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BUILD SO MANY UNDERGROUND MRT STATIONS, WHAT IF ONE DAY GLOBAL WARMING THE ISLAND SINK AND ALL THE MRT STATION FLOODED WITH WATER?

That's why it's a waste of money digging here n there, lol, they will tell u they will flood prevention lol
 
Presently, many (if not all) underground MRT stations are below sea level.
No need to wait for global warming floods.
How?
 
Only the silly ones will echo a hoax.

The earth is not going to last forever because our sun, which is star, will not last forever. All stars go through death throes when the fuel runs out.

Screenshot 2025-02-27 at 4.55.36 PM.png
 
Is that an evidence or a theory?

The life cycle of stars has been studied extensively and there is evidence from the life cycle of other stars in the universe that our sun will follow the same life cycle.

Unless the laws of physics change along the way I don't see any reason why the outcome will be different in our solar system.
 
Looks like there are some dimwits who still believe the anti-carbon cult. :roflmao:
 
The life cycle of stars has been studied extensively and there is evidence from the life cycle of other stars in the universe that our sun will follow the same life cycle.

Unless the laws of physics change along the way I don't see any reason why the outcome will be different in our solar system.
Yes, please show us the evidence produced using scientific method.
 
Only the silly ones will echo a hoax.

The earth is not going to last forever because our sun, which is star, will not last forever. All stars go through death throes when the fuel runs out.

From ChatGPT,

A star's life cycle is a fascinating journey that spans millions to billions of years, depending on its size. Here's how it typically unfolds:

It all begins with a nebula, a vast cloud of gas and dust in space. Under the influence of gravity, this cloud starts to collapse, forming a dense core. As the core heats up and contracts, it becomes a protostar—a hot, glowing object that’s not yet a full-fledged star. This stage can last for tens of thousands to millions of years.

Once the core gets hot enough—around 10 million degrees Celsius—nuclear fusion kicks in. Hydrogen atoms fuse into helium, releasing a tremendous amount of energy in the form of light and heat. At this point, the protostar ignites and becomes a main sequence star, like our Sun. This is the longest phase of a star’s life, lasting millions to billions of years, depending on its mass. Smaller stars burn cooler and slower, while massive stars burn hotter and faster.

When the hydrogen fuel starts running low, the star’s core contracts under gravity, and its outer layers expand. For a star like the Sun, this marks the red giant phase. The core keeps fusing helium into heavier elements like carbon and oxygen, while the outer layers swell up to hundreds of times the star’s original size. This phase lasts a few million years.

What happens next depends on the star’s mass. For a medium-sized star like the Sun, the outer layers eventually drift away as a beautiful planetary nebula, leaving behind a hot core that cools and shrinks into a white dwarf. Over billions of years, the white dwarf fades into a cold, dark black dwarf.

Massive stars—those at least eight times the Sun’s mass—go out with a bang. After exhausting their fuel, their cores collapse under intense gravity, triggering a supernova explosion. This blast scatters heavy elements like iron into space, enriching the cosmos. What’s left behind could be a neutron star, a super-dense object made mostly of neutrons, or, if the star was massive enough, a black hole, where gravity is so strong that not even light can escape.

So, in summary: nebula to protostar, main sequence star, red giant or supergiant, then either a white dwarf or an explosive supernova leading to a neutron star or black hole. The cycle’s length and endgame hinge on the star’s starting mass—small stars fade quietly, while big ones exit in a cosmic spectacle!
 
The earth is not going to last forever because our sun, which is star, will not last forever. All stars go through death throes when the fuel runs out.

From ChatGPT,

A star's life cycle is a fascinating journey that spans millions to billions of years, depending on its size. Here's how it typically unfolds:

It all begins with a nebula, a vast cloud of gas and dust in space. Under the influence of gravity, this cloud starts to collapse, forming a dense core. As the core heats up and contracts, it becomes a protostar—a hot, glowing object that’s not yet a full-fledged star. This stage can last for tens of thousands to millions of years.

