A Curious Problem with Red Galaxies - Sixty Symbols

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Sixty Symbols

Sixty Symbols

Күн бұрын

Professor Mike Merrifield on a new paper about Red Galaxies - and why that may cause a rethink about galaxy formation. More links and info below ↓ ↓ ↓
The paper in Nature: www.nature.com/articles/s4158...
And on arXiv: arxiv.org/abs/2207.12446
Professor Merrifield is an astronomer at The University of Nottingham: bit.ly/NottsPhysics
Mike Merrifield Playlist: bit.ly/Merrifield_Playlist
Mike on Twitter: / astromikemerri
Visit our website at www.sixtysymbols.com/
We're on Facebook at / sixtysymbols
And Twitter at / sixtysymbols
This project features scientists from The University of Nottingham
bit.ly/NottsPhysics
Patreon: / sixtysymbols
Sixty Symbols videos by Brady Haran
www.bradyharanblog.com
Editing by James Hennessy
Email list: eepurl.com/YdjL9

Пікірлер: 210
@ElijahMathews
@ElijahMathews 11 ай бұрын
It feels so weird to have grown up watching Sixty Symbols as a kid and then as a grad student wind up being part of a work that gets covered here 😅
@brianjones9780
@brianjones9780 11 ай бұрын
I think that's great!
@DrKaii
@DrKaii 11 ай бұрын
ᕙ⁠(⁠ ͡⁠°⁠ ͜⁠ʖ⁠ ͡⁠°⁠)⁠ᕗ
@knightwik
@knightwik 11 ай бұрын
wow congrats!
@evionlast
@evionlast 11 ай бұрын
Is this show that old?
@RedSunT
@RedSunT 11 ай бұрын
@@evionlast The first videos on this channel came out 14 years ago, so definitely possible for a grad student to have watched as a kid..
@jeroenvandorp
@jeroenvandorp 11 ай бұрын
It _is_ possible to explain difficult science in a correct, non-spectacular, non-oversimplified, not-pr-like yet interesting way to everyone interested in the subject. My compliments for every video so far.
@ro_yo_mi
@ro_yo_mi 11 ай бұрын
Agreed... Everyone in Brady's Bunch all do a fantastic job of explaining their field so well.
@Q_QQ_Q
@Q_QQ_Q 11 ай бұрын
press releases are PR . you need to read offical papers to know the thing .
@DrKaii
@DrKaii 11 ай бұрын
​@@Q_QQ_Q press release is also PR 🤯
@ArawnOfAnnwn
@ArawnOfAnnwn 11 ай бұрын
@@Q_QQ_Q Official papers are not written for the general public, and are typically quite hard to understand.
@nickvanamstel
@nickvanamstel 11 ай бұрын
All of the contributors are great, but I really like Professor Merrifields ability to break down these truly complex facts.
@AdamBlacksburg
@AdamBlacksburg 11 ай бұрын
Best KZfaq channel there is.
@helvio89
@helvio89 11 ай бұрын
Unfortunately I'm about to finish watching all its videos. Wish there were even more.
@Panda_436
@Panda_436 11 ай бұрын
For sure... the lack of views/support is the worst...
@StephanTrube
@StephanTrube 11 ай бұрын
While the explanation was enlightening, I loved the last part the most, starting at 11:04. Something could be wrong. And then see the excitement and humbleness of the scientist delving in how his/our understanding might be wrong, closing in his preference to study nearby galaxies because they look nice. This gave the video a wholesome human touch.
@RFC-3514
@RFC-3514 11 ай бұрын
2:53 - Whoever does those animations really needs to be told that *redshift (of something that starts out blue) doesn't go **_through_** purple.* It's (at least) the second time they make something go blue -> magenta-> red, which is the _opposite_ of the way redshift works. It would go blue -> green -> yellow -> red (progressively *increasing* wavelengths / decreasing frequencies). In fact, magenta isn't a wavelength at all, it's just the way our brain interprets a mix of frequencies at the low and high end of our visible visible spectrum (i.e., red and blue/violet), in the absence of mid-range frequencies (i.e., yellow / green). If you're doing a colour shift to illustrate some physical property and going _through_ magenta, you're doing something wrong.
