The universe is around 13.6 billion years old and has a barred spiral called the Milky Way.

There are quick facts about the universe.

–  Galaxy type: Barred spiral

– Age: 13.6 billion years (and counting)

– Size: 100,000 light-years across

– Number of stars: about 200 billion

– Rotation time: 250 million years

Our home galaxy has a disk that is 100,000 light-years in diameter and 1000 light-years thick.

The solar system is in the center of the universe. Our solar system takes approximately 250 million years to complete a single revolution, according to Interesting Engineering. Dinosaurs were just emerging and mammals were still evolving when our planet was last in this situation.

The city center is about 25,000 to 30,000 light-years away. The life in the outskirts is good and we are located in one of the smaller neighborhoods. We would find the Scutum-Centaurus and Norma arms if we traveled inwards.

There is a guide for beginners and enthusiasts.

We can see the bright lights of the city on a clear night. Our window into the universe is a group of stars, dust and gas.

The black hole Sagittarius A* is located at the center of the universe. About 4 million times the mass of the sun, this beast consumes anything that strays too close, consuming stellar material to grow into a giant. For the first time, we were able to see the shadow of the black hole thanks to an innovative technique.

Why is our galaxy called the Milky Way?

According to the American Museum of Natural History, our home in the universe is called the Milky Way because it appears to be white in the sky. The goddess Hera sprayed milk across the sky to make this band appear.

Different names are given to the Milky Way around the world. In China and South Africa, it's called the "Silver River" and the "backbone of night", respectively.

Milky Way galaxy type and the great debate of 1920

andromeda galaxy bathed in pink. The large spiral galaxy glows orange and pink and is filled with stars, gas and dust. It sits against a backdrop of stars and the blackness of space.

The Andromeda Galaxy is on a collision course with the Milky Way. (Image credit: Yang Hanwen and Zhou Zezhen )
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Astronomers used to think that all the stars in the sky belonged to our galaxy, but they have since changed their mind.

According to the National Academy of Sciences, the debate about the scale of the universe took place in 1920.

On the other side of the debate, Shapley thought that we weren't at the center of the universe. He said that the stars were a part of the Milky Way. On the other side of the debate, he argued that there were large island universes such as Andromeda that were beyond the limits of the Milky Way.

The dispute was solved by Hubble's observations of variable stars. The closest galaxy to us is 2.5 million light-years away.

Astronomers have been trying to figure out what type of galaxy it is. It is thought that it is a barred spiral, meaning that there is a bar across the center. Calculating the shape of the Milky Way can be done by looking at the stars in the sky.

A future collision of galactic proportions

two spiral galaxies colliding with each other. The galaxy on the left appears to be smaller and more brown/orange in color while the one on the right is larger and looks more blue.

Studying other galactic collisions provides insight into the future Andromeda and Milky Way merger. (Image credit: NASA Hyperwall)
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The Local Group of galaxies, made up of over 30 of them, include the local group of the Milky Way, as well as the others. It's good to know who your neighbors are, as they might be closer than you think. The Milky Way is traveling at a rate of over one million km/h. It's not due for another 4 billion years and there is no need to worry.

NASA and other space entities have been observing distant galaxy collides for decades to get a sense of what we will be facing. There is little to worry about in the short story and the longer tale shows how the universe may change.

Observations of a three-way collision using the Hubble Space Telescope gave some interesting insights. As it got into a tight circle with the other two, the largest of the group was able to grab some material. There was a streak of gas, dust and other materials visible from Earth.

The space between individual stars is large enough that they are not at risk of being ripped up by this process. Don't look for stars colliding, as they won't happen. Due to the amount of gas being pumped into our galaxy, we will have a population that will grow in millions of years.

The low risk of star collision should make our solar system relatively safe. We might be thrown into a completely different path as the merger pushes through.

One practical effect is that the constellations we observe from Earth may change as stars are added into the mix; that said, the collision is happening so far in the future that the constellations we see today may be altered in any case. The night sky will change over time.

The Milky Way: Size, structure and mass

Men silhouetted in front of the night sky with the band of the Milky Way stretching across the sky.

The Milky Way's mesmerizing glowing band has had humankind star-struck for eons. (Image credit: Photo by Kendall Hoopes from Pexels)
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It used to be hard to study the stars. The effort to describe the size and structure of a forest can be compared to being lost in the middle of it. We don't have an overview from our position. Since the 1990s, two ground-breaking space telescopes have been launched. Since the launch of the European Space Agency's Gaia mission, major strides have been made.

