The universe is incomprehensively vast. Nonetheless, some day it will cease to exist as we currently perceive it. The sun will use up all its fuel and die in about 5 billion years or so. At that time the solar system will no longer be habitable. Will humans be around at that time? No one knows.
The theory that currently has the most support in explaining what we think will end the universe is one called "The Big Freeze". The big freeze theory claims that the universe will continue to expand until it reaches nearly absolute zero and all things cease to move. This is supposed to happen in about 10100 years. For comparison the universe is currently 13.7 Billion years old (13,700,000,000) where as the big freeze would happen in approximately 10100 (100,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000, 000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000) years, and the entire history of the human race is a mere 200,000 years.
It is important to note that even if/when the big freeze occurred, the universe would still exist. it would merely be lifeless and void of all movement. Also, because matter and energy are nearly synonymous as far as physics is concerned (E=mc^2), there would still be movement on a super-subatomic level. The most recent theory regarding this being the string theory, but back to the main question.
It is possible to theorize that since the universe has a defined beginning, as calculated by Stephen Hawking, that it could have a legitimate end as well. speaking purely philosophically, it would seem that a finite universe, which has a beginning, may necessarily have an end that we do not know; the other theory would be that the universe could cease to exist upon the same grounds, which brought it into existence. I speak philosophically here because physics cannot be used to define knowledge of events that took place outside of our universe and thus outside of our laws and confines of natural science
Answer: No, the universe is Bounded, no beginning or end.
The Universe will change not cease to exist.
Answer: Although the Universe has a clear beginning (with the Big Bang), it seems it won't have a clearly-defined end - it will just continue expanding. However, a time will come when it won't be able to support any type of life, because of the Second Law of Thermodynamics. In other words, all useful energy will have been used up.
Dark energy. The current estimates for the distribution of mass/energy in the Universe are approximately: 68% dark energy 27% dark matter 5% baryonic (i.e. "normal") matter
Dark energy.
There are several pieces of evidence for dark matter. For example: * Our galaxy, and many other galaxies, rotate way too fast for the amount of known matter. * Evidence from gravitational lensing.
Dark Universe - film - was created in 1993.
No. It's generally believed that the universe has insufficient mass density to slow or halt its expansion (and in fact, there's some evidence that the rate of expansion is actually increasing due to "dark energy", which is a slightly more academically acceptable way of saying "we don't know what").Excellent answer!The Universe (our universe) will probably end in a «Big RIP» or a «Big Freeze» scenario, after the «Dark Era and Photon Age», about 10100 years from now.Please rememer that after the «Dark Era» age, what happens after this is speculative.There could even occur a new «Big Bang», supereons after the «Dark Era».Or else the «String Theory» is correct, and our universe is a «membane», or «Brane», and may collide with another «brane» sooner, creating a new universe, God nows what type of universe would be created...
Dark energy -- whatever it turns out to be -- constitutes about 74% of the energy in our Universe.
Yes. Dark energy is responsible for the expansion of the universe.
The Universe contains matter, energy, dark matter, dark energy, empty space - and of course, lots of structures made up of those.The Universe contains matter, energy, dark matter, dark energy, empty space - and of course, lots of structures made up of those.The Universe contains matter, energy, dark matter, dark energy, empty space - and of course, lots of structures made up of those.The Universe contains matter, energy, dark matter, dark energy, empty space - and of course, lots of structures made up of those.
Dark energy. The current estimates for the distribution of mass/energy in the Universe are approximately: 68% dark energy 27% dark matter 5% baryonic (i.e. "normal") matter
No. What is killing the Universe is the Second Law of Thermodynamics.
Dark energy is the force that is driving the expansion of the universe
The mysterious substance which is believed to accelerate the Universe's expansion. Look up "dark energy" on Wikipedia for more details.
there are the energy that mostly makes up this universe and its had been here since the beginning of the universe and also they are invisible.
Negative energy and dark energy are two distinct concepts in physics. Negative energy refers to a theoretical concept where energy levels are below zero, which is not observed in nature. On the other hand, dark energy is a mysterious force that is thought to be responsible for the accelerating expansion of the universe. While negative energy is not directly observed, dark energy has a significant impact on the dynamics of the universe by counteracting the gravitational pull of matter and causing the universe to expand at an increasing rate.
The one where the universe is expanding and accelerating.
Current theory states that it's "dark energy".
The energy in the universe is primarily distributed across three main components: dark energy, dark matter, and ordinary matter. Dark energy, which comprises about 68% of the universe's total energy content, is thought to drive the accelerated expansion of the universe. Dark matter accounts for about 27% and plays a crucial role in the structure formation of galaxies and galaxy clusters. Ordinary matter, including stars, planets, and interstellar gas, makes up only about 5% of the total energy density, highlighting the dominance of dark components in cosmic energy distribution.