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Posted on 05/13/2025 1:16:19 PM PDT by MtnClimber
Explanation: What does our Milky Way Galaxy look like from the top? Because we are on the inside, humanity can’t get an actual picture. Recently, however, just such a map has been made using location data for over a billion stars from ESA’s Gaia mission. The resulting featured illustration shows that just like many other spiral galaxies, our Milky Way has distinct spiral arms. Our Sun and most of the bright stars we see at night are in just one arm: Orion. Gaia data bolsters previous indications that our Milky Way has more than two spiral arms. Our Galaxy's center sports a prominent bar. The colors of our Galaxy's thin disk derive mostly from dark dust, bright blue stars, and red emission nebula. Although data analysis is ongoing, Gaia was deactivated in March after a succession mission.
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Or by mail to: Free Republic, LLC - PO Box 9771 - Fresno, CA 93794
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For more detail go to the link and click on the image for a high definition image. You can then move the magnifying glass cursor then click to zoom in and click again to zoom out. When zoomed in you can scan by moving the side bars on the bottom and right side of the image.
🪐 🌟 🌌 🍔
Our solar system is on the bottom of the second image just below the “O” in Orion.
We’re in the Galactic Boondocks................
What is “The Bar”?
I can see my house! :)
Wow.
Cool.
Galactic UFO.
Scientists use four terms to differentiate the different types of galaxies: spiral galaxies, barred spiral galaxies, elliptical galaxies, and irregular galaxies. This article assesses the similarities and differences of the barred spiral galaxy vs. an unbarred spiral galaxy. The main difference between a barred spiral and unbarred spiral galaxy is the large bar that runs through the center of the former. While the structure of both galaxies is largely similar, this elongated bar suggests that the galaxy is a more mature version of the spiral galaxy. Continue reading to learn about the similarities and differences between barred and unbarred spiral galaxies.
This is the barred NGC 1300 Galaxy
Spiral galaxies are flat, rotating disc composed of gas, dust, and stars. A barred spiral galaxy is that which has a bar-shaped structure made from stars at its center. Edwin Hubble first discovered these galaxies in the early part of the twentieth century, and scientists use the classification SB to differentiate them. And we can break this classification down even further. An SBa galaxy contains very tightly bound arms, whereas an SBc galaxy has significantly more loosely bound arms. As many as 65% of spiral galaxies contain bars; these affect the movement of the gas, dust, and stars that surround them. Scientists believe the bar acts similarly to a funnel, pulling matter into the disc’s bulge. This leads to starbursts in the center of the galaxy. The central bar in a galaxy provides information about the age of that galaxy, with scientists estimating that a bar takes around two billion years to form. Our galaxy is a barred spiral; while the largest Barred Spiral that we can see is the Condor Galaxy, found in the Pavo constellation. The so called “bar” isn’t a solid object. Instead, its formation is due to a range of unstable stars at the center of a galaxy that give the appearance of a solid object thanks to their high density.
What Is An Unbarred Spiral Galaxy?
This is the unbarred Whirlpool Galaxy
An unbarred spiral galaxy is a variety of spiral galaxy that lacks a central bar; scientists use the classification SA to differentiate them from other galaxy types. The arms of a spiral galaxy contain numerous amounts of gas and dust, plus a range of young stars that shine brightly but briefly. The formation of spiral arms remains to be something of a puzzle for scientists. One theory is that high-density waves traveling through the outer disc could be responsible for these formations, but no one knows. Scientists also believe that spiral galaxies eventually evolve into elliptical galaxies as they age. But the latter is difficult to measure thanks to their abundance of older, dimmer stars that give them less visibility in the night sky. The bigger a galaxy is, the faster it will spin, with the arms of a large galaxy spinning at up to two million kilometers per hour. A different version of the unbarred spiral galaxy is the unbarred lenticular galaxy. A lenticular galaxy is one whose structure sits somewhere between a spiral and elliptical gallery. It contains a large disc, but its arms are not the same magnitude as a spiral galaxy. Scientists denote this type of galaxy as SA0.
The Similarities Between Unbarred And Barred Galaxies.
The physical structure of barred and unbarred galaxies is similar in many ways. Most spiral galaxies possess a bulge at their center, with a rotating disc of stars surrounding it. Both galaxies have a defined shape, which bulges in the middle. Another characteristic shared by both types of galaxies is that the older stars reside closer to the nucleus, while the younger stars spread out across the arms. Stars contained in the bulge of a spiral galaxy tend to be redder (as well as older) than the rest. This bulge is created by an incredibly dense nucleus that draws matter into its center. Scientists classify unbarred and barred galaxies by how tightly the spiral arms are wound. SAa or SBa galaxies are those that possess tight arms, whereas a SAc or SBc galaxy is one with a loose formation.
Differences Between Barred and Unbarred Spiral Galaxies.
While a barred spiral galaxy holds many of the same characteristics as an unbarred spiral galaxy, there is one obvious difference. The barred galaxy has a huge bar running through its center that affects everything from the movement of the stars to the arms of the galaxy’s spiral. 2008 studies demonstrated that barred spiral galaxies are the older of the two types as a central bar indicates that a galaxy has reached its full maturity. A barred galaxy forms when the orbits within a spiral galaxy become unstable and deviate from their circular path. These divergences in the star’s orbit gradually elongate its path, which eventually locks into a bar. A bar is thought to be the last significant process of a spiral galaxy which forces a large amount of gas towards its center while fuelling the formation of new stars and feeding supermassive black holes.
Summary
Barred and unbarred spiral galaxies share the same basic shape and many of the same characteristics. They have a large central disc, around which massive arms of gas and dust swirl. The difference between the two is the presence of a large bar. This bar is formed due to the unstable nature of the orbits within that galaxy and signifies that the galaxy in question is older than an unbarred spiral galaxy.
But...I get the point.
Thanks for the info.
Does having my house in a Barred Galaxy increase its value?
[We seem to be deep in the ‘burbs.]
I think the unbarred spirals have the highest home values. They are newer.
Well, there goes the neighborhood.
“The side view from yesterday:”
This image raises a curiosity. What is pulling on it to make it Asymmetric like that rather than flat and Symmetric? Whatever it is, it is affecting all the bodies on the right opposite from all the bodies on the left. Extremely interesting...
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