system developed in this study holds the possibility of helping us better understand how the universe was formed and evolved, and could provide some insight into how magnetic fields were first created.

Young blood: The fountain of youth?

Villeda SA et al. Young blood reverses age-related impairments in cognitive function and synaptic plasticity in mice. June 2014, Nature Medicine.
Sinha M. et al. Restoring systemic GDF11 levels reverses age-related dysfunction in mouse skeletal muscle. June 2014, Science.

Two recent studies of lab mice showed that transfusions of blood from younger individuals reverse the effects of aging in their elders. One research group showed that neural damage of mice with age-related cognitive impairments could be reversed by such transfusions. Alternatively, injecting the younger plasma into the brain was also very effective at repairing neural damage. Another research group showed that blood from younger mice repaired age-related heart defects in older mice. Researchers further discovered that high levels of the protein GDF11, present in the blood of younger mice, were the key for rejuvenation. Researchers proposed that blood from younger mice contains molecules with anti-aging properties that awaken the stem cells of the brain and heart muscles and thus initiate the rejuvenation. These studies are incredibly encouraging for combating Alzheimer’s disease, heart disease, and many other age-related diseases; however, a comprehensive set of clinical tests needs to be conducted before testing the effects in humans.

“Chameleon” plant discovered

Gianoli E. and Carrasco-Urra F. Leaf mimicry in a climbing plant Protects against herbivory. May 2014, Current Biology.

Scientists thought for many years that camouflage and mimicry were only observed in the animal kingdom. A newly discovered wood vine in Chile, Boquila trifoliolata, has been found to transform its leaves to mimic a variety of host trees. B. trifoliolata is the first plant ever shown to imitate multiple hosts. This is a rare trait called “mimetic polymorphism” and it was only previously observed in butterflies. As B. trifoliolata climbs onto a tree’s branches, it changes the color, size, shape, orientation, and even the vein patterns of its leaves to match the surrounding flora. When the same vine crosses over to a second tree, the size of its leaves can even increase 10 times  to match the second host plant. According to scientists, mimicry may protect the vine from plant-eating herbivores such as weevils and leaf beetles. It is perplexing how a plant can distinguish between individual trees and keep changing its physical characteristics. Odors, chemicals, or microbes that are released form host plants are potential candidate mechanisms for this intriguing plant behavior.

The life of a star is affected by two main factors: while gravitational forces pull the gas contained in the star towards the center, pressure that is generated by the nuclear fusion which takes place in the center pushes the gas outwards. When a star runs out of fuel, gravitational forces take over and it results in the sudden collapse of the star. As a result of this sudden collapse, oversized stars get dispersed into space through a massive explosion. These explosions are called supernovas.

It may be a hard task to predict beforehand whether a particular star will be dispersed in the shape of a supernova. When explosion takes place, dispersal of the supernova happens so fast (within 2-3 minutes) that it is almost impossible for astronomers to capture the exact moment of the explosion. After the initial explosion, there is extreme brightness and this lasts for a couple of weeks. This event when observed from a distance is taken as if the birth of a new star. Later on, the brightness gets dimmer and eventually disappears. Astronomers only have to investigate the remnants of the supernova from this point on. In some supernovas, stars get completely destroyed by dispersal into space (Type 1), but in some, a neutron star is left behind (Type 2).

Type 1 supernovas

Even though supernovas are known to be explosions of oversized stars, smaller ones can also explode and still be considered as a supernova. Interestingly, supernovas of smaller stars are even brighter. Stars with a mass less than the total mass of eight suns turn into a red giant at the end of their lives. After the red giant stage, exterior layers of the star get blown into space and it turns into a white dwarf with a mass equal to 0.6 times the mass of the sun. If a hydrogen rich material from a large star nearby flows over this white dwarf, it turns the white dwarf into an explosive composition. The white dwarf reaches the brightness of a million stars by exploding. These types of explosions are called novas.

