Upside-down Shadows: An Interesting Phenomenon

You viewers are no stranger to the pin hole camera you might have studied in your 6th or 7th grade, where it inverts the upright image. The concept of convex and concave lens is also familiar to you. The image formed by convex lens is inverted and that formed by concave lens is upright. Inverted images are usually formed on the screen…(Ok, I’m going to far). Coming back to the topic, you’ve heard of and seen inverted images, but I bet you must have not seen your own shadow being inverted.

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Nanotechnology: The Anticipated future

”Why can’t we right all the 24 volumes of the Encyclopedia Britannica on the head of a pin?”, asked Richard Feynman.

Science has developed since the birth of the universe, but we slowly knew them after the birth of humans, birth of famous scientists, thinkers, and many more. But, there is a difference. Science of today has more difference than science of yesterday, and science of yesterday has more difference  than science of day before yesterday. Like that, science has changed so much in the past that we are able to enjoy the technology that we have today. Science has produced so many thinkers that they are able to anticipate the future which awaits for the human beings and of course, our planet Earth. Albert Einstein and Stephen Hawking were two great examples of thinkers, who were able to ‘simulate’ the future in their minds themselves. What technology awaits for us, then, in the future, you might ask? Yes, the future technology: Nano technology.

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Biological Immortality

I’m pretty sure you viewers must have gotten happy on seeing the word ‘immortality’. All of us don’t want to die, right? Sadly, we have to, also, the topic on which I’m talking about, ‘Biological immortality’, only applies for other special animals, not us humans. Why not us? Is there a way we can ‘revive’ after death? All the questions will be answered on this amazing article on this amaaaazing topic!

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Top 9 deadliest insects on Earth that make you want to stay in home only!

Lions are entitled the ‘King of the Jungle’, elephants are the largest mammals on land. All those stories you might have heard of. But, a teeny-weeny insect scares the scariest lions on Earth, the biggest elephant on Earth. Believe that? Probably, mostly, no. But, these insects are literally so scary that you probably will be happy that you’re not near forests. And, please note, the title was not an exaggeration. Insects can cause death too. 

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HOW DO GALAXIES LOOK LIKE

In  most of the galaxy , the stars are not uniformly  distributed , but instead  are  arranged  in  certain patterns.  The  most frequent ones are spiral galaxies .The center of such galaxies is thick  with  several old , red  shining stars. A flat  disc stretcher all around  this  centre in wich  the individual arms of  the spiral are present. It has a  thickness  of  just about 100 light years, which is  very thin as compared to the size of a galaxy. The spiral arms contain a lot of young bright blue stars. If a sprial  galaxy . other  types of galaxies are  the egg-shaped  “elliptical galaxies ” and the  irregular  galaxies , which  are  completely disordered.

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ORIGIN OF UNIVERSE

The most popular theory of our universe’s origin centers on a cosmic cataclysm unmatched in all of history—the big bang. This theory was born of the observation that other galaxies are moving away from our own at great speed, in all directions, as if they had all been propelled by an ancient explosive force.

Before the big bang, scientists believe, the entire vastness of the observable universe, including all of its matter and radiation, was compressed into a hot, dense mass just a few millimeters across. This nearly incomprehensible state is theorized to have existed for just a fraction of the first second of time.

Big bang proponents suggest that some 10 billion to 20 billion years ago, a massive blast allowed all the universe’s known matter and energy—even space and time themselves—to spring from some ancient and unknown type of energy.

The theory maintains that, in the instant—a trillion-trillionth of a second—after the big bang, the universe expanded with incomprehensible speed from its pebble-size origin to astronomical scope. Expansion has apparently continued, but much more slowly, over the ensuing billions of years.

Scientists can’t be sure exactly how the universe evolved after the big bang. Many believe that as time passed and matter cooled, more diverse kinds of atoms began to form, and they eventually condensed into the stars and galaxies of our present universe.

Origins of the Theory

A Belgian priest named Georges Lemaître first suggested the big bang theory in the 1920s when he theorized that the universe began from a single primordial atom. The idea subsequently received major boosts by Edwin Hubble’s observations that galaxies are speeding away from us in all directions, and from the discovery of cosmic microwave radiation by Arno Penzias and Robert Wilson.

The glow of cosmic microwave background radiation, which is found throughout the universe, is thought to be a tangible remnant of leftover light from the big bang. The radiation is akin to that used to transmit TV signals via antennas. But it is the oldest radiation known and may hold many secrets about the universe’s earliest moments.

The big bang theory leaves several major questions unanswered. One is the original cause of the big bang itself. Several answers have been proposed to address this fundamental question, but none has been proven—and even adequately testing them has proven to be a formidable challenge.

FORMATION OF STARS

Neutron stars are ancient remnants of stars that have reached the end of their evolutionary journey through space and time.

These interesting objects are born from once-large stars that grew to four to eight times the size of our own sun before exploding in catastrophic supernovae. After such an explosion blows a star’s outer layers into space, the core remains—but it no longer produces nuclear fusion. With no outward pressure from fusion to counterbalance gravity’s inward pull, the star condenses and collapses in upon itself.

neutron-star_8914_600x450
Neuron star

Despite their small diameters—about 12.5 miles (20 kilometers)—neutron stars boast nearly 1.5 times the mass of our sun, and are thus incredibly dense. Just a sugar cube of neutron star matter would weigh about one hundred million tons on Earth.

A neutron star’s almost incomprehensible density causes protons and electrons to combine into neutrons—the process that gives such stars their name. The composition of their cores is unknown, but they may consist of a neutron superfluid or some unknown state of matter.

Neutron stars pack an extremely strong gravitational pull, much greater than Earth’s. This gravitational strength is particularly impressive because of the stars’ small size.

When they are formed, neutron stars rotate in space. As they compress and shrink, this spinning speeds up because of the conservation of angular momentum—the same principle that causes a spinning skater to speed up when she pulls in her arms.

Pulsing Lights

These stars gradually slow down over the eons, but those bodies that are still spinning rapidly may emit radiation that from Earth appears to blink on and off as the star spins, like the beam of light from a turning lighthouse. This “pulsing” appearance gives some neutron stars the name pulsars.

After spinning for several million years pulsars are drained of their energy and become normal neutron stars. Few of the known existing neutron stars are pulsars. Only about 1,000 pulsars are known to exist, though there may be hundreds of millions of old neutron stars in the galaxy.

The staggering pressures that exist at the core of neutron stars may be like those that existed at the time of the big bang, but these states cannot be simulated on Earth.

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