Astronomers were able to see the basic structure of some of the closest galaxies with telescopes. It took a long time to reconstruct the shape and structure of our home. The process involved building a catalog of stars and figuring out how far away they are.

Jan Oort, sometimes dubbed the master of the galactic system, was the first to realize that the Milky Way isn't motionless but rotates. Oort was responsible for determining the position of the sun in the universe. A repository of trillions of comets far from the sun was named after him.

Artist's illustration of the Milky Way from above and each of the arms spraying out from the galactic center in a spiral fashion.

The structure of the Milky Way galaxy as seen from above the galactic disk. (Image credit: NASA/Adler/U. Chicago/Wesleyan/JPL-Caltech)
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A spiral galaxy appeared to be ordinary.

There is a black hole at the center of the universe. The black hole has a mass equal to four million suns and can be seen with a radio telescope.

The gateway to nothingness is the most important thing in the universe. There is a tightly packed region of dust, gas and stars in its immediate vicinity. The bulge is peanut-shaped and is 10,000 light-years across. It harbors 10 billion stars, mostly old red giants, which formed in the early stages of the universe's evolution.

The 'Weird signal' comes from the stars. Why is it happening?

The disk is extended beyond the bulge. The feature is 100,000 light-years across and 1,000 light-years thick, and it's home to the majority of the galaxy's stars. There are stars in the disk in the sky. It's the edge-on view of the disk that takes our breath away when we look up at night.

The stars in the disk form streams that look like arms from the bulge. Research into the mechanisms that drive the creation of spiral arms is still in its infancy, but the latest studies suggest that these arms can be formed and dispersed within a short period of time.

The density of the stars, dust and gas inside those arms is more tightly packed than in the less dense areas of the disk, which leads to more intense star formation. Stars in the disk are younger than those in the bulge.

Spiral arms are like traffic jams in that the gas and stars crowd together and move slower in the arms. As material passes through the dense spiral arms, it is compressed and this causes more star formation.

According to the National Science Foundation, there are four spiral arms in the universe. The Sagittarius and Local Arm are not as pronounced as the main arms. The position and shape of these arms are discussed by scientists.

The disk is not flat but warped. It is like a spinning top. The stars in the disk take about 700 million years to complete a full rotation. Astronomers think it's a result of a previous collision.

Artist's illustration of the Milky Way demonstrating how the disk is not flat but warped like a wobbling spinning top.

The structure of the Milky Way with its rotating warped galactic disc. (Image credit: Stefan Payne-Wardenaar; Inset: NASA/JPL-Caltech; Layout: ESA)
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According to a statement from the European Space Agency (opens in new tab), there are a number of objects around the disk and bulge.

The halo of dust and gas is twice the width of the disk. The entire universe is embedded in a larger halo of dark matter. The existence of dark matter can only be inferred from its effects on the motions of stars. According to calculations, this stuff makes up to 90% of the mass.

According to recent NASA estimates, the mass of the Milky Way is equal to 1.5 trillion suns. The visible matter is spread between the stars, planets, and massive clouds of dust and gas. Even though we have only found a few thousand planets, one NASA estimate says there are more than 100 billion planets in the universe. We don't know how many solar systems there are in the sky.

Where is the sun in the Milky Way?

Image of the glowing orange and yellow orb that is the sun.

The sun is one of 200 billion stars making up the Milky Way galaxy. (Image credit: NASA/GSFC/SDO)
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The sun is in the middle of a disk of stars. The sun takes more than 200 million years to complete a full circle around the center of the universe.

The Local Arm of the Milky Way is located at the edge of the sun. Astronomers found that the sun is surfing a wave of gas that's 9000 light-years long, 400 light-years wide and 500 light-years above and below the disk according to the European Space Agency.

There are planets in the solar system that are not in the plane of the galaxy.

Merav Opher is an astronomer at George Mason University in Virginia.

What is the black hole in the Milky Way?

picture of star clusters in blue with an arrow pointing to sagittarius a* black hole

Sagittarius A*, taken by NASA's Chandra X-Ray Observatory. (Image credit: NASA/CXC/Caltech/M.Muno et al.)
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There is a black hole in the sky. It's very difficult to observe the black hole. Astronomers discovered that Sagittarius A* is 4.3 million times larger than the sun. The diameter is approximately 2 million kilometers. The Milky Way is 100,000 light years wide and 1,000 light years thick.

The gas around Sagittarius A* billows out as far away as 30 light-years from the black hole. There is a tenuous area of gas that gives Sagittarius A* activity. The region emits X-rays due to feeding on the gas or being stuck in the disk as temperatures soar to as high as 18 million degrees Fahrenheit.