Even though we see stars in the sky as individual bodies, 60% of them are found in pairs. An amazing star bomb is generated when the two white dwarfs in a star duo join one another. These massive explosions of White Dwarfs as a result of their complete dispersal into space by thermonuclear chain reactions can even be observed from distant galaxies. They always explode at the same mass threshold and since the amount of released energy is the same, they are used as standard light sources by astronomers. When the resulting star (formed after the two dwarfs unite) exceeds the critical size of 1.4 times the mass of the sun, it starts to collapse on its own with gravitational forces. Central pressure increases during this collapse and with the start of thermonuclear reactions, it eventually builds up internal pressure.

Since the outer layer of the star is hardened, it completely disperses into space with an enormous explosion. Remnants left behind by the explosion begin to expand very rapidly (at a speed of 30,000 km/s). Brightness more powerful than a billion stars is generated during the energy release of Type 1 supernova. In other words, the energy supernova released for a couple weeks is much greater than the total lifetime energy released by the sun. The initial strength of the supernova diminishes after a few weeks. As the supernova expands, its brightness decreases proportionately.

Ultimately it becomes a gas and a dust cloud known as a nebula.

Supernovas may be observed in different levels of brightness depending on the distance of the star to the earth. Closer supernovas can be seen as big and bright as the moon however distant ones can be observed like a bright, dimmed star, or may not be visible at all.

Type 2 supernovas

Stars with a mass between 8 and 50 times the mass of the Sun go through a series of changes a lot faster than smaller stars, eventually turning into a neutron star. During these kinds of changes, all stages of nuclear fusion takes place, as first hydrogen, then in order, helium, carbon, nitrogen, oxygen, silicon, and iron are synthesized in the stars. Iron is found in the center and other elements surround it in layers. When such a star runs out of fuel, nuclear fusion ends. The finale of nuclear fusion reactions at this stage is characterized especially with iron representing a stable nuclear structure.

When the reactions are over in the center, the iron core collapses on its own with gravitational forces. Because of the intense pressure on iron, protons of this atom unite with its electrons forming neutrons. This event takes place very fast and also particles called neutrinos are emitted. These particles apply an outward pressure on the exterior layer of this star which has already turned into a super red giant, causing burst of external layers into space. This event is described as being a Type 2 supernova.

Remnants of supernovas

Supernova remnants are radioactive. In fact, a major portion of the light emitted by a supernova is derived from radioactivity. Furthermore, supernova remnants are very powerful sources of cosmic radiation. These remnants can be observed in two forms: the first form is directly observable gamma rays when high energy particles including protons and electrons interact with interstellar gasses; and the second form is indirectly observable radio waves when high speed electrons emitted via explosion get accelerated at the interstellar magnetic fields. Gases rich in heavy elements that constantly expand are left behind after supernovas. Because of abundant neutrons in the environment, elements heavier than iron are also synthesized. This richness is entirely thrown into the interstellar place. All of the heavy metals including iron are thought to have joined the solar system through a supernova explosion. “We have sent down iron” in Chapter 57 of the Holy Qur’an may refer to the dispersal of iron and other elements into the space through supernova explosions.1

Sun rising from the West

What happens when a star nearby our system explodes as a supernova? A second sun appears in the sky. Does such a supernova explosion disrupt the conditions on the earth via causing a similar or bigger impact than the sun on the planet in terms of light and heat? If such an exploding star happens to be in the west, can we consider it as the sun rising from the west? Considering that supernovas are strong light sources, a second sun appearing in the near sky for a couple of weeks will have significant impacts on planet earth.

At first, day and night would disappear. Planetary temperatures would rise to lethal degrees. Evaporation of seas and oceans may cause worldwide flooding. Local temperature rise caused by the two suns may generate severe storms. Remnants of the star as it loses brightness after a couple of weeks can color the sky blood red as described in the verse: “And finally when the heaven is rent asunder, and it becomes rosy like red hide!” (Rahman 55:37). Events pointing to doomsday as described in apocalyptic verses can take place. Surely God knows the best of everything.

