In 1927, an astronomer named Georges Lemaître had a big idea. He said that a very long time ago, the universe started as just a single point. He said the universe stretched and expanded to get as big as it is now, and that it could keep on stretching.

What an Idea!

The universe is a very big place, and it’s been around for a very long time. Thinking about how it all started is hard to imagine.

Some More Information

Just two years later, an astronomer named Edwin Hubble noticed that other galaxies were moving away from us. And that’s not all. The farthest galaxies were moving faster than the ones close to us.

This meant that the universe was still expanding, just like Lemaître thought. If things were moving apart, it meant that long ago, everything had been close together.

Everything we can see in our universe today—stars, planets, comets, asteroids—they weren't there at the beginning. Where did they come from?

A Tiny, Hot Beginning

When the universe began, it was just hot, tiny particles mixed with light and energy. It was nothing like what we see now. As everything expanded and took up more space, it cooled down.

The tiny particles were grouped. They formed atoms. Then those atoms grouped together. Over lots of time, atoms came together to form stars and galaxies.

The first stars created bigger atoms and groups of atoms called molecules. That led to more stars being born. At the same time, galaxies were crashing and grouping together. As new stars were being born and dying, then things like asteroids, comets, planets, and black holes formed!

A Super Long Time

How long did all of this take? Well, we now know that the universe is 13,800,000,000 years old—that’s 13.8 billion. That is a very long time.

What's in a Name?

That’s pretty much how the universe began. Because it got so big and led to such great things, some people call it the "Big Bang." But maybe a better name would be the "Everywhere Stretch." What do you think?

https://spaceplace.nasa.gov/big-bang/en/

A 2013 map of the background radiation leftover from the Big Bang, taken by the ESA's Planck spacecraft, captured the oldest light in the universe. This information helps astronomers determine the age of the universe.

The Big Bang Theory is the leading explanation about how the universe began. At its simplest, it says the universe as we know it started with a small singularity, then inflated over the next 13.8 billion years to the cosmos that we know today.

Because current instruments don't allow astronomers to peer back at the universe's birth, much of what we understand about the Big Bang Theory comes from mathematical formulas and models. Astronomers can, however, see the "echo" of the expansion through a phenomenon known as the cosmic microwave background.

While the majority of the astronomical community accepts the theory, there are some theorists who have alternative explanations besides the Big Bang — such as eternal inflation or an oscillating universe.

The phrase "Big Bang Theory" has been popular among astrophysicists for decades, but it hit the mainstream in 2007 when a comedy show with the same name premiered on CBS. The show follows the home and academic life of several researchers (including an astrophysicist).

The first second, and the birth of light

In the first second after the universe began, the surrounding temperature was about 10 billion degrees Fahrenheit (5.5 billion Celsius), according to NASA. The cosmos contained a vast array of fundamental particles such as neutrons, electrons, and protons. These decayed or combined as the universe got cooler.

This early soup would have been impossible to look at because light could not carry inside of it. "The free electrons would have caused light (photons) to scatter the way sunlight scatters from the water droplets in clouds," NASA stated. Over time, however, the free electrons met up with nuclei and created neutral atoms. This allowed light to shine through about 380,000 years after the Big Bang.

This early light — sometimes called the "afterglow" of the Big Bang — is more properly known as the cosmic microwave background (CMB). It was first predicted by Ralph Alpher and other scientists in 1948 but was found only by accident almost 20 years later. [Images: Peering Back to the Big Bang & Early Universe]

Arno Penzias and Robert Wilson, both of Bell Telephone Laboratories in Murray Hill, New Jersey, were building a radio receiver in 1965 and picking up higher-than-expected temperatures, according to NASA. At first, they thought the anomaly was due to pigeons and their dung, but even after cleaning up the mess and killing pigeons that tried to roost inside the antenna, the anomaly persisted.

Simultaneously, a Princeton University team (led by Robert Dicke) was trying to find evidence of the CMB and realized that Penzias and Wilson had stumbled upon it. The teams each published papers in the Astrophysical Journal in 1965.

Determining the age of the universe

The cosmic microwave background has been observed on many missions. One of the most famous space-faring missions was NASA's Cosmic Background Explorer (COBE) satellite, which mapped the sky in the 1990s.

Several other missions have followed in COBE's footsteps, such as the BOOMERanG experiment (Balloon Observations of Millimetric Extragalactic Radiation and Geophysics), NASA's Wilkinson Microwave Anisotropy Probe (WMAP), and the European Space Agency's Planck satellite.

Planck's observations, first released in 2013, mapped the background in unprecedented detail and revealed that the universe was older than previously thought: 13.82 billion years old, rather than 13.7 billion years old. [Related: How Old is the Universe?] (The research observatory's mission is ongoing and new maps of the CMB are released periodically.)

The maps give rise to new mysteries, however, such as why the Southern Hemisphere appears slightly redder (warmer) than the Northern Hemisphere. The Big Bang Theory says that the CMB would be mostly the same, no matter where you look.

Examining the CMB also gives astronomers clues as to the composition of the universe. Researchers think most of the cosmos is made up of matter and energy that cannot be "sensed" with conventional instruments, leading to the names of dark matter and dark energy. Only 5 percent of the universe is made up of matter such as planets, stars, and galaxies.

Gravitational waves controversy

While astronomers could see the universe's beginnings, they've also been seeking out proof of its rapid inflation. The theory says that in the first second after the universe was born, our cosmos ballooned faster than the speed of light. That, by the way, does not violate Albert Einstein's speed limit since he said that light is the maximum anything can travel within the universe. That did not apply to the inflation of the universe itself.

