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Timeline: The Tallest Buildings in The World


Architecture has grown by leaps and bounds in the last 150 years. Here, we present before you the list of the tallest buildings in the world in the last 150 years.

Period
Building
Height
1870–1884
Equitable Life Building, New York
40 metres
1884–1890
Home Insurance Building, Chicago
42 metres
1890–1894
New York World Building, New York
94 metres
1894–1895
Manhattan Life Insurance Building, New York
100 metres
1895–1899
Milwaukee City Hall, Milwaukee
108 metres
1899–1901
Park Row Building, New York
119 metres
1901–1908
Philadelphia City Hall, Philadelphia
167 metres
1908–1909
Singer Building, New York
186.57 metres
1909–1913
Metropolitan Life Tower, New York
213.36 metres
1913–1930
Woolworth Building,New York
241 metres
1930
Bank of Manhattan Trust Building, New York
283 metres
1930–1931
Chrysler Building, New York
319.9 metres
1931–1972
Empire State Building, New York
381 metres
1971–1973
World Trade Center, New York
417 metres
1974–1998
Sears Tower,Chicago
442 metres
1998–2004
Petronas Towers, Kuala Lumpur
451.9 metres
2004–2010
Taipei 101, Taipei
509.2 metres
2010 –
Burj Khalifa, Dubai
828 metres






The Evolution Of The Periodic Table


The periodic table is one of the most iconic symbols of science. Over the years, it has evolved into the periodic table that we know today. Its history can be traced back to over 200 years ago. The Periodic Table has been altered, changed and redrawn into the modern Long Form Periodic Table.

The word periodic, comes as the periodic table contains elements following a periodic repetition of basic properties. The origins of the periodic table lie in a list of 33 known elements made by French scientist Antoine Lavoisier, Antoine Fourcroy, Louis-Bernard Guyton de Morveau and Claude-Louis Berthollet in 1787. In the earliest attempt to oraganise elements into fixed groups, German chemist Johann Döbereiner, in 1817, organised elements into groups of 3 called triads. He noticed that if the three members of a triad were ordered according to their atomic weights, the properties of the middle element fell in between those of the first and third elements. Also, Döbereiner showed that the atomic weight of the middle element is almost the average of the weights for the first and third members of the triad. Peter Kremers of Cologne also used the triad theory to suggest that certain elements could belong to two triads placed perpendicularly. He compared elements geometrically, a feature that later proved to be an important part of Mendeleev’s system.

In 1857 French chemist Jean-Baptiste- André Dumas turned away from the idea of triads and focused instead on devising a set of mathematical equations for increase in atomic weight among groups of chemically similar elements. But atomic weight is not the fundamental property of the elements, and so, he was not successful. English chemist John Newlands suggested in 1864 that when the elements were arranged in order of atomic weight, any one of the elements showed properties similar to those of the elements eight places ahead and eight places behind in the list- the Law of Octaves.

The first periodic table is said to have been drawn by Russian chemistry professor Dimitri Ivanovich Mendeleev and completed on the 17th February 1869. It included 63 elements in order of increasing atomic weight and also had spaces for elements proposed be undiscovered.

One of the most important features of the Mendeleev table was that it showed periodicity among elements, a feature that had been observed in 1862 by French geologist Alexandre- Emile Béguyer de Chancourtois. He positioned the elements according to increasing atomic weight along a spiral inscribed on the surface of a cylinder and inclined at 45 degrees from the base. The spiral started from oxygen and the first full round was completed at sulphur and so on.

Chemist Julius Lothar Meyer of Breslau University in Germany in 1868 produced a periodic table that turned out to be remarkably similar to Mendeleev’s famous 1869 version. But it did not come out until 1870 because of a publisher’s delay, a factor that contributed to a dispute that ensued between Lothar Meyer and Mendeleev. Had it not been for that publisher, we might have been reading Lothar Mayer’s name instead of Mendeleev’s (it’s easier to learn anyways!).

In 1894, William Ramsay of University College London and John William Strutt discovered the element argon over the next few years, Ramsay dicovered four other elements—helium, neon, krypton and xenon.In 1913 Dutch physicist Anton van den Broek suggested arrangement principle for the periodic table should be the nuclear charge of each atom. This fundamental quantity is now known as atomic number.

The modern periodic table has been designed in such a way that the position if elements directly corresponds with the position of electrons in the atomic electron shells. In 1924 physicist Wolfgang Pauli set out to explain the length of each row in the table. As a result, he developed the Pauli Exclusion Principle, which states that no two electrons can exist in exactly the same quantum state.

In the last 30 years too, researchers have tried to make alterations to the periodic table. Fernando Dufour has developed a three-dimensional periodic table, which displays the fundamental symmetry of the periodic law. In 1980 Ray Hefferlin devised a periodic system for all the diatomic molecules that could be formed between the first 118 elements. In a similar effort, Jerry R. Dias of the University of Missouri at Kansas City devised a periodic classification of a type of benzenoid aromatic hydrocarbons.