Notes

1 For a similar discussion on a possible connection of this phenomenon with this Qur’anic verse, you may refer to a previously published article titled “Supernova Explosion and a Miracle of the Qur’an” by Nuh Gedik (The Fountain #54, 2006).

References

Silk, Joseph. 1997. A Short History of the Universe, W. H. Freeman.

Zeilik, Michael. 1994. Astronomy: The Evolving Universe, New York: John Wiley & Sons Inc.

]]> https://fountainmagazine.com/all-issues/2010/issue-76-july-august-2010/synthetic-life-hype-or-reality/ Thu, 01 Jul 2010 00:00:00 +0000 http://107.21.79.195/all-issues/2010/issue-76-july-august-2010/synthetic-life-hype-or-reality/ 1- Synthetic life: hype or reality?

Original Article: Gibson, D.G. et al., Science Express (2010).

A team of genome researchers at the J. Craig Venter Institute in the U.S recently announced that after almost 15 years of work and with a budget of $40 million, they had finally built the first bacterial strain with a completely synthetic genome. In the study, researchers chopped the genome of Mycoplasma mycodies into 1,000 pieces in the computer, chemically synthesized these fragments and assembled them into an artificial chromosome in yeast cells. The reconstructed artificial genome was subsequently transferred to a closely related bacterium Mycoplasma capricolum, whose genome was removed. Remarkably, the strain with the artificial genome was able to guide the protein machinery of the host cells, produce the necessary enzymes and macromolecules for a bacterium to survive and most importantly to grow and divide. Team leader Prof. J. Craig Venter, best known for his pioneering efforts in human genome mapping project, commented on their findings as “we created a ‘synthetic cell’ and it is the first self-replicating species we’ve had on the planet whose parent is computer.” Many media sources also publicized the study as the first successful creation of the artificial life. As much as the scientific community agreed that the synthesis, transfer and retention of a functional synthetic genome is a breakthrough, most of the scientists have found Prof. Venter’s comments and the media’s reflection on the study to be somewhat of an overstatement. It would be quite unfair to call the new bacteria an example of “artificial life.” The synthesized genome was a copy of another living bacterium with slight modifications. The genome is a blueprint, whereas the proteins perform the actual cellular functions. This new approach shows that we can copy the book of cellular blueprints reliably but it brings no new parts to our inventory. Moreover, the synthetic genome had to be assembled in live yeast cells, processed with biochemical extracts from mycoplasma cells and finally transplanted into another (closely related) live cell. In other words, “natural life” was absolute prerequisite for the so-called “artificial life.” The generation of a fully functioning organism directed by machine-synthesized genome certainly represents a major step in our ability to manipulate large chunks of genetic material. It is clear that this study will positively influence many scientists, especially synthetic biologists, to try writing novel “synthetic” software to recruit the variety of organisms’ cellular hardware for solving various global problems like energy shortage or environmental pollution. However, the philosophical questions that probe the essence of life, like: “Can we reduce life to material? Is the human being ever going to be able to build a live cell from only a few chemicals?” will likely remain as major controversial issues for many years in the age of molecular biology.

2- Sharing the powers of Spiderman

Original Article: Vogel, M.J. & Steen, P.H., PNAS (published online before print on February 4, 2010).

