Danesh Kumar Thiyagarajan
Stories (9/0)
How does memory works
In the realm of cognition, the human brain remains an uncharted frontier, giving rise to questions that tantalize and intrigue. Among these inquiries, the nature of memory has been a subject of fascination for generations. As we delve into the labyrinthine corridors of memory, we uncover theories that offer us a glimpse into the intricate workings of our minds.
By Danesh Kumar Thiyagarajan9 months ago in Humans
Why do we dream
Throughout history, the enigmatic nature of dreams has captivated human minds. From ancient civilizations to modern scientific research, the quest to understand why we dream has been a journey filled with intriguing theories and captivating insights.
By Danesh Kumar Thiyagarajan9 months ago in FYI
Joey in "FRIEND"
Joey Tribbiani, portrayed by Matt LeBlanc, is one of the most beloved and memorable characters from the iconic television series "Friends." With his endearing personality, distinct catchphrases, and unwavering loyalty, Joey brings a unique charm to the show that has left a lasting impact on fans around the world.
By Danesh Kumar Thiyagarajan9 months ago in Fiction
A boy named Ethan
In the quiet town of Willowbrook, where the streets were lined with houses that seemed to harbor secrets, lived a boy named Ethan. He was a solitary figure, often seen wandering through the town's serene park, lost in his own thoughts. Ethan's eyes held a melancholic depth, a reflection of a sorrow he carried within.
By Danesh Kumar Thiyagarajan9 months ago in Families
How Will Our Universe End?
We're all familiar with the concept of the Big Bang, and it's quite disheartening that the popular TV series "The Big Bang Theory" has come to an end. However, let's steer away from the candy bars and delve into a different aspect – the Big Crunch. While most people have heard of the Big Bang, fewer are acquainted with the Big Crunch. Despite various theories like the Big Freeze and the Big Rip, the Big Crunch stands out as the most plausible scenario for the eventual fate of the universe.
By Danesh Kumar Thiyagarajan9 months ago in Earth
What Happens To Your Body 100 Years After Death
Your body is a complex composition, comprising over 200 bones, trillions of microbes, and as many as 37 trillion cells. While death is often perceived as the end of an individual's existence, the body still undergoes a significant journey after the cessation of life. Shortly after death, the brain is one of the first components to deteriorate. When the heart stops beating, blood flow ceases, preventing the delivery of oxygen to organs and tissues. Consequently, the most active and oxygen-dependent parts of the body start to degrade. This process leads to the release of fluids, given that these organs and tissues consist of about 70% water. Without oxygen, cells undergo self-destruction, causing fluids to seep onto the surface.
By Danesh Kumar Thiyagarajan9 months ago in Humans
The most valuable place in space
Ever since the inaugural launch of an artificial satellite in 1957, various entities like governments, corporations, and research institutions have staked their claims in the cosmic expanse. Although space may appear boundless, certain regions in this vast arena hold more significance than others. These specific spots are known as Lagrange points, and when it comes to the realm of human space exploration, they could very well be the most critical locales within our solar system. Named after an 18th-century mathematician who discerned their positions, Lagrange points are unique pockets of equilibrium in our ever-shifting universe. The gravitational force exerted by celestial bodies affects objects in their proximity, pulling them into and out of orbits. Alongside various apparent forces, gravity shapes the nature of these orbits. However, Lagrange points emerge as the places where all these influences find equilibrium. In essence, they serve as celestial parking spots—once an object occupies a Lagrange point, minimal energy is needed to maintain its position. Consequently, whenever humans seek to anchor an object in a stable location without excessive fuel consumption, these points become paramount.
By Danesh Kumar Thiyagarajan9 months ago in Earth
Where Did the Titanic Iceberg Really Come From?
A beam of electric light pierces the darkness above the serene waters of the Atlantic Ocean. The Titanic sails quietly through the waves, its passengers asleep. Suddenly, a colossal white figure appears in the light beam – the faithful iceberg is about to collide with the legendary ship. This event occurred on April 14, 1912, just two days before an unusual elliptically shaped iceberg would be photographed. This iceberg, formed from snow that fell 100,000 years ago, likely originated from a cluster of glaciers in Southwest Greenland. Modern computer modeling and historical data help trace its journey.
By Danesh Kumar Thiyagarajan9 months ago in History
What if planets were triangles or cubes?
Have you ever wondered about the intriguing spherical shape of all planets? Imagine if these celestial objects decided to challenge convention and adopt different forms. Could we end up with cube-shaped planets, triangular moons, or even unimaginable intergalactic structures? Let's dive into this concept. So, how do planets actually come into existence? The universe contains massive clouds of dust and gas, known as molecular clouds, consisting of various elements like hydrogen, helium, carbon, and oxygen. These clouds act like a cosmic kitchen, providing the ingredients necessary for creating new planets. The initial step in forming planets is known as the accretion theory. Consider a scenario where an event triggers gravitational instability, perhaps a nearby supernova explosion. This disturbance causes the gas and dust within the cloud to come together due to gravity. These particles start to gather around a central point, much like squeezing a ball in your hand. Over time, they compact tightly, causing the cloud to flatten and form a disk shape, much like mixing flour and water to make pizza dough. This resulting disk is referred to as a protoplanetary disk, and its rotation is a consequence of the initial spin of the cloud particles. Visualize tiny dust particles and gas molecules dancing within the disk. Occasionally, they collide and stick together, forming clumps called planetesimals—these serve as the fundamental building blocks of planets. Through subsequent collisions and mergers, these planetesimals gradually grow larger, evolving into protoplanets. As these protoplanets gain mass, their gravitational pull intensifies, making them the dominant entities within their cosmic realms—the planets we're familiar with. Each planet possesses its own unique combination of gases, rocks, and potentially water. But what's responsible for the planets' spherical appearance? This is primarily due to gravity. Imagine squeezing a balloon—the air inside resists this pressure, resulting in equilibrium. Similarly, on planets, gravity compresses material inward, while the material's pressure pushes outward, counteracting the force of gravity. This balance is referred to as hydrostatic equilibrium. Another contributor to the spherical shape is the planet's rotation. Think of a rapidly spinning ball of Play-Doh—the material at the equator pushes outward, causing a bulge, while the poles flatten. The same principle applies to planets as they rotate on their axes. The interplay of gravity and rotation leads to a bulging effect at the equator, giving planets their spherical form. This unique interplay of factors is responsible for their distinct appearance. However, what if planets were not spherical? What if they took on cube-shaped or triangular forms? If a celestial body deviates from a sphere, its mass distribution changes significantly, impacting gravity. On a cube or triangle-shaped planet, gravity would vary across its surface. Standing at the center of a face, you'd feel the strongest gravitational pull, as the faces are closest to the center of mass. As you move toward the edges or corners, gravity's angle becomes steeper, much like ascending a mountain or steep slope. Water and atmosphere distribution would also change, rendering certain regions inhospitable due to extreme climates and reduced atmospheric pressure. To conclude, while our Earth embraces its spherical form, contemplating alternative shapes lets our imagination run wild. This exploration prompts us to appreciate the wonders of our remarkable planet, regardless of its shape.
By Danesh Kumar Thiyagarajan9 months ago in Earth