Submitted by Riceeatingcommunist t3_zgjyij in space
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Submitted by Riceeatingcommunist t3_zgjyij in space
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I think we are looking into the inside of the galaxy as we are on the outskirts? Also I don’t think we really know what MW looks like.
My best guess is by taking the photos around us and constructing a diagram based on distance away.
We don't have photos of the Milky Way as a whole, but all the stars you see around you are part of the Milky Way. Astronomers study the stars and build models to approximate their positions which helps give us a rough idea of what the Milky Way looks like, although there are parts we can't see very well (anything on the other side of the galactic core is mostly obscured by dust around the core itself, for example).
It's like not having a mirror, but being able to feel your face. We're "feeling" the stars with telescopes and can model of what we see based on our observations.
I think by mapping the stars we can see (distance, location, speed), we get a partial shape. We can then compare that known shape with other galaxies we can see, and extrapolate that we must be in the arm of a spiral galaxy. I would bet that our known data points and math are exact enough that we have a rather detailed and accurate idea of what our galaxy looks like.
We assume our galaxy looks like most and we can tell how far are the stars around us, this allows us to have a rough approximation of our galaxy
We can see other galaxies, that's how there are photos of them. As for the Milky Way, we can see towards the centre and some of the arms so we can deduce the shape based on that and what we see from other galaxies
The OP doesnt mean how can he see what the milky way looks like. He wants to know how we (mankind) know what it looks like.
This gif illustrates what you're talking about. Although, in reality, we have a lot more data points.
In short; we don’t. Recent studies suggest that the Milky Way has a wobble on the edges of its outer arms like a warped record, and that it may even be bigger than the Andromeda galaxy. Also, we can map out the stars to get a pretty good idea. Other than that, we really don’t know.
Before we had airplanes and satellites, people went around measuring the distances between objects on the land. Map makers took these measurements and made maps on the Earth's surface.
For the past hundred years, astronomers have been measuring the distances to groups of stars and their directions. Astronomers have used these measurements to make illustrations of the general shape of the Milky Way.
Is it perfect? No, astronomers are still discovering features of the Milky Way, such as the wave in the disc.
All I know is on a clear moonless night 1000 miles into the sea, the Milky Way casts a shadow at your feet it's so bright. Seeing that for the first time as a grown adult, realizing the 99% of humans that came before me knew this as commonplace while it astonishes us. That's sad.
In the (edit: Northern hemisphere), in the summer months, at night, we are facing towards the galactic core of the Milky Way. In the winter, at night, we are facing outwards away from the core.
We’re in it and we can plot the stars that we see all around us. Like a 3D model.
What hemisphere are you in?
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This made me think. How far up perpendicular to galactic plane would we need to go to get a good 'selfie'? Possible with the tech we have in a reasonable timeframe (as in several decades)?
What's the source saying it may be bigger than Andromeda? Just curious since I thought Andromeda was bigger than the Milky Way by at least an order of magnitude.
Mostly through comparing other spiral galaxies to our own, applying our knowledge of stars’ locations, and constructing models from that. Our mapping of our galaxy is still in developing stages, much like maps of the world from the medieval era.
I habve seen some fantastic images of the Milly way and many on youtube videos so I know what it looks like
Not even close. Voyager 1 and 2 have been traveling for decades and have barely left our solar system.
Well apart from mapping the stellar distributions locally to get an idea of depth & feature of nearby arms the key way to get an overall idea if our galaxies shape is via radio observations if the neutral hydrogen emission line.
This emission line from hydrogen at a wavelength if 21cm can be plotted across the sky with variances in the frequency denoting relative velocity. combining this with models of the orbital velocity of matter in our galaxies helps in ascribing the emission to actual hydrogen clouds across the galaxy & thus builds up an overall map of matter distribution.
IIRC, the local supermassive black hole is smaller than you'd typically get in a galaxy of our size. That also might not be a coincidence - bigger & more active black holes may be troublesome for the formation of life.
I thought this immediately as well. Then I realized that whether in the northern or the southern hemisphere, we all look the same direction during our nights.
>Possible with the tech we have in a reasonable timeframe (as in several decades)?
Doubtful. I read recently that with current technology it would take us something like 18,000 years to reach Alpha Centauri, the next nearest star system. The galaxy is much, much thicker than that distance.
So unless there's some massive breakthrough on the level of sci-fi warp drives in our lifetime, I wouldn't expect any galactic selfies.
Imagine being stuck in the edge of a frisbee. What would your view of the world look like? We can guess at the shape of the milky way because we can see that the density of stars around us is concentrated in a disc shape. And as ground based and space based telescopes get better, we get better at measuring the density of stars in different directions and distances, which improves our understanding of the shape of our galaxy.
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To be fair, from what i understand our solar system is on the edge of it and we can look inwards and see it. Even with the naked eye on a clear night
Look up the Sloan digital sky survey. Its work is INCREDIBLE. Also, thanks to such surveys, we know the distances of the stars and whether they're interacting gravitationally, as in following the same orbit around the galactic center, comparing their distance to much closer stars we know are in the galaxy with 100% certainty etc. By measuring the position, trajectories and so on, we can accurately determine its shape. On the Sloan survey website you can load up the 3d map and go fly through the universe, everything you see is exactly how it is out there in the universe
To piggy back, I believe we've also done enough observations on nearby galaxies to get a general idea of what they look like, which would help us shape our own from within
Our maps of not just the milky way, but the observable universe are far beyond any comparison to medieval era maps which in some cases were quite inaccurate. One such map we've made for the observable universe is the Sloan digital sky survey. Its one of the most detailed maps in human history, and we have a 3d model of the universe. Google it and go to its website. You can fly around the universe there in amazing detail. The amount of data it has is insane. It's literally the largest 3d map ever created
It was a relative phrase of speech that I borrowed from my astronomy professor. He showed us the new maps of the Lanikea supercluster and beyond.
I assumed it would just be black. That's insane.
Sweet man. I'm sure your prof would give you extra credit if you went on sloans site and wrote a report haha I took a bunch of astronomy classes when I was in school and loved it. I went for aerospace engineering and ended up doing a minor in physics because I got obsessed with it lol Outside of that, 6 of my required electives were astronomy. 4 with the same prof who was probably the best teacher I ever had. He worked at nasa for like 16 years I think, retired and started teaching. His level of passion showed every single class. He's a rare breed.
You're standing in a sparse crowd of people - you can see many people, and know their positions and speeds with respect to you quite well.
Now, those folk are stars and gas clouds - does that make it seem less mysterious that you can map their position from another vantage point?
Whenever you guys discuss cosmic rays etc, if a report/project etc is asked for, if you want to blow your prof away, make an at home particle detector and take it to class for a demo. It's incredibly easy. Theres a setup called a cloud chamber. You'll be able to visibly see alpha particles etc. My prof loved it and the rest of the class was in awe.
Somneone had an extreme out of body experience and reported back to NASA with the details
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You’re quite right. Thank you. I thought OP was suggesting that at a certain time of year (at night) we would be facing a particular direction relative to the Milky Way. So I wonder which time of year that is? Assuming this to be true for large swathes of time due to our long orbit around the centre of the galaxy…
u/Technical-Grass9441 mentions the summer and the winter and after more thought, I realize that you are on-point to question which hemisphere. I realized that the northern winter is the southern summer and visa-versa.
It is all rather confusing. I’m in Australia so I generally think twice then doubt thrice when it comes to this kind of thing. Thanks for hashing it out w me
[deleted] t1_izh8zbk wrote
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