Once the core gets hot enough—around 10 million degrees Celsius—nuclear fusion kicks in. Hydrogen atoms fuse into helium, releasing a tremendous amount of energy in the form of light and heat. At this point, the protostar ignites and becomes a main sequence star, like our Sun. This is the longest phase of a star’s life, lasting millions to billions of years, depending on its mass. Smaller stars burn cooler and slower, while massive stars burn hotter and faster.

When the hydrogen fuel starts running low, the star’s core contracts under gravity, and its outer layers expand. For a star like the Sun, this marks the red giant phase. The core keeps fusing helium into heavier elements like carbon and oxygen, while the outer layers swell up to hundreds of times the star’s original size. This phase lasts a few million years.

What happens next depends on the star’s mass. For a medium-sized star like the Sun, the outer layers eventually drift away as a beautiful planetary nebula, leaving behind a hot core that cools and shrinks into a white dwarf. Over billions of years, the white dwarf fades into a cold, dark black dwarf.

Massive stars—those at least eight times the Sun’s mass—go out with a bang. After exhausting their fuel, their cores collapse under intense gravity, triggering a supernova explosion. This blast scatters heavy elements like iron into space, enriching the cosmos. What’s left behind could be a neutron star, a super-dense object made mostly of neutrons, or, if the star was massive enough, a black hole, where gravity is so strong that not even light can escape.

So, in summary: nebula to protostar, main sequence star, red giant or supergiant, then either a white dwarf or an explosive supernova leading to a neutron star or black hole. The cycle’s length and endgame hinge on the star’s starting mass—small stars fade quietly, while big ones exit in a cosmic spectacle!
This one is rubbish if it cannot be translated to physical evidence observed by anyone

Many sheeple are going to be brainwashed to “believe” AI bots because the AI bots said so.

This is how education will be like in future
 
This one is rubbish if it cannot be translated to physical evidence observed by anyone

Many sheeple are going to be brainwashed to “believe” AI bots because the AI bots said so.

This is how education will be like in future

The laws of physics are used to create technology that you are typing on now. All the integrated circuits in your electronic devices are designed based upon the same physical laws that govern our universe. If they were wrong nothing that matters in today's world would work.

Even the laws of relativity postulated by Einstein have been proven correct and are factored into GPS devices in order to correct for relativity.

All these physical laws at both newtonian and quantum level were verified and used in applications long before AI was even heard of.
 
The laws of physics are used to create technology that you are typing on now. All the integrated circuits in your electronic devices are designed based upon the same physical laws that govern our universe. If they were wrong nothing that matters in today's world would work.

Even the laws of relativity postulated by Einstein have been proven correct and are factored into GPS devices in order to correct for relativity.

All these physical laws at both newtonian and quantum level were verified and used in applications long before AI was even heard of.
If you can’t produce physical evidence for observation, measurements and experiments, you can write whatever theory that pleases you
 
If you can’t produce physical evidence for observation, measurements and experiments, you can write whatever theory that pleases you

The physical evidence is the fact that theories, when applied, actually work in real life. That's how all facts are established.

As time goes by we may find out even more about why things work the way they do but that does not make the original equations wrong all it does is add more factors to the equation.

EG Newton's equations did not factor in relativity but when Einstein came along and showed how time dilated and contracted it added to our understanding of the physical world but did not displace Newton's laws at low speeds relative to light.
 
The physical evidence is the fact that theories, when applied, actually work in real life. That's how all facts are established.

As time goes by we may find out even more about why things work the way they do but that does not make the original equations wrong all it does is add more factors to the equation.

EG Newton's equations did not factor in relativity but when Einstein came along and showed how time dilated and contracted it added to our understanding of the physical world but did not displace Newton's laws at low speeds relative to light.
Your understanding with these is called scientism. Scientism is a belief system that doesn’t need any individuals to conduct science themselves but rather believing that the “scientists” have already done it for you. So believe the “scientists” will do.

Real science is for everyone who can observe, demonstrate, experiencing themselves and find out the outcomes for themselves
 
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