In 2014, astronomers said they had found evidence in the CMB concerning "B-modes," a sort of polarization generated as the universe got bigger and created gravitational waves. The team spotted evidence of this using an Antarctic telescope called "Background Imaging of Cosmic Extragalactic Polarization", or BICEP2.

"We're very confident that the signal that we're seeing is real, and it's on the sky," lead researcher John Kovac, of the Harvard-Smithsonian Center for Astrophysics, told Space.com in March 2014.

But by June, the same team said that their findings could have been altered by galactic dust getting in the way of their field of view.

"The basic takeaway has not changed; we have high confidence in our results," Kovac said in a press conference reported by the New York Times. "New information from Planck makes it look like pre-Planckian predictions of dust were too low," he added.

The results from Planck were put online in a pre-published form in September. By January 2015, researchers from both teams working together "confirmed that the Bicep signal was mostly, if not all, stardust," the New York Times said in another article.

Separately, gravitational waves have been confirmed when talking about the movements and collisions of black holes that are a few tens of masses larger than our sun. These waves have been detected multiple times by the Laser Interferometer Gravitational-Wave Observatory (LIGO) since 2016. As LIGO becomes more sensitive, it is anticipated that discovering black hole-related gravitational waves will be a fairly frequent event.

Faster inflation, multiverses, and charting the start

The universe is not only expanding but getting faster as it inflates. This means that with time, nobody will be able to spot other galaxies from Earth or any other vantage point within our galaxy.

"We will see distant galaxies moving away from us, but their speed is increasing with time," Harvard University astronomer Avi Loeb said in a March 2014 Space.com article.

"So, if you wait long enough, eventually, a distant galaxy will reach the speed of light. What that means is that even light won't be able to bridge the gap that's being opened between that galaxy and us. There's no way for extraterrestrials on that galaxy to communicate with us, to send any signals that will reach us, once their galaxy is moving faster than light relative to us."

Some physicists also suggest that the universe we experience is just one of many. In the "multiverse" model, different universes would coexist with each other like bubbles lying side by side. The theory suggests that in that first big push of inflation, different parts of space-time grew at different rates. This could have carved off different sections — different universes — with potentially different laws of physics.

"It's hard to build models of inflation that don't lead to a multiverse," Alan Guth, a theoretical physicist at the Massachusetts Institute of Technology, said during a news conference in March 2014 concerning the gravitational waves discovery. (Guth is not affiliated with that study.)

"It's not impossible, so I think there's still certainly research that needs to be done. But most models of inflation do lead to a multiverse, and evidence for inflation will be pushing us in the direction of taking [the idea of a] multiverse seriously."

While we can understand how the universe we see came to be, it's possible that the Big Bang was not the first inflationary period the universe experienced. Some scientists believe we live in a cosmos that goes through regular cycles of inflation and deflation, and that we just happen to be living in one of these phases.

https://www.space.com/25126-big-bang-theory.html

The big bang theory is a cosmological model stating that the universe started its expansion of about 13.8 billion years ago. Pieces of evidence supporting this theory are

● (1) the occurrence of redshift,

● (2) background radiation, and

● (3) the abundance of light elements.

Redshift

In the 1910s, Vesto Slipher and Carl Wilhelm Wirtz measured the wavelengths of light from spiral nebulae, which are interstellar clouds of dust and ionized gases. They discovered that the light from the nebulae increased in wavelength. They explained their discovery as a

Doppler shift

The Doppler shift or Doppler effect explains that when an object gets closer to us, its light waves are compressed into shorter wavelengths (blueshifted, because blue light has the shortest wavelength in the visible region).

On the other hand, when an object moves away from us, its light waves are stretched into longer wavelengths (redshifted, because red light has the longest wavelength in the visible region).

Slipher and Wirtz then explained that the redshift or increase in wavelength was due to the increase in the distance between the Earth and the nebulae. They concluded that the redshift occurred due to the expansion of space.

In 1929, Edwin Hubble used the redshift of light from galaxies to calculate the velocities and distances of these galaxies from the Earth. He discovered that they were moving away from the Earth and from each other. His calculations supported the theory that the universe is expanding.

Cosmic Microwave Background Radiation

In 1965, Robert Wilson and Arno Penzias discovered a low, steady “hum” from their Holmdel Horn antenna (an antenna built to support NASA’s Project Echo).

They concluded that the noise is Cosmic Microwave Background Radiation (CMBR), the remains of energy created after the big bang expansion. The abundance of Light Elements The observed abundance of light elements supports the big bang theory.

The theory predicts that the universe is composed of 73% hydrogen and 25% helium by mass. The prediction correlated to the measured abundances of primordial material in unprocessed gas in some parts of the universe with no stars.

Formation of Light Elements

Big bang nucleosynthesis is the process of producing the light elements during the big bang expansion. In the beginning, the universe was very hot that matter was fully ionized and dissociated. Few seconds after the start of the big bang, the universe was filled with protons, neutrons, electrons, neutrinos, and positrons.

After the first three minutes, the universe cooled down to a point where atomic nuclei can form. Protons and neutrons combined to form atomic nuclei such as deuterium.

However, the temperature of the universe was still much greater than the binding energy of deuterium. Binding energy is the energy required to break down a nucleus into its components. Therefore, deuterium easily decayed upon formation.

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