@raideurng2508
@raideurng2508 11 ай бұрын
I knew I wasn't the only one to notice that!
@harbingerdawn
@harbingerdawn 11 ай бұрын
Yeah, they need to interpolate the transition in counterclockwise HSV space rather than RGB space.
@DrMackSplackem
@DrMackSplackem 11 ай бұрын
Yeah, what the heck? That's basic ROYGBIV-level stuff.
@RFC-3514
@RFC-3514 11 ай бұрын
@@DrMackSplackem - I suspect whever did the animation just through "redshift" meant "add some red".
@DrMackSplackem
@DrMackSplackem 11 ай бұрын
@@RFC-3514 LOL. I agree, that's most likely what they/them did.
@smitemus
@smitemus 11 ай бұрын
It's actually cool when science and discovery throws you for a loop and is not exactly what you expected
@DaxLLM
@DaxLLM 11 ай бұрын
I think that's what makes science so exciting! 🎉
@Smitsva
@Smitsva 11 ай бұрын
only 12 minutes ?? i can watch Mike for hours !
@alancash6420
@alancash6420 11 ай бұрын
As well as the Lyman and Balmer, if you spot the Amen Break in your spectra then you can confidently date the galaxy's formation to no earlier than 1969.
@renerpho
@renerpho 11 ай бұрын
I hope this comment gets the appreciation it deserves.
@skyelord6229
@skyelord6229 11 ай бұрын
@@renerpho Oh, brother...
@iveharzing
@iveharzing 11 ай бұрын
And then you've also got the Ballmer peak.
@talamioros
@talamioros 11 ай бұрын
I love that I understood the reference
@Buizie
@Buizie 11 ай бұрын
Thanks I can never get amenbreaks out of my head-
@Ojisan642
@Ojisan642 11 ай бұрын
Mike Merrifield is the platonic ideal form of a science educator.
@DrKaii
@DrKaii 11 ай бұрын
They say his brain is a perfect sphere
@sudazima
@sudazima 11 ай бұрын
@@DrKaii smooth brain best brain
@DrKaii
@DrKaii 9 ай бұрын
Of unit radius.
@AbelShields
@AbelShields 11 ай бұрын
Wow, this video is an amazing explanation. I saw another video about lyman-alpha breaks (going over similar observations from JWST) and I sort of got it, but this gives a really great explanation of how it occurs and what the double break means. Thanks!
@backwashjoe7864
@backwashjoe7864 11 ай бұрын
Agreed! This is by far the best explanation I've ever seen. He explained the lyman-alpha break in a great set of steps. 1. all energies above a certain level will ionize the atom, absorbing all of the radiation. 2. the spectrum will have a drop, a cliff, as you move to the left, at the point where all of the radiation starts being absorbed. 3. because the spectrum's y-axis is the intensity of the radiation. 4. (exercise for the viewer) and because the spectrum's x-axis is wavelength, which is inversely proportional to energy. The shorter wavelengths as you go left are higher energies. I could do that step 4 on my own because I finally understood 1, 2, and 3. Awesome!
@123Shel12
@123Shel12 11 ай бұрын
Very likely the best explanation about these distant mysterious galaxies I’ve heard so far on any of the astronomy/physics KZfaq channels I subscribe to! Well done!!!!
@kwgm8578
@kwgm8578 11 ай бұрын
It's good to see a fresh Sixty Symbols on the channel. Thank you! 👍🏼
@Rattiar
@Rattiar 11 ай бұрын
Really appreciate Dr. Merrifield's clear explanations of this stuff. Can't wait for more JWST data and more explanations. We'll be wrong about more stuff, and I am here for it! :)
@StefanoMersi
@StefanoMersi 11 ай бұрын
This is probably the best science talk I remember. Clear, concise, engaging, ACCURATE. Bravo, professore!
