new year gift...

Follow these steps:

Open Notepad paste below code into it
now go to Edit > Replace (use CTRL+H)
replace 6 with _ and click Replace All
Enjoy

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The all new launching of Tata Nano 2012

Individual Interests....

How fast can you guess these words?

1. F_ _K 

2. PU_S_ 

3. S_X 

4. P_N_S 

5. BOO_S 

6. _ _NDOM 

Answers: 

1. FORK 

2. PULSE 

3. SIX 

4. PANTS 

5. BOOKS 

6. RANDOM 

You got all 6 wrong, didn't you?

Beautiful eyes...

You see these eyes……...one of the most beautiful I’ve seen.

Har ghar kuchh kehta hai………like wise har aankhe kuchh kehti hai. Don’t flash lights upon us. It’s not good for my health…..alas! Most of us have experienced the flashing of lights of vehicle coming from the opposite direction in night. So what is its relevance in this blog which is mainly concerned with emotions. Well everybody, whosoever is accidently reading this, would agree that such flashing of light usually give rise to unpleasant feelings and negative emotions. Well whenever I come across such a situation, my first reaction is to curse the driver of coming vehicle. The cursing is even more when the coming vehicle is better than mine. In earlier days of my driving I use to choose a way back home which had least traffic just to avoid this but now a days there are a lot of homo sapience going their respective homes along with or opposite to me, thanks to population blast we are facing. So the final out come of this population problem was that this problem of flashing of lights in nights can not be avoided (I say government should do something regarding problem of increasing population). When it become inevitable that I face these things, I tried to adapt myself to these light.

My first reaction was trial of dipper in night but nobody in this city of ‘Nazakat & Nafasat’ cared to respond. It only resulted in my being frustrated. I was not able to understand why people don’t respond to the dippers. Was there something wrong in my technique of doing or people comprehend them like some alien signals and decide to ignore them as accepting the presence of aliens may increase the already prevailing confusion of their lives. Next reaction was retaliation. I stopped giving and asking for dippers. I thought let them have a taste of their own medicine. To my surprise, I discovered that fact that eyes of all people are not alike. For few, light flashes at night are painful and for few they are pleasant. I also discovered the fact that giving straight lights to a bigger vehicle than yours might increase the speed of coming vehicle by some unknown mechanism. May be this law of reaction Newton forgot to discover….Eureka. My next reaction was of denial. When I faced lights, I told myself that it’s nothing. These may cause temporary blindness on roads but they won’t harm. That flashes may result in accidents but they won’t cause any damage to vision.

Between all these self interactions I also grew like my fellow city mates. Now I don’t give or ask for dippers at night. High intensity light flashes don’t disturb me. I just turn on one of the popular FM radio channel and drive absentmindedly and often I’m not able to recall how I reached home.

But every cloud has a silver lining. So even this city has few people, who know some driving etiquettes. Who give dippers in night. Give pass when asked according to the traffic rules. I often think of giving thanks to these people whenever I get dipper in night or get pass. But after asking from many learned people, I came to know that there is no sign in traffic books by which two vehicle drivers can say thank you to each other when they get good pass or dipper. It may not be a pressing concern for the city police currently celebrating traffic week. But there must be some way to express thank you to the fellow driver while driving if one appreciate other’s gesture.

Thanks for bearing with me.

Always allow the boss to speak first

A junior manager, a senior manager and their boss are on their way to a meeting. On their way through a park, they come across a wonder lamp.

They rub the lamp and a ghost appears. The ghost says, Normally, one is granted three wishes but as you are three, I will allow one wish each"

So the eager senior manager shouted, "I want the first wish. I want to be in the Bahamas, on a fast boat and have no worries"."Pfufffff and he was gone.

Now the junior manager could not keep quiet and shouted "I want to be in Florida with beautiful girls, plenty of food and cocktails". Pfufffff, and he was also gone.

The boss calmly said," I want these two idiots back in the office after lunch at 12.35pm"

Moral: "Always allow the boss to speak first"

Enthusiastic Salesman

A new vacuum cleaner salesman knocked on the door on the first house of the street. A tall lady answered the door.

Before she could speak, the enthusiastic salesman barged into the living room and opened a big black plastic bag and poured all the cow droppings onto the carpet.

" Madam , if I could not clean this up with the use of this new powerful vacuum cleaner, I will EAT all this S...!" exclaimed the eager salesman.

"Do you need chilli sauce or ketchup with that?" asked the lady.

The bewildered salesman asked, " Why, madam? "

"There's no electricity in the house.. ." said the lady

Learn To Admit Your Mistakes

One reason Hitler lost World War II was that he did not fully understand the situation. Bearers of bad news were punished. Soon no one dared tell him the truth. Not knowing the truth, he could not act appropriately.

Many of us are individually guilty of the same error. We do not like to admit to ourselves our mistakes, errors, shortcomings, or ever admit we have been in the wrong. And because we will not see the truth, we cannot act appropriately.

Someone has said that it is a good exercise to daily admit one painful fact about ourselves to ourselves.

