I’ve always wondered how astronomers can actually observe galaxies that are millions or even billions of light-years away. What exactly are we seeing when we look at them?

And when scientists say there are hundreds of billions, or possibly trillions, of galaxies in the observable universe, how do they know that if we obviously haven’t seen and counted every single one?

  • AFK BRB Chocolate (CA version)@lemmy.ca
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    21 hours ago

    It turns out that when light travels through the mostly emptiness of space, it can travel amazingly far without being significantly diminished. So we see galaxies the same way we see stars - you can see some with the naked eye, in fact, but to see detail you need a telescope. They come in somewhat different configurations, but generally look like this:

    image

    We don’t know exactly how many there are, we have to estimate it, and the range of estimates is huge: between 100 billion and 200 billion!

    How do we estimate it? By counting the galaxies in a teeny tiny area of the sky, and then multiplying by that fraction. There are an amazing number of galaxies that are viewable in an area of the sky the size of the head of a pin held at arm’s length. It looks like this;

    image

    By the way, the galaxy at the top of this comment is eighty million light years away. That means the light were seeing from it now left eighty million years ago; we’re seeing back in time.

  • LastYearsIrritant@sopuli.xyz
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    16 hours ago

    Just so you know, you don’t need special equipment to see another galaxy. If you have good eyes, you can just go to a very dark place and look up. A pair of binoculars definitely helps though.

    https://en.wikipedia.org/wiki/Andromeda_Galaxy

    There’s actually a bunch of local galaxies that you can see with just a pair of binoculars, a small telescope, or a good camera and some time.

    The Messier Objects are one catalog of things that are pretty bright in the sky that you can see with your eyeballs through any basic telescope or binoculars. The numbers don’t really mean anything, they’re just the order they were cataloged in.
    https://en.wikipedia.org/wiki/Messier_object

    If you check out the list, you can see that a lot of them are galaxies. If you spend a little time learning how to find them, you can see them yourself. – Andromeda is M32.

    Those are all part of the Local Group. Which are a bunch of galaxies that are all nearby and pretty easy to find with telescopes.
    https://en.wikipedia.org/wiki/Local_Group

  • lime!@feddit.nu
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    21 hours ago

    have you seen the Hubble Deep Field image?

    it’s a picture of a section of the sky “about the size of a tennis ball at a hundred meters” taken by pointing the telescope at a point that appeared completely dark over a period of 10 days. there are over 3000 galaxies in that image.

    • queerlilhayseed@piefed.blahaj.zone
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      20 hours ago

      I remember the first time I saw that image. The dazzling scope of it. The feeling that Carl Sagan described about the Pale Blue Dot photograph is the closest thing I’ve seen to describing the incredible sense of smallness the Deep Field image gives me. I still get a shadow of it, especially with the JWST images, but that was the first time I really felt how huge the universe is. It’s… words fail me. It’s so big, and there’s so much stuff in it. It boggles the mind.

      I can’t fucking wait for the Roman data to start rolling in. We’re going to find so many cool things we’ve never seen before.

      • Mantzy81@aussie.zone
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        17 hours ago

        As a geologist we talk in millions and billions of years regularly and it’s part of our thing to realise how small and insignificant our lives and humanity is in general.

        But as an amateur astronomer, the vastness and time of space is just another level.

        • Alex@lemmy.ml
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          16 hours ago

          The age of the Earth is a significant fraction of the age of the universe so we are not totally divorced from the timescale.

          • queerlilhayseed@piefed.blahaj.zone
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            14 hours ago

            Age of Universe: ~13.8B years
            Age of Earth: ~4.5B years
            Life on Earth: ~3.7B years

            Assuming those estimates are correct, there has been life on earth for about a quarter of the time since the Big Bang. The solution to the Fermi Paradox could well be that we’re simply among the first species able to look out into the stars. Maybe the Universe is just getting started.

            • Alex@lemmy.ml
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              13 hours ago

              Or we could be about to add a data point to the great filter theory, take your pick 😉

              • queerlilhayseed@piefed.blahaj.zone
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                8 hours ago

                If by we you mean humans, IDK it’s looking pretty dicey at the moment. We as in Earth? I think will be just fine a million or so years after we’re gone, and in that time other intelligences may rise. Maybe octopi start forming complex social groups, or chimpanzees fill the niche we leave, or the fungal network finally reaches critical mass and becomes a planet-spanning superconsciousness and catapults itself into the space age by interpreting ancient human artifacts. I think Earth is gonna be a galactic contender. Whether humans are around when that happens is another question.

  • hokuspokus@piefed.socialOP
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    16 hours ago

    Thanks everyone for all the answers and explanations! I really appreciate you taking the time to break this down.

    It’s honestly mind-boggling to think about the distances involved, how long that light has been travelling before it reaches us, and just how unbelievably many galaxies are out there. The scale of the universe is very hard to wrap your head around.

  • neidu4@piefed.social
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    14 hours ago

    With a good telescope, what may have previously appeared as stars, turns out to be a collection of millions of stars in a tiny secti9n of the sky.

  • crapwittyname@feddit.uk
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    21 hours ago

    We make the following assumptions:

    1. We are not in a privileged or special place in the universe.
      1a. Therefore the universe should look the same from where we are as from almost anywhere else.
    2. Supernovae emit a very reliable amount of light.
      2a. Therefore we can accurately tell how far away a supernova is by its light signature.
    3. We can tell how far away distant galaxies are when a supernova goes off in them.

    Therefore, we can map out and count the galaxies in our local area, and, using assumption 1, we know that the number of galaxies in our volume of space is the same as in every volume of space. Multiply the one by the other and you’ve got your answer.

    • LastYearsIrritant@sopuli.xyz
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      16 hours ago

      This is a great comment, but just for completeness, the Type Ia Supernovae is only one part of the Cosmic Distance Ladder.

      https://en.wikipedia.org/wiki/Cosmic_distance_ladder

      We can start with small, easier to measure things, and work our way outwards to more and more complicated measurement techniques. Most of these techniques overlap each other and can be used to confirm our measurements.

      One of the big unsolved questions in cosmology is that many of our measurements disagree, this isn’t a “problem” just an unsolved question, and as a result, we don’t know how far away things are to the accuracy we would like. That being said, we still know how far away they are to a pretty damn close approximation.

      The interesting thing is, the better we get at measuring how far away things are, the more our measurements differ from each other. There’s a lot of reasons why this might be, but one of them is that a Type Ia Supernovae might not be as standard as we think it is.

      https://en.wikipedia.org/wiki/Hubble's_law#Hubble_tension

      • crapwittyname@feddit.uk
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        15 hours ago

        I chose a simple standard candle for a quick explanation, but yes, these are all independently verified by other methods, which in turn verify each other etc. Parallax is a good one: at one side of the earth’s orbit and the other, you measure the relative position of the thing you want to know the distance to, which is just like closing one eye then the other. Distant objects move less in your vision/against the background stars than close objects do.

  • SuiXi3D@fedia.io
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    17 hours ago

    We see the galaxies as they were however many years it took for the light to reach us.

    Every time we look, we find something new because there’s both a LOT of stuff in space and because light from further away keeps eventually reaching us.

    …but mostly it’s a very complicated guess with a lot of math based on what we’ve already seen. Truth is, we don’t know precisely how many galaxies there are, but there’s always a whole shit ton of them everywhere we look, so it’s reasonable to assume the number is pretty big. And getting bigger because, again, we keep seeing new stuff.

  • remon@ani.social
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    21 hours ago

    By pointing a telescope at them and looking. You can see some of the larger ones through a cheap home telescope for a couple hundred dollars.