The adhesive powers of Spiderman, jumping from one building to another and walking on the walls, attracted most of our interests. The recent invention of scientists from Cornell University brings this power from science fiction cartoons/movies to the real life. Inspired from a little creature, leaf beetle, which can stick to leaves by generating a force exceeding 100 times its body weight, these researchers designed a device which can stick to surfaces by using the adhesive powers of water. The device consists of a plate not thicker than a credit card with hundreds of tiny holes on it. The water is pumped through these holes, which builds liquid bridges between surfaces and thus generates a strong adhesive force. Simply pushing back the water un-sticks the device in a controllable and switchable manner. There are no solid moving parts nor any kinds of glue used in the system, and this makes device even more promising. The capabilities of the device are not at the level of the leaf beetle yet, but the inventors believe that it can be improved by building on the same principles. The system can potentially be used in many practical applications, such as robotics, and it can also be implemented into shoes and gloves allowing them to stick to surfaces. Accordingly, it is no longer improbable to imagine sharing the sticky-powers of Spiderman and walking on the walls very soon.

3- Igniting a Supernova

Original Article: Gilfanov, M. & Bogdan, A., Nature 463, 924 (2010).

upernova: the Rosetta stone that may help us put together the missing pieces of the cosmic jigsaw puzzle; one of the most energetic and most luminous explosions in the universe, putting out energies equivalent to what our sun could produce in 10 billion years. Yet the mechanism that produces these explosions still eludes us. Once our sun consumes its remaining fuel in another 5 billion years, it will shrink into a “white dwarf.” These compact stars are believed to produce subsequent explosions leading to supernovas if they reach beyond a critical limit of mass. One way to gain mass is to steal material from a companion star through an “accretion” process. Accretion was thought to be the most common means that might help push the mass of a white dwarf beyond the critical mass limit, until a recent study revealed that two clashing (in-spiraling) white dwarfs might be the missing fuse that ignites supernovas. German astronomers measured the X-ray flux of four nearby elliptical galaxies and the core of the Andromeda Galaxy to see whether the amount of X-rays from these galaxies are consistent with predictions based upon the accretion mechanism. Contrary to expectations, the observed X-rays were 2–3% of the amount that would have been produced if accreting white dwarfs were the primary trigger of supernova explosions. Hence, perhaps merging white dwarfs are more commonplace in the cosmos after all.

4- Strategy of bats finding their way

Original Article: Yovel Y et al., Science 327, 701 (2010).

Bats, dolphins, shrews and swiftlets use sound waves for navigation and hunting. They emit short sonar pulses and listen to the echoes reflecting back from solid objects. Microsecond differences in the arrival times of echoes are coded by detector neurons and used as a main cue for positioning objects in an environment. This phenomenon is known as biosonar. A recent study published in Science reveals one unknown part of this perfect sound processing strategy. The study shows that bats do not center the sonar beam on the target. Instead, they aim to match the maximum slope of the beam to the target in order to increase the signal-to- noise ratio. Around the sharp edge, small variations of the target position can be detected as a clear signal change in reflected sound intensity. Furthermore, the researchers showed that if the environment is very noisy, bats could bias this critical point to increase amplitude of the echoes. This powerful technique has already been employed by humans in engineering and used in various technological tools such as atomic force microcopy. Whether this strategy is used in general by other echolocating animals remains to be answered.

…And We sent down Iron, in which is great might, as well as many benefits for mankind… (Hadid 57:25)

The above verse in the holy Qur’an uses the Arabic expression “anzalna”which means “sent down” for iron. But why? Early commentators understood this as having a metaphorical meaning to explain that iron has been sent to benefit people. But after understanding the nature of one of the most powerful explosions in the universe, you realize that the direct meaning “being physically sent down from the sky” miraculously points out to a very important scientific fact that was discovered only very recently. To understand and appreciate this miracle of the Qur’an, we will first talk about the life and death of stars and then come back to this verse to describe its relevance in detail.

Just like human beings, stars are also born, live, and die. One big difference is that they can live billions of years compared to the less than 100 years of human life. Also, for us, there is no way of knowing how long we will live or how we will die. But for a star, given its mass, you can predict its lifetime and the way it will die. Stars about the size of our sun live for a long time (a couple of billion years) and die gradually. Whereas massive stars with a mass of about 8 times the mass of our sun or more have short lifetimes (tens of million years) and die in a quick and incredibly violent explosion known as a supernova.