Look for and seek out true information concerning yourself, your problems, other people, or situation, whether it is good news or bad news.

Adopt the motto – “It doesn’t matter who’s right, but what’s right.”

Admit your mistakes and errors but don’t cry over them. Correct them and go forward. In dealing with other people try to see the situation from their point of view as well as your own

10 Scientific Laws and Theories You Really Should Know..

1: Heisenberg's Uncertainty Principle

Einstein's broader theory of relativity told us more about how the universe works and helped to lay the foundation for quantum physics, but it also introduced more confusion into theoretical science. In 1927, this sense that the universe's laws were, in some contexts, flexible, led to a groundbreaking discovery by the German scientist Werner Heisenberg.

In postulating his Uncertainty Principle, Heisenberg realized that it was impossible to simultaneously know, with a high level of precision, two properties of a particle. In other words, you can know the position of an electron with a high degree of certainty, but not its momentum and vice versa.

Niels Bohr later made a discovery that helps to explain Heisenberg's principle. Bohr found that an electron has the qualities of both a particle and a wave, a concept known as wave-particle duality, which has become a cornerstone of quantum physics. So when we measure an electron's position, we are treating it as a particle at a specific point in space, with an uncertain wavelength. When we measure its momentum, we are treating it as a wave, meaning we can know the amplitude of its wavelength but not its location.

2: Theory of General Relativity

Albert Einstein's theory of general relativity remains an important and essential discovery because it permanently altered how we look at the universe. Einstein's major breakthrough was to say that space and time are not absolutes and that gravity is not simply a force applied to an object or mass. Rather, the gravity associated with any mass curves the very space and time (often called space-time) around it.

To conceptualize this, imagine you're traveling across theEarth in a straight line, heading east. After a while, if someone were to pinpoint your position on a map, you'd actually be both east and far south of your original position. That's because the Earth is curved. To travel directly east, you'd have to take into account the shape of the Earth and angle yourself slightly north. (Think about the difference between a flat paper map and a spherical globe.)

Space is pretty much the same. For example, to the occupants of the shuttle orbiting the Earth, it can look like they're traveling on a straight line through space. In reality, the space-time around them is being curved by the Earth's gravity (as it would be with any large object with immense gravity such as a planet or a black hole), causing them to both move forward and to appear to orbit the Earth.

Einstein's theory had tremendous implications for the future of astrophysics and cosmology. It explained a minor, unexpected anomaly in Mercury's orbit, showed how starlight bends and laid the theoretical foundations for black holes.

3: Evolution and Natural Selection

Now that we've established some of the fundamental concepts of how our universe began and how physics play out in our daily lives, let's turn our attention to the human form and how we got to be the way we are. According to most scientists, all life on Earth has a common ancestor. But in order to produce the immense amount of difference among all living organisms, certain ones had to evolve into distinct species.

In a basic sense, this differentiation occurred through evolution, through descent with modification [source: UCMP].Populations of organisms developed different traits, through mechanisms such as mutation. Those with traits that were more beneficial to survival such as, a frog whose brown coloring allows it to be camouflaged in a swamp, were naturally selected for survival; hence the term natural selection.

It's possible to expand upon both of these theories at greater length, but this is the basic, and groundbreaking, discovery that Darwin made in the 19th century: that evolution through natural selection accounts for the tremendous diversity of life on Earth.

4: Archimedes' Buoyancy Principle

After he discovered his principle of buoyancy, the ancient Greek scholar Archimedes allegedly yelled out "Eureka!" and ran naked through the city of Syracuse. The discovery was that important. The story goes that Archimedes made his great breakthrough when he noticed the water rise as he got into the tub [source: Quake].

According to Archimedes' buoyancy principle, the force acting on, or buoying, a submerged or partially submerged object equals the weight of the liquid that the object displaces. This sort of principle has an immense range of applications and is essential to calculations of density, as well as designing submarines and other oceangoing vessels.

5: Laws of Thermodynamics

The British physicist and novelist C.P. Snow once said that a nonscientist who didn't know the second law of thermodynamics was like a scientist who had never read Shakespeare [source: Lambert]. Snow's now-famous statement was meant to emphasize both the importance of thermodynamics and the necessity for nonscientists to learn about it.

Thermodynamics is the study of how energy works in a system, whether it's an engine or the Earth's core. It can be reduced to several basic laws, which Snow cleverly summed up as follows [source: Physics Planet]:

·         You can't win.

·         You can't break even.

·         You can't quit the game.

Let's unpack these a bit. By saying you can't win, Snow meant that since matter and energy are conserved, you can't get one without giving up some of the other (i.e., E=mc²). It also means that for an engine to produce work, you have to supply heat, although in anything other than a perfectly closed system, some heat is inevitably lost to the outside world, which then leads to the second law.

The second statement -- you can't break even -- means that due to ever-increasing entropy, you can't return to the same energy state. Energy concentrated in one place will always flow to places of lower concentration.

