Explore the Unknown

In the realm of theoretical physics, few objects are as mysterious as white holes. While black holes are well-documented cosmic bodies that trap everything—including light—white holes are their mathematical opposites. They are solutions to Einstein's equations that expel matter and energy, and nothing can enter them.

But do white holes actually exist in our universe? Or are they merely mathematical curiosities? Let’s explore the origins, theories, and challenges of white holes.

For decades, black holes were thought to be destructive monsters, devouring everything in their path. But recent discoveries have revealed a much more complex role for these cosmic objects: black holes help regulate the life cycles of galaxies, including how and when stars are born.

This article explores how black holes, particularly supermassive black holes at the centers of galaxies, influence galactic structure and star formation through gravitational forces, energy feedback, and cosmic regulation.

When we think of extreme phenomena in the universe, black holes and supernovae often come to mind. But beyond these well-known cosmic giants lie even stranger, more powerful, and lesser-known objects. In this article, we’ll explore some of the most extreme astrophysical phenomena—including quasars, magnetars, blazars, neutron star collisions, and gamma-ray bursts—that push the boundaries of what we understand about physics and space.

Mini black holes remain one of the most fascinating and elusive possibilities in modern astrophysics. Though we have yet to detect them, their existence could explain some of the universe’s greatest mysteries—from the nature of dark matter to the conditions of the early cosmos.

As observational techniques continue to advance, the next decade may finally reveal whether these tiny black holes are out there—and whether they are shaping the universe in subtle, invisible ways.

The solar system as we know it—containing the Sun, eight planets, moons, asteroids, and comets—was born over 4.5 billion years ago from a cloud of gas and dust. This process, called solar system formation, is supported by astronomical observations, computer simulations, and analysis of meteorites.

For over 75 years, Pluto was considered the ninth planet of our solar system. Discovered in 1930 by American astronomer Clyde Tombaugh, Pluto held a special place in textbooks, science museums, and popular culture. But in 2006, the International Astronomical Union (IAU) reclassified Pluto as a “dwarf planet,” triggering a wave of public confusion and debate.

So what really happened? Why was Pluto stripped of its planetary status? Here’s the real, science-based explanation.