Supernova explosions are one of the most spectacular astronomical events observable by human beings. Normally, in a typical galaxy there are about 10 billion stars. A supernova happens to be one of these ordinary stars until it explodes. During the explosion, the amount of energy released by the supernova can exceed the energy of all the other stars combined in its galaxy! The power of this explosion is far too big even to imagine. The energy released is even greater than the total energy our sun will put out during its 10 billion year life!

The brightest supernova of modern times was an extragalactic supernova recorded in 1987. Since it was the first supernova in 1987, it was labeled as “1987A.” This is by far the best studied supernova of all times. In Fig. 1, the left panel shows the region of the sky two weeks after the supernova exploded. The supernova is still very bright. The right panel shows the same region before the explosion, with the arrow indicating the star undergoing the supernova explosion. This particular supernova was 160,000 light years away from us. This means that the actual explosion happened 160,000 years ago, but because it was so far from us, it took 160,000 years for the light rays from the explosion to reach us.

Fig 1. After and before images of the 1987A supernova. The left panel shows the region of the sky two weeks after the 1987A supernova exploded. The supernova is still very bright. The right panel shows the same region before the explosion and the arrow indicates the star undergoing the supernova explosion.

Since the supernova becomes extremely bright, it is even sometimes possible to see it with the naked eye in daytime. In fact, there are historical reports from ancient times concerning supernova explosions. On July 4th, 1054 A.D., Chinese astronomers noticed a “guest star,” which was visible in daylight to the naked eye for 23 days. Its remnant was discovered by the British amateur astronomer John Bevis in 1731. We now know that this bright “guest star” was a supernova. Its remnants, known as the Crab Nebula, are shown in the left panel of Fig. 2. This supernova is one of the very few that have been observed in our Milky Way galaxy. The last supernova to explode in our galaxy was in 1607 (see Fig. 2 right panel).

Supernova explosions are one of the most violent events that happen in the universe. They release an unbelievable amount of energy. But why would a star explode anyway? If it has so much energy still, why does it not remain shining peacefully as it does for most of its lifetime? To answer these questions, we need to remember how stars work.

Figure 2 Supernovae remnants. The left panel shows remnant of the supernova that exploded in 1054. It is about 6,500 light years from earth. It consists of diffuse interstellar gas and dust (nebula) spread in a circular region of a diameter of 6 light years.(Image Credit: FORS Team, 8.2-meter VLT, ESO ). The right panel shows remnants of the last supernova, which exploded in our galaxy in 1604. This combined image — from NASA’s Spitzer Space Telescope, Hubble Space Telescope, and e Chandra X-ray Observatory — unveils a bubble-shaped shroud of gas and dust that is 14 light-years wide and is expanding at 4 million miles per hour (2,000 kilometers per second). It is about 20,000 light years away from us.(Image and caption credit: NASA )/

Let us start by answering a more basic question: What is the energy source of stars? Stars produce their energy through a process called nuclear fusion. The idea is very simple; you fuse together light nuclei, like hydrogen, to produce heavier nuclei, like helium. In this process, the combined mass of low-mass nuclei is more than the resulting fused massive nucleus. This difference in the masses is converted to energy through the Einstein’s famous E=mc2 equation, where E is the energy released, m is the mass difference that is released in the reaction, and c is the speed of light.

But since the nuclei are positively charged, they repel each other, so there must be extremely high densities and temperatures to overcome this barrier. The most common form of fusion that takes place in stars is the fusion of four hydrogen nuclei to produce one helium nucleus. The temperature needs to be about 8 million C0 for this reaction to occur. It requires higher temperatures to fuse nuclei that are heavier than hydrogen. For example, fusing helium requires temperatures higher than 100 million C0.

