The universe is a vast and awe-inspiring place, filled with wonders that have captivated humanity for millennia. While scientists have made incredible strides in understanding the cosmos, some phenomena remain stubbornly mysterious. You’re here because you’re curious about what makes these cosmic events so difficult to explain, and we’ll explore exactly that.
Before diving into specific mysteries, it’s helpful to understand the core challenges astronomers face. The complexity of these phenomena isn’t just about the events themselves, but also about the incredible difficulty of observing them.
One of the most profound mysteries in all of science is dark matter. It is the invisible substance that scientists believe makes up about 27% of the universe. We know it’s there, but we have no idea what it is.
In the 1970s, astronomer Vera Rubin was studying the rotation of galaxies. She expected to see stars on the outer edges moving slower than stars near the center, just as outer planets in our solar system move slower than inner planets. Instead, she found that the outer stars were moving just as fast as the inner ones. This was a huge shock. The only way to explain this speed was if there was a massive, invisible halo of matter surrounding the galaxy, providing the extra gravitational pull needed to keep those speedy stars in orbit.
The problem with dark matter is that it doesn’t seem to interact with light or any other form of electromagnetic radiation. It doesn’t shine, it doesn’t reflect, and it doesn’t cast a shadow. It’s completely invisible to all our telescopes. Its existence is only inferred through its gravitational effects on the things we can see, like stars and galaxies. Scientists around the world are running complex experiments deep underground, like the Large Underground Xenon (LUX) experiment, trying to catch a dark matter particle as it passes through the Earth, but so far, they have found nothing.
If dark matter is the universe’s invisible glue, dark energy is its mysterious accelerator. Scientists believe it makes up a staggering 68% of the universe, and it’s responsible for one of the most surprising discoveries in modern astronomy.
For most of the 20th century, astronomers debated whether the expansion of the universe, which started with the Big Bang, was slowing down. They assumed gravity would eventually put the brakes on everything. In 1998, two separate teams of scientists studying distant supernovae (exploding stars) made a revolutionary discovery. They found that not only is the universe not slowing down, but its expansion is actually speeding up. The farther away a galaxy is, the faster it is moving away from us.
There is no explanation for this accelerated expansion in our current understanding of physics. Scientists have named the unknown force causing it “dark energy,” but giving it a name doesn’t explain what it is. Is it an inherent property of space itself, a “cosmological constant” as Einstein once proposed? Or is it a new type of energy field that permeates the entire cosmos? We don’t know. Because it’s a gentle, uniform push spread across the entire universe, it’s incredibly difficult to study and measure on any local scale.
Imagine a flash of light from a distant galaxy that, for a few thousandths of a second, releases as much energy as our sun does in three days. Now imagine that flash isn’t light, but radio waves. That’s a Fast Radio Burst, or FRB.
The first FRB was discovered in 2007, and since then, we’ve detected hundreds more. They are extremely powerful, incredibly brief, and come from billions of light-years away. Some FRBs repeat from the same location, while others seem to be one-off events. The Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope has been particularly successful at detecting them.
The sheer energy required to produce an FRB is mind-boggling, which severely limits the possible sources. The leading theory is that they are created by magnetars, which are young neutron stars with unimaginably powerful magnetic fields. However, this theory doesn’t perfectly explain all the different types of FRBs we’ve seen. The brevity of the events makes them very difficult to catch and study in detail. Pinpointing their exact origin galaxy is a monumental task that requires coordinating multiple radio telescopes around the world.
What’s the difference between dark matter and dark energy? Think of it this way: Dark matter is an attractive force. Its gravity pulls galaxies together and holds them in shape. Dark energy is a repulsive force. It pushes everything apart, causing the expansion of the universe to accelerate. They are two separate, massive mysteries.
Could any of these be signs of alien life? While it’s a fascinating thought, scientists always look for natural explanations first. For something like FRBs, a natural source like a magnetar is considered far more likely than an alien signal. The famous “Wow! Signal” from 1977 is a better candidate for a potential alien signal, but because it was a one-time event that has never been detected again, it remains an unsolved and intriguing cosmic puzzle.
How do we know these things exist if we can’t see them? This is the core of modern astrophysics. We know they exist through indirect evidence. We can’t see the wind, but we can see the trees moving and feel it on our skin. Similarly, we can’t see dark matter, but we can see its gravitational pull on the stars we can see. We can’t see dark energy, but we can measure its effect on the expansion of the entire universe.