@fishnsyd
@fishnsyd 11 ай бұрын
This is the best explanation of the wavelength breaks I’ve ever heard. I feel like I finally understand 😅
@98swarup
@98swarup Ай бұрын
Professor Merrifield constructs such a beautiful narrative in terms of explaining the paper. He doesn't even reach the crux of the paper till more than midway in the video, providing a solid understanding and context, building it up till he explains the paper itself. Masterfully done
@lumotroph
@lumotroph 11 ай бұрын
Oh my gosh I’ve never seen ionisation described with an energy level diagram like that - that’s amazing!
@guyh3403
@guyh3403 11 ай бұрын
And THIS is how you explain things! Sure it raised a lot of questions in the end, but that's just a good thing. Thank you so much!
@Ethelgiggle
@Ethelgiggle 11 ай бұрын
I gotta say as someone who considers switching to science journalism Brady is one of the biggest inspirations I have had for a long time. It's always excellent especially in a field where there a so many people doing it badly. If you read this thank you!
@AndreaCalaon73
@AndreaCalaon73 11 ай бұрын
What a Beautiful explanation!
@resonatingsilence
@resonatingsilence 11 ай бұрын
Thank you for this.
@davidcampos1463
@davidcampos1463 11 ай бұрын
Thank you. I needed all of this reasoning part of the argument.
@june-ls1hw
@june-ls1hw 11 ай бұрын
Amazing video. I hope to see an update about this paper in the future :)
@HEMANTRAJYADAV
@HEMANTRAJYADAV 11 ай бұрын
If I had to keep watching one youtube channel for rest of my life, it would be this channel. Absolutely loved this video!
@alimanski7941
@alimanski7941 11 ай бұрын
It's incredible how much can be resolved from so little signal - a few pictures in different wavelengths and a few very clever people with the right tools can break the current understanding of galaxy formation. Remarkable.
@robertfraser9551
@robertfraser9551 11 ай бұрын
Brilliant. Clear crisp and entertaining !!
@ricardoabh3242
@ricardoabh3242 11 ай бұрын
Crazy nice explanation Thanks
@GuentherShadow
@GuentherShadow 7 ай бұрын
Mike Merrifield is just awesome at explaining the most intricate theories. Thank you so much.
@alandyer910
@alandyer910 11 ай бұрын
Superbly explained! Thank you!
@w0ttheh3ll
@w0ttheh3ll 11 ай бұрын
Great video, thanks!
@LA-MJ
@LA-MJ 11 ай бұрын
Thank you for explaining the double break. Seems intuitive in hindsight.
@jbtownsend9535
@jbtownsend9535 11 ай бұрын
Magnificent video! Thanks for keeping it current and not dumbing things down too much. Would love to know more about the limit of how far back we can measure objects VS time of Big Bang.
@drsatan9617
@drsatan9617 11 ай бұрын
The limit will be 41 billion lightyears. The observable universe. These galaxies are about 30 billion light years away
@thegodofhellfire
@thegodofhellfire 11 ай бұрын
Fantastic video!
@pedrolopa2
@pedrolopa2 11 ай бұрын
Fascinating!
@-Kerstin
@-Kerstin 11 ай бұрын
Things like this are often dumbed down or badly explained but this video (and channel) is excellent.
@seionne85
@seionne85 11 ай бұрын
Best explanation of why ionized gas is opaque I've ever heard and the video just got started!
@Ryan_gogaku
@Ryan_gogaku 11 ай бұрын
What I like most is how Prof. Merrifield gets *most* excited when Brady asks him what could potentially be *wrong* with his own work at about 11:03. That is a sort of concentrated form of the spirit of inquiry as seen through facial expression and gesture.
@DwainDwight
@DwainDwight 11 ай бұрын
best channel on yt. thanks fellas
@GeoffryGifari
@GeoffryGifari 11 ай бұрын
Is it right to say that the closer the light spectrum to the (lyman, balmer, ...) breaks, the easier it its to identify the object and how far it is?
@ScientiaHistoria
@ScientiaHistoria 11 ай бұрын
Excellent.