Still, the Periodic Table remains the most iconic chemistry symbols. After so much of evolution, we finally have perhaps the most perfect table ever.





The Solar System: Our Powerhouse - The Sun


The Solar System is our home. The earliest place we can map life to have begun is the solar system, when the planets broke apart from one central sun. So here, we start our series of articles about the Solar System. In the first of this series of articles, we describe for you the grandfather of the solar system – The Sun.
The sun lies at the very heart of the solar system. It is a medium- sized star which formed about 4.6 billion years ago (‘not very long ago’ in the universe!). But compared to even the largest planets of our solar system, it is way, way bigger. It has a diameter of about 1.38 million kilometers which is more than 110 times greater than that of the Earth. Despite being made fully of gases, its weight is more than 300,000 times that of the Earth.

The sun formed from a huge cloud of gas and dust which was pulled together by gravitation, like all other stars. The early solar system was a huge cloud of rocks and dust which has blasted off from the sun after its formation. Large chunks of rock pulled other particles together to form deformed bodies. These bodies later became planets and moons. These, bodies, which were moving randomly at high speeds, slowed down by the effect of the sun’s gravity and slowly can under its control and started moving around it. They were very hot due to volcanoes for a long time and cooled down to form the solar system as we know it today.

The sun is mainly composed of gases Hydrogen and Helium 92% Hydrogen and 8% Helium). At its center, the temperature may reach as high as 14,000,000 °C, hot enough for atoms to smash into each other to generate energy. This process is called nuclear fusion and the main energy produced by it are heat and light. It also involves the generation of helium atoms from hydrogen. In the sun, about 661 billion tons of hydrogen is converted into 657 billion tons of helium, which is used up gradually by conversion into 4 billion tons of energy. The heat and light of this energy reach up to great distances, heating even mars and lighting up bodies beyond Pluto. The surface temperature of the sun is about 5500 °C.
So this was the sun for you. It generates 99% of the energy of the solar system and is an absolute powerhouse. Our indebtedness to it is infinite.


Kepler 76b : The Einstein Planet


Einstein's special theory of relativity now has another feather in an already coveted hat, it has been used to discover an alien planet around another star.
The new planet –Kepler 76b- nicknamed "Einstein's planet" by the astronomers who discovered it is the first to be found through the relativity theory. The new Einstein-based works mainly for larger worlds, and is currently incapable of finding Earth-sized planets. Still, it offers some benefits, as it does not require high-precision measurements of a star's velocity. This method was first proposed by Dr Avi Loeb of the Harvard-Smithsonian Center for Astrophysics and Dr Scott Gaudi from Ohio State University in 2003.
The astronomers mainly focussed on very delicate effects predicted by Special relativity, such as the effect through which light from the parent star brightens as it comes closer to the planet by its planet’s effect, and dims as the planet pulls it away.
The planet is about 25 percent larger than Jupiter and weighs about twice as much, putting it in a section of planets known as "hot Jupiters." It is located some 2,000 light-years from Earth in the constellation Cygnus.
Also, gravitational tides from the orbiting planet caused its star to stretch slightly into a football shape, causing it to appear brighter when its wider side faces us. The planet itself also reflects a small amount of starlight. The planet is tidally locked to its star, always showing the same face to it. As a result, Kepler-76b broils at a temperature of about 3,600 degrees Fahrenheit.
The researchers used data from NASA's Kepler spacecraft, which provided the very detailed observations.





The Moon : Geography And Tourism


The most remarkable feature of the moon that can distinctly be seen with the naked eye are the dark Maria or ‘spots’. The most remarkable thing about these Maria is that all but one of them lie on the same side of the moon (the one facing the Earth)! Crater, too, are present on the moon. The moon was probably heavily bombarded by meteorites for a long period of time with led to the creation of these craters and the Maria. But along with carters formed by meteorites, there are also possible volcanic craters. An example of such a crater is Astarchus. Gases have been found to have emerged from it occasionally and it also has a clear peak. The geography of the moon is quite dull in a way, but in detail, it is really very interesting. In fact, poles of the moon have also yielded signs of water !
The moon was visited a large number of time by humans and machines between 1960 and 1975. The first organization to visit the moon was the Soviet Union, with its series of Lunik satellites, in 1959. In 1959 Lunik-2 crashed into the moon. And Lunik-3 orbited it. It was only in 1966 that Lunik-9 made a soft landing on the moon. NASA’s first aircrafts to visit the moon were the Rangers, in 1964 and 1965, crashing into it. Ranger 7 and 9 sent images of never-before seen areas of the moon, 1200 time better than could be seen with the best Earth telescope then. From 1966 to 1967, NASA launched Lunar Orbiters, which orbited the moon and took images from close, studying its surface. The first NASA crafts to land on the moon were the Surveyor series crafts, attaining a soft landing on the moon. Surveyor 5 even made advanced tests of the lunar surface. This helped us conclude the chemical nature of the moon’s surface, deducing it to be like basalt. During the 1970s, the Soviet Union continued sending its soft-landing probe vehicles to the moon, also sending two-wheeled Lunakhods 1 and 2, which were moved on the lunar surface by remote controls on the Earth.
In 1961, the Apollo mission was inaugurated, aiming to send man on the moon. In 1968, a series of Apollo missions sent astronauts to the moon, and in July 1969, Neil Armstrong and Edwin Aldrin became the first humans to step on the moon. The brought home samples of the  lunar surface and also took photographs before returning. Apollo- 17 was the last manned mission to the moon.