During most of their lifetime, stars produce energy by fusing hydrogen into helium. After they run out of hydrogen, if the temperatures in their cores are high enough, they start to fuse helium nuclei into carbon and oxygen. And when they run out of helium, they then start to fuse carbon and oxygen. As mentioned above, fusing heavier elements requires extremely high temperatures and high pressures, so it can only happen for massive stars in the late stages of their lives where such conditions are met. For lighter stars like our sun, temperatures are not enough for this.

Even for the massive stars, fusion reactions cannot continue forever. The game of building heavier and heavier elements stops when iron is produced in the core. Iron is a very special element. It has the highest binding energy per nucleon. This makes it the most stable element. You actually lose energy when you fuse iron nuclei together rather than gain energy, so elements heavier than iron cannot be made during these cycles. At this stage of its life, the star looks like an onion, in the sense that it has a layered structure. At the core there is iron, surrounding this core there are layers of lighter elements in the order of their atomic weights, with hydrogen being at the outermost layer (see Fig. 3).

At this point in time, a very delicate balance that holds the star steady becomes unstable. Normally, the gravitational attraction tries to compress everything together. Therefore, the star has a tendency to collapse onto itself due to gravity. This is balanced by the outward radiation and thermal pressure that are generated by intense fusion reactions that are occurring in the core. But when the core turns into iron, fusion can no longer take place. That means there is no longer a supporting outward force that prevents the star from collapsing.

Figure 3 The onion skin model of a supernova. As it gets close to its death, a pre-supernova star has a layered structure that resembles an onion. Heavy elements produced by nuclear fusion inside the star are concentrated toward the center of the star. Iron, being the most stable element, sits at the core.

After the iron core gets to a certain size, this iron core suddenly collapses onto itself. This collapse happens so fast that it takes only a fraction of a second for the initially earth-sized core to shrink to a radius of 60 km. As the core collapses, the outer layers of the star start to collapse and rush in to fill the gap created by the collapsing core. At this point, another drastic event occurs. The iron core cannot compress forever. When the density in the core reaches the nuclear density, it rebounds. This time the core starts to move outward. But wait, the outer layers are still collapsing! When the collapsing envelope of the star meets with the rebounding core, one of the most powerful explosions in the universe occurs. This is known as a supernova explosion, which can be seen millions of light years away!

This gigantic collision ejects the outer layers of the star into the interstellar medium. As a result of the extreme conditions generated by this, the fusion of heavier elements (heavier even than iron) occurs. As the material from the exploding star collides with the interstellar gas and dust, a whole range of light emissions (from visible to X-ray) occurs. Colorful nebulae (as seen in Fig 2.) that will glow for thousands of years are thus generated.

One of the most important outcomes of supernova explosions is that heavy elements, including iron, are ejected into the interstellar medium. In fact, the only source of heavy elements is such events. All the heavy elements that are found in our solar system are made in one of these violent explosions. They cannot be made in our solar system, as they require extremely high temperatures. That means, the carbon that makes our cells, the hemoglobin that carries oxygen in our blood, and basically almost everything in our body are all made of elements produced in these explosions. We are, in the most literate sense, stardust. It is estimated that on average each carbon atom in our body went through four of these cycles in the past.

It is very clear that these explosions are important for the existence of life on earth. But, understanding the mechanism of these events was only possible in recent years.

It is extremely surprising to hear that iron and almost every other element in our body were made during one of these explosions. Even more astonishing is when we look at what the Holy Qur’an says about iron.

In the Holy Qur’an, there is a special chapter about iron, known as “Hadid” or “Iron”. The first thing that surprises you about this chapter is its chapter number: 57. The interesting thing about this is that it matches the atomic weight of one of the isotopes of iron. Iron can have stable isotopes with atomic weights of 54, 56, 57, and 58. The most common form of iron is the one with atomic weight 56 (56Fe).