@applechocolate4U
@applechocolate4U 11 ай бұрын
I love sixty symbols so much
@JeffreyKane
@JeffreyKane 11 ай бұрын
just fantastic.
@Pawle123
@Pawle123 8 ай бұрын
Not connected to this video, but please do a video on Ho'oleilana.
@dav1dsm1th
@dav1dsm1th 11 ай бұрын
Great explanation of "the problem" that even a knuckle dragger like me could somewhat understand.
@unvergebeneid
@unvergebeneid 11 ай бұрын
Didn't those early stars tend to be more massive? Could that mean that the 200 million years for the big stars to explode number could be wrong for the earliest galaxies? Or do we always get a certain number of stars that need 200 million years to explode?
@Veptis
@Veptis Ай бұрын
I always wondered how you attribute a red shifted transmission line to a specific element. But I guess sufficient resolution as well as multiple peaks is the way to go.
@beck4218
@beck4218 11 ай бұрын
Yes!
@Panda_436
@Panda_436 11 ай бұрын
I have a question... maybe I don't know enough about science in general, but what are the units of time considered when studying this, I always get confused about the mindset applied when understanding these subjects, is it the time applied only for light speed? Or is it about factoring OUR time unit into analyzing this? (I'm sorry if I sound dumb... u.u)
@GeoffryGifari
@GeoffryGifari 11 ай бұрын
From what i understand, the longer the wavelength the harder it is to resolve fine details. Does it mean we get less "features"/information when looking at extremely far objects?
@kerstin3267
@kerstin3267 11 ай бұрын
It's correct that the same aperture of a telescope will provide less resolution at longer wavelengths.
@trickyd499
@trickyd499 11 ай бұрын
Mike Merrifield is my favorite Professor
@scottpelak1856
@scottpelak1856 11 ай бұрын
I wish I could give this 100 likes. Very well done!
@Jesusisyhwh
@Jesusisyhwh 11 ай бұрын
If the electron is ionized and has been torn away from the atom, what is then absorbing the energy? As I understand it, the protons can't do that, only the electrons. But, do they still have higher energy states if they are no longer a part of an atom?
@abhijitborah
@abhijitborah 11 ай бұрын
". . . they are not really very exciting, are they?" "ngaaa" 😂 @12:00
@Valdagast
@Valdagast 11 ай бұрын
I mean, it would be pretty boring if JWST just confirmed our existing theories.
@Theraot
@Theraot 11 ай бұрын
I'm having a hard time with this: You say you have dips in the spectrum because some wavelength are absorbed by the specific energy levels... But you also say that anything below the maximum energy level tends to be absorbed which results in a big dip in the lower end the spectrum... But is that before the dips mentioned earlier if those dips are from energy levels that are part of the range that causes the big dip?
@JCO2002
@JCO2002 11 ай бұрын
The graph used had wavelength as the x-axis. So it went from high energy levels on the left to lower on the right, which made the dip appear at higher energy.
@TitanOfClash
@TitanOfClash 11 ай бұрын
The graph you're looking at is actually in the positive direction for wavelength, but the negative direction for energy. Look at the equation for a photon's energy, E = hf, and then look at the equation for the photon's speed, c = fλ. If you do enough jigging about, you get λ = ch/E. Or in other words, as the energy goes up, the wavelength goes down, and vice versa. So you're right, all the energy is absorbed the higher you go, which is further to the left on the diagram.
@gameeverything816
@gameeverything816 11 ай бұрын
Neat
@z-beeblebrox
@z-beeblebrox 11 ай бұрын
This is really interesting, but as a layperson, I gotta say my immediate concern would be...we have Red Shift, AND we have the contention that these galaxies are red as a separate feature? That's SO much red! How do we know which red is which???
@executivesteps
@executivesteps 11 ай бұрын
Is there really a big problem being “off” by a factor of 2 regarding anything like distance or time in the very early Universe?