The Moon (In A Nutshell)

The Moon is the only natural satellite orbiting the Earth. It orbits the Earth due to the gravitational pull exerted by the Earth on it and in turn, exerts such a pull on the Earth too, thereby causing tides.
Since time immemorial, the moon has been a topic of mystery for all, first due to its regularly changing shape and then due to its very composition. It has been used a calendar by civilizations and viewed as a God by societies. 1609 was the year when the moon first came to be viewed as an object of real scientific interest, when Galileo first viewed it through his telescope. He identified distinct craters and mountains, which he called Maria, the Latin word for sea.
The moon is nearly spherical, with diameter 2,163 miles. The Earth and moon have among the lowest planet to satellite size ratios among the planets of the solar system, with the moons of Pluto the only ones with a lesser ratio. The distance of the Earth from the moon is about 240,000 miles, with it pulling away at 1.5 inches a year. The mass of the moon is about 1/82 that of the Earth, with its volume being 1/49 of it, meaning it is less dense than our planet.
The moon shines with the light reflected from the sun, called albedo. This is only about 7 per cent of the light that actually falls on it. When the moon is directly in line between the sun and the Earth, it is referred to as the new moon. When the sun makes a right angle with the moon, it forms a half moon. When the sun and moon are in a line again, with the Earth between them, it forms a fully illuminated moon, called the full moon. Between the half and full moon, the shape is called a gibbous, while between the half and new, moon, the shape is a crescent. The faded line between the dark and light portions of the moon is called the Terminator.
There is more than one kind of lunar month. The first is a synodic month, the interval from one new moon to another: 29.5 days. The other is a sidereal month, the time taken by the moon to orbit the Earth: 27.3 days.


Travelling In Space


Travelling in a jet is a rather fast way to go, but not fast enough for even small cosmic distances. The speed of light is 186,000 mps. Astronomers use light years to describe really large distances in space. A light beam can travel 5.88 Trillion miles in a year! The value of jet speed is taken to be 600 mph, and though it helps travel within countries in a matter of hours, it’s just a bit too slow for space. Here is a comparison based on the time taken to travel to popular ‘nearby’ destinations across space, travelling a light speed and jet speed:



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How The Universe Will End (In A Nutshell)

There have been a number of theories about the future of the universe, how it will and and whether it will even end. Here are some of them:

The Big Crunch Theory
This Theory is almost the exact opposite of the Big Bang Theory. It says that gravity may eventually slow down the expansion of the universe and pull everything back until everything ends in a big crash.

The Slowing Down Theory
This theory states that the universe does not have a definite end and will go on expanding endlessly and everything will gradually fade away. The density of the universe will keep going down greatly and the universe will eventually become a cold space of solitary particles.

The Oscillating Universe Theory
This theory implies that the universe consists of a series of Big Bangs and Big Crunches. It says that the universe works more like a heart, first expanding enormously due to a Big Bang and then succumbing to the force of gravity and coming back to form a Big Crunch only to repeat this again.

The Big Rip
This theory says that due to a large expansion of the universe in the future, everything in it, from galaxies to subatomic particles, is gradually and progressively torn apart.

Steady State Theory
This is a now discredited theory that said that the universe is a non-changing entity and has always remained as it is today. It says that the universe, basically, does not have a beginning or end and its density and size have remained and will remain the same over time infinite.

So these are the theories that suggest different fates for the universe. Which one is correct? You Choose!

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The Formation Of The Universe (In A Nutshell)



The Universe or Cosmos is the name used to denote the collection of all matter and energy (and everything else). How the Universe was created has remained a mystery over the years. Thousands and papers and myths have described the process of its creation but we really don’t know. It is said to have begun about 13.7 Billion years ago in and unimaginably violent a large explosion, called the Big Bang. This theory is known as The Big Bang Theory
.
The Big Bang is said to have been an explosion of mainly hydrogen and helium (and we know how violent they can be). This explosion cooled and formed tiny particles. These particles, as has been practically and theoretically proven, began to expand in all directions and dimensions (however many there are). Over time (a lot of it), clouds of hydrogen and helium formed, and these clouds later joined into dense clumps. The early universe was very dense, dense enough not to allow light to travel in it. Over time, density decreased and the clumps got together into localized groups. These localized groups got together to form galaxies.

In about 10 billion years after the Big Bang, 3.7 billion years before us (“near present time”), our sun began to form towards the outer part of a spiral galaxy, that we now call the milky way. Over the next 3 billion years, our planetary system, the solar system as we call it, was ready.

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