Scientists want to know more about how the black hole was formed and how it was able to grow. Smaller black holes getting quite large as they eat up dust and gas in the environment nearby is one of the possibilities.

Image of Sagittarius A*, looks like a blurry orange donut against the black backdrop of space.

An image of the supermassive black hole at the center of the Milky Way, a behemoth dubbed Sagittarius A*, revealed by the Event Horizon Telescope on May 12, 2022. (Image credit: Event Horizon Telescope collaboration)
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Scientists have improved models for black holes. Nuclear fusion stops the mass of our sun from collapsing. They shrink to a powerful object that warps time and space around it so much that light can't escape.

The first ever image of the black hole was obtained on May 12, 2022. The shadow on the image is caused by heated matter moving fast towards the center of the black hole. The size of Earth required a large set of observatories around the world, which was possible through the event horizon telescope.

The world was turned into a telescope to see a black hole.

Mapping the Milky Way's history

Clouds of gas and dust began to collapse, pushing together by gravity. The first stars came up from the collapsing clouds. The halo and disk came after. The force of gravity pulled everything together as the galaxy began to grow.

Graphic showing the approximate timeline for the formation of the Milky Way.

The Milky Way is approximately 13.6 billion years old. (Image credit: Future)
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The evolution of the universe is shrouded in mystery. The first catalog of data released by the Gaia mission is slowly unraveling some of the mysteries of the universe.

The exact positions and distances of more than 1 billion stars can be measured with the help of the Gaia telescope. Astronomers can use the position data to determine the speed and direction of the stars. Calculating the path of the stars billions of years into the future is possible because of the predictable trajectory of things in space. The evolution of the universe is captured in a stellar movie.

Evidence points to the fact that the Milky Way collided with several smaller galaxies. A group of 30,000 stars moved in the same direction to the rest of the stars in the data set. Scientists had previously seen the motion pattern in simulations. The stars were different in color and brightness, suggesting they came from a different universe.

Monochrome image showing the Milky Way bulge stretching across the center and several smaller dwarf galaxies are seen in the vicinity. White boxes surround the smaller galaxies so their location can be seen.

Contrary to expectations, dwarf galaxies in the vicinity of the Milky Way have only just arrived. (Image credit: ESA)
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There were remnants of a collision a year after. Smaller galaxies are being devoured by the Milky Way today. Sagittarius, not to be mistaken with the black hole, has been smashing through its disk several times in the past 7 billion years. According to the study, our sun was born some 4.5 billion years ago.

Photographing the Milky Way

Milky way galaxy stretching across the night sky.

Photographing the Milky Way requires a dark sky. (Image credit: Getty)
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It takes a dark sky, a good season, and the ability to use photographic equipment to photograph the stars. It is possible to take pictures of the Milky Way in both the northern and southern hemisphere.

You will want to scout the area for the best angles if you can get to your site during the day. Look for natural features such as mountains, boulders or rock shapes in good Milky Way images.

The photo shoot takes place next. Use a tripod, set your equipment for a timelapse mode, and be prepared to experiment with different focuses. We have a full guide on how to take a picture of the Milky Way.

The future of the Milky Way research

The massive stellar catalog has been updated by the Gaia mission. Astronomers from all over the world are analyzing the data to find new information.

The Hubble Space Telescope is famous for generating research papers. Astronomers will be busy for decades to come if the catalog it has compiled is anything to go by.

Hipparcos was founded by an ancient Greek astronomer who began to chart the night sky before Christ. About 100,000 of the stars in the sun's neighborhood were seen by Hipparcos. It was not as precise as it could have been.

Astronomers can model the behavior of the entire Milky Way even though they only see a small percentage of stars.

Additional resources

This free learning material from the Open University can help you learn more about the stars. You can explore the universe in virtual reality with the help of the European Space Agency. There is a real-time, 3D, astronomy visualization software that uses the data from the European Space Agency's Gaia mission. In this article from the European Space Agency, you can learn why it was so hard to study the Milky Way.

Bibliography

Rix, HW. There is a time-resolved picture of our Milky Way's early formation history. Nature 603, 599, and603 were published in the year 2000.

Robin, Annie C. There is a synthetic view on structure and evolution.

Walter and James Binney are related. There are mass models of the Milky Way.

"Helmi" is the name of the person. There are streams, substructures, and the early history of the Milky Way in the annual review of astronomy and astrophysics.