Finally, the third law -- you can't quit the game -- refers to absolute zero, the lowest theoretical temperature possible, measured at zero Kelvin or (minus 273.15 degrees Celsius and minus 459.67 degrees Fahrenheit). When a system reaches absolute zero, molecules stop all movement, meaning that there is no kinetic energy, and entropy reaches its lowest possible value. But in the real world, even in the recesses of space, reaching absolutely zero is impossible -- you can only get very close to it.

6: Newton's Laws of Motion

As long as we're talking about one of the greatest scientists who ever lived, let's move on to Newton's other famous laws. His three laws of motion form an essential component of modern physics. And like many scientific laws, they're rather elegant in their simplicity.

The first of the three laws states an object in motion stays in motion unless acted upon by an outside force. For a ball rolling across the floor, that outside force could be the friction between the ball and the floor, or it could be the toddler that kicks the ball in another direction.

The second law establishes a connection between an object's mass (m) and its acceleration (a), in the form of the equation F = m × a. F represents force, measured in Newtons. It's also a vector, meaning it has a directional component. Owing to its acceleration, that ball rolling across the floor has a particular vector, a direction in which it's traveling, and it's accounted for in calculating its force.

The third law is rather pithy and should be familiar to you: For every action there is an equal and opposite reaction. That is, for every force applied to an object or surface, that object pushes back with equal force.

7: Universal Law of Gravitation

We may take it for granted now, but more than 300 years ago Sir Isaac Newton proposed a revolutionary idea: that any two objects, no matter their mass, exert gravitational force toward one another. This law is represented by an equation that many high schoolers encounter in physics class. It goes as follows:

F = G × [(m1m2)/r²]

F = G × [(m₁m₂)/r²]

F is the gravitational force between the two objects, measured in Newtons. M₁ and m₂ are the masses of the two objects, while r is the distance between them.G is the gravitational constant, a number currently calculated to be 6.672 × 10-¹¹ N m² kg^-2 [source:Weisstein].

The benefit of the universal law of gravitation is that it allows us to calculate the gravitational pull between any two objects. This ability is especially useful when scientists are, say, planning to put a satellite in orbit or charting the course of the moon.

8: Kepler's Laws of Planetary Motion

For centuries, scientists battled with one another and with religious leaders about the planets' orbits, especially about whether they orbited our sun. In the 16th century, Copernicus put forth his controversial concept of a heliocentric solar system, in which the planets revolved around the sun -- not the Earth. But it would take Johannes Kepler, building on work performed by Tyco Brahe and others, to establish a clear scientific foundation for the planets' movements.

Kepler's three laws of planetary motion -- formed in the early 17th century -- describe how planets orbit the sun. The first law, sometimes called the law of orbits, states that planets orbit the sun elliptically. The second law, the law of areas, states that a line connecting a planet to the sun covers an equal area over equal periods of time. In other words, if you're measuring the area created by drawing a line from the Earth to the sun and tracking the Earth's movement over 30 days, the area will be the same no matter where the Earth is in its orbit when measurements begin.

The third one, the law of periods, allows us to establish a clear relationship between a planet's orbital period and its distance from the sun. Thanks to this law, we know that a planet relatively close to the sun, like Venus, has a far briefer orbital period than a distant planet, such as Neptune.

9: Hubble's Law of Cosmic Expansion

Let's stick with Edwin Hubble for a second. While the 1920s roared past and the Great Depression limped by, Hubble was performing groundbreaking astronomical research. Hubble not only proved that there were other galaxies besides theMilky Way, he also discovered that these galaxies were zipping away from our own, a motion he called recession.

In order to quantify the velocity of this galactic movement, Hubble proposed Hubble's Law of Cosmic Expansion, aka Hubble's law, an equation that states: velocity = H₀ ×distance. Velocity represents the galaxy's recessional velocity; H₀ is the Hubble constant, or parameter that indicates the rate at which the universe is expanding; and distance is the galaxy's distance from the one with which it's being compared.

Hubble's constant has been calculated at different values over time, but the current accepted value is 70 kilometers/second per megaparsec, the latter being a unit of distance in intergalactic space [source:White]. For our purposes, that's not so important. What matters most is that Hubble's law provides a concise method for measuring a galaxy's velocity in relation to our own. And perhaps most significantly, the law established that the universe is made up of many galaxies, whose movements trace back to the big bang.

10: Big Bang Theory

If you're going to know one scientific theory, make it the one that explains how the universe arrived at its present state. Based on research performed by Edwin Hubble, Georges Lemaitre and Albert Einstein, among others, the big bang theory postulates that the universe began almost 14 billion years ago with a massive expansion event. At the time, the universe was confined to a single point, encompassing all of the universe's matter. That original movement continues today, as the universe keeps expanding outward.

The theory of the big bang gained widespread support in the scientific community after Arno Penzias and Robert Wilson discovered cosmic microwave background radiation in 1965. Using radio telescopes, the two astronomers detected cosmic noise, or static, that didn't dissipate over time. Collaborating with Princeton researcher Robert Dicke, the pair confirmed Dicke's hypothesis that the original big bang left behind low-level radiation detectable throughout the universe.

true love

Being deeply loved by someone gives you strength, while loving someone deeply gives you courage