@strehlow
@strehlow 11 ай бұрын
My intuition is that early galaxies would coalesce and grow in the early universe significantly faster than they could later. The density of mass to accrete was much higher and had much shorter distance to travel to clump up. It could have been quite reasonable for some to form within the first couple hundred million years. Was this not actually the case? Has it been shown that the galaxies didn't form much faster?
@JoeFoxJr
@JoeFoxJr 11 ай бұрын
Was there some motivation for specifically searching for massive galaxies in this redshift range? Was there reason to speculate that the prevailing theory (that such massive/early galaxies are rare) was wrong, or was this a stab in the dark?
@garethdean6382
@garethdean6382 11 ай бұрын
The basic motivation was to get higher resolution and more varied images of early galaxies to test our current models of early galaxy formation. This specific set of galaxies is a sub-section of that wider effort and have shown that our models may not be correct. Other models (such as the direct collapse of supermassive stars into the earliest black holes) are also being tested and may be confirmed or ruled out entirely.
@danielparsons2859
@danielparsons2859 11 ай бұрын
The JWST finding galaxies so close to when the Big Bang is supposed to have occurred is like taking someone to an island that is supposed to of never had human habitation and when you get there you find a shopping mall.
@Mernom
@Mernom 11 ай бұрын
2:50 that animation showed red shifting through the blue part of the spectrum, instead of the yellow part...
@RFC-3514
@RFC-3514 11 ай бұрын
It's even worse than that, it showed it shifting through _magenta,_ which isn't part of the spectrum at all.
@jules2545
@jules2545 11 ай бұрын
Out of interest, what Z number do these galaxies equate to please?
@sheldoniusRex
@sheldoniusRex 4 ай бұрын
Is it possible that early galaxies had a higher proportion of red dwarf stars than modern galaxies? If they did, would the light from those stars be so red shifted that we have no instruments capable of seeing them at all? How would that affect the mass calculations of early galaxies?
@JohnDlugosz
@JohnDlugosz 11 ай бұрын
So this is saying that stars formed and started going through their lifecycle, *before* the hydrogen recombination that released the CMB?
@garethdean6382
@garethdean6382 11 ай бұрын
No. It's saying that galaxies several hundred million years after the CMB are surprisingly bright and large for what we expect from current models. No visible light signal 'behind' the CMB should exist, since that involved a universe-wide 'fog' that scattered all light.
@dcorgard
@dcorgard 8 күн бұрын
I'd solidly bet that there's more to redshift than the Doppler effect. An "intrinsic" redshift.
@JeroenBouwens
@JeroenBouwens 11 ай бұрын
Professor Copeland would smack you for drawing a hydrogen atom as a nucleus with a little ball orbiting around it.
@joerecoveryjoerecovery5781
@joerecoveryjoerecovery5781 11 ай бұрын
I like to think that when we encounter extraterrestrial intelligent life, and they don't know as much as we know, we will teach them with markers drawn on printer paper.
@timseguine2
@timseguine2 11 ай бұрын
I am wondering if we expect to finally find population III stars with the JWST.
@Li-yt7zh
@Li-yt7zh 9 ай бұрын
But how are they determining the galaxy masses with such certainty of measurements ?
@guff9567
@guff9567 7 ай бұрын
I do not understand. If the edge of the visible universe is the beginning of time, how can that increasingly large sphere of galaxies all fit back into the tinier sphere 1,100³ times smaller ?
@nahuelolgiati5969
@nahuelolgiati5969 11 ай бұрын
Why is so short this video? I demand a second part
@iteerrex8166
@iteerrex8166 11 ай бұрын
Of course the observation is not wrong, the problem lies in the theories. But the explanations are beaten into the astronomers probably since childhood. So its difficult for them to go outside, and seek a new fundamental explanation. This is good that it shakes out the flaws.
@bazpearce9993
@bazpearce9993 11 ай бұрын
I wonder how early universe SMBHs have to do with this unexpected result. Maybe if their masses were higher than previously thought at this stage.
@PhngluiMglwnafh
@PhngluiMglwnafh 11 ай бұрын
Dr. Mike talks about Ballmer Breaks, but there needs to be awareness about the Ballmer Peak 😉
@dougg1075
@dougg1075 9 ай бұрын
They will throw food in boxes and ice coolers for tigers so they can be mentally stimulated trying to get in them. The mysteries of the universe are boxes and coolers for humans
@joen0411
@joen0411 11 ай бұрын
Didn’t stars come before galaxies? Couldn’t these stars have come before they all gathered together to form a galaxy
@d5uncr
@d5uncr 11 ай бұрын
Yes, galaxies are formed by stars. But it isn't stars we're looking at in these plots and images - it's the galaxies. We really can't see single stars that far away.
@timjohnson3913
@timjohnson3913 11 ай бұрын
@@d5uncr agreed and if they were simply random early stars, they would be evenly distributed everywhere you pointed the JWST as opposed to clumped together as you see in the photos of the galaxies in the video.
@Onychoprion27
@Onychoprion27 11 ай бұрын
All the simulations of galaxy formation I’ve seen are of a disperse soup of material; though as I understand it the very early universe was very dense, to where fusion and black holes happened not just inside the hearts of stars. Cuz that’s where and when those supermassive black holes at galactic centers formed, right? Wouldn’t it make sense that, after the formation of these galactic cores, but before the universe got as sparse as it would be by the galactic era, the supermassive black holes kept a lot of the mass around then? Like, their gravity held onto the dense matter against inflation, so the earliest galaxies would have started out with a lot more mass?
@garethdean6382
@garethdean6382 11 ай бұрын
Possibly. Currently there's a spread of models for the early universe, from primordial black holes to massive stars collapsing to entire galactic nuclei forming a single massive starlike object that collapses. Each produces galaxies of different mass spreads at different rates. This current data should help us pick which models and ideas operated in our early universe.
@RWin-fp5jn
@RWin-fp5jn 11 ай бұрын
The observations are not wrong. But our interpretation of the redshift is. We took for granted that the fabric of our own galactic plane, doesnt distort the photon image. But it does! The recent EHT image of sag a* clearly proves a quantum effect is taken place turning the image of the centre of our galaxy 90 degrees rotated. Likewise we will have a distorted image of our outward view of the cosmos, as a QP effect would also entail the inverse arrow of time when looking out. Meaning a cosmoc redshift os actually a blue shift. Which means galaxies are heading towards us, not away. Likewise they are NOT related to a big bang event so they could be much older than we think. Problem solved. Next please.
@shantanubharvirkar7759
@shantanubharvirkar7759 11 ай бұрын
My monthly dose of sixty symbols is HEERE!
@woooooooooow
@woooooooooow 11 ай бұрын
Seeee red was first all the time :D ❤️
@MichaelClark-uw7ex
@MichaelClark-uw7ex 11 ай бұрын
What I always wondered is why isn't there a different red shift on one side of these distant galaxies. If they are rotating then one side would be traveling toward us or a considerable amount slower than the side moving away from us thereby causing a different red shift. And wouldn't the gravity of the source galaxy actually cause a red shift as well, especially after working on that light for a few billion years? Then you have to add in the blue shift caused by our galaxy pulling on the light for billions of years too.
@sixtysymbols
@sixtysymbols 11 ай бұрын
I have a feeling we've discussed this either here or on Deep Sky Videos? kzfaq.info
@jellorelic
@jellorelic 11 ай бұрын
IIRC this is a thing, yes. And on nearby galaxies you can absolutely measure those differences to help get at things like rotational speeds and such. But we don't have the resolution needed to do those kinds of measurements with really distance objects. Look at the pictures they talked about at the end there - these objects are literally 6-8 pixels across at best. Everything in that light becomes a mixed average of the everything coming out of the galaxy as a whole.
@rhamph
@rhamph 11 ай бұрын
@@jellorelic Even then they're only 6 to 8 pixels because they're bright enough to bleed over into adjacent cells of the sensor. In terms of actual resolution they're smaller than a single pixel.
@guytech7310
@guytech7310 11 ай бұрын
If they build a Space Telescope for the microwave\mm bands the same effect will appear. There was no big bang. CMBR also disproves BBT because CMBR maps change every year which is not possible. Most of the CMBR comes from inside the milky way. The better the instruments get, the older the universe gets.
@KaiseruSoze
@KaiseruSoze 11 ай бұрын
And if these distant galaxies are that massive and that far away, there might be others even further away.
@DamianReloaded
@DamianReloaded 11 ай бұрын
Maybe the universe has always existed and it's pouring in from a place similar to the one it's pouring out.
@Coursitout
@Coursitout 11 ай бұрын
Can't two (or more) old small galaxies merge to become what is now seen as a massive old one ?
@flaco777
@flaco777 11 ай бұрын
From my understanding that leads to a burst of new star formation in the newly merged galaxy.
@garethdean6382
@garethdean6382 11 ай бұрын
Generally mergers reinvigorate a galaxy, causing new stars to form. The galaxy itself, especially if it's a binary merger, will tend to keep evidence of that merger as well.
@fernbedek6302
@fernbedek6302 11 ай бұрын
Any chance massive stars were just less likely to form in the early universe?
@renerpho
@renerpho 11 ай бұрын
We'd expect the opposite, due to some of the intricacies of how star formation works. The early universe had fewer heavy elements. When you form stars, you need to collapse a cloud of gas, and to do that, you actually need some way to cool that gas. For that, you need dust, and you can't make dust without heavy elements. In other words, those clouds of gas needed to be a lot more massive in order to collapse into a star, resulting in much more large stars (and much fewer small ones).
@russchadwell
@russchadwell 11 ай бұрын
These galaxies are obviously embarrassed over arriving early.
@HellMuttCoppersnake
@HellMuttCoppersnake 11 ай бұрын
Early crew!
@adamreynolds3863
@adamreynolds3863 11 ай бұрын
Can scientists make the current observations fit the current theory and then see how different the observations would have to be to be accurate? Maybe only 1 measurement is 0.001% off and that might throw the whole thing out of whack
@WilliamDye-willdye
@WilliamDye-willdye 11 ай бұрын
Illustrations are goid, but could we also demonstrate the curve with filters and photos of physical lights on Earth? A neon light or a hydrogen flame in a lab, for example.
@musicalcacti
@musicalcacti 11 ай бұрын
Hello!
@jonathonjubb6626
@jonathonjubb6626 11 ай бұрын
Halton Arp would probably disagree. I'd love to know why he is wrong....
@fabianmerki4222
@fabianmerki4222 11 ай бұрын
balmer break? i am only aware of the ballmer peak! 😂 Google it if you don't know 😂
@snowballeffect7812
@snowballeffect7812 11 ай бұрын
1:00 that wedding ring looks extremely tight and uncomfortable. I hope he's doing ok.
@AstroMikeMerri
@AstroMikeMerri 11 ай бұрын
I had it enlarged, so now it slides off fine. Not, I hasten to add, that I ever take it off!
@snowballeffect7812
@snowballeffect7812 11 ай бұрын
@@AstroMikeMerri Haha! Happy to hear that! Thank you for putting my mind at ease. Cheers!
@NathanaelNewton
@NathanaelNewton 11 ай бұрын
I wonder hypothetically.. If money was no object and all of the resources of human civilization were simultaneously dedicated to building one telescope.. what could we make and what could we see..
@MichaelClark-uw7ex
@MichaelClark-uw7ex 11 ай бұрын
We would see ourselves starve and go extinct because we wasted all our resources on a telescope instead of food and shelter.
@danieljensen2626
@danieljensen2626 11 ай бұрын
We could see a lot for sure. Optical interferometry (combining multiple optical telescopes into one big one) is a growing field, although there are a lot of challenges there to making a really big array. We have radio interferometry pretty well locked down though, I think if there was enough funding for it we could launch a bunch of radio telescopes into space and get like a million times more resolution than even the Event Horizon Telescope they used for those black hole pictures (which combined telescopes from all around the Earth).
@InternetStranger476
@InternetStranger476 11 ай бұрын