The reason why this chapter is called “Iron” is the fact that in one verse of this chapter, the Holy Qur’an talks about iron. The second thing that is surprising is the verse number of this particular verse: 25 (or if you count the basmala, it becomes 26). This number (26) is the number of protons in an iron nucleus. And the third numerical code is the total number of verses in this chapter and that is equal to 30. This is equal to the number of neutrons in the most common form of iron nuclei (56Fe). Additional numerical codes can be found through a more detailed inspection of this Qur’anic chapter. No one knew anything about the iron nuclei in the 7th century when the Qur’an was revealed in its present form. And the chance of these numbers being purely coincidental is less than one in a thousand.

After studying these numerical codes, the content of the verse is even more interesting and closely related to our topic. In this verse, the Almighty says: …And We sent down Iron, in which is great might, as well as many benefits for mankind … (57:25). The expression “sent down” used for iron in this verse is the English translation of the Arabic word “anzalna”. This can either be understood as having a metaphorical meaning to explain that iron was given for the benefit of people. But, if the literal meaning, “being physically sent down from the sky,” is considered, we realize that this verse miraculously indicates the scientific fact that all the iron in our solar system came from the sky from supernova explosions.

Another interesting aspect is the fact that the verse says “…in which is great might …” The Arabic word “shaded” used to describe this can also be translated as “in which is great power” or as “in which is great violence”. If you assume this phrase is referring to iron, you can understand it to mean that iron has a great strength. Or a deeper meaning would be to consider the fact that iron nuclei is the most stable nuclei, i.e. the fact that it has the highest binding energy per nucleon. If you consider this phrase as referring to the act of sending down, in that case it reminds you of the great violence in supernova explosions.

In summary, supernova explosions are the violent deaths of massive stars. The course of events that leads to these gigantic explosions, as well as their far reaching consequences, is very interesting. They are the only source of iron and other heavy metals found in our solar system. They show the mercy of God, as life on earth without them would not be possible. At the same time, they can be thought of as an incredible show of divine power. As the Holy Qur’an says at the end of the verse that mentions iron:

Surely God is the All-Strong, the All-Glorious with irresistible might. (Hadid 57:25)

The Anglo-Australian Observatory (http://www.aao.gov.au/)

http://antwrp.gsfc.nasa.gov/apod/ap030914.html

http://www.nasa.gov/multimedia/imagegallery/image_feature_219.html

For more detailed discussion, see for example: Adam Burrows, Nature 403 (6771), 727 (2000).

http://chandra.harvard.edu/resources/illustrations/superPre.html

For example, according to numerological (abjad) calculations, the abjad of the word “Al-Hadeed” in Arabic, when the numerological values of its letters are added up is also 57 and numerological value of the word “Hadid” alone is 26. ( http://www.miraclesofthequran.com/scientific_30.html )

Did you know that we are actually stardust? Most probably, you didn’t. Nuh Gedik lifts our eyes from the ground into the depths of space. In his thought-provoking article he describes how a star explodes to present a marvelous celestial supernova show. Supernova explosions are actually “the only source of heavy elements, including iron . . . the carbon that makes our cells, the hemoglobin that carries oxygen in our blood, and basically almost everything in our body are all made of elements produced in these explosions.” “Supernova Explosions” explains more not only about stars, but also about our chemical make-up.

The mysteries of nature are disclosed a bit more by another show, this time on earth: The glowworms of the Waitomo caves in New Zealand are bioluminescent flies which present stunning shows that rival the star-lit sky at night. The theory of evolution fails to explain the complex nature of this minute insect which can yield light at an output of 100% with no energy wasted as heat. Have we yet reached such a capacity of power production? Safak Ozturk tells us more in his “A Message from Glowworms.”

Inefficient use of time is something that we all complain about. Everyday, we get up in the morning and rush to our jobs to start work in time. However, today, more frequently than ever, we end up having spent our days having done little more than checking several e-mails, making telephone calls, and going to meetings to change schedules and deadlines. Cafer Tayyar Yavuz highlights the importance of even the smallest slice of time we usually ignore and explains how better efficiency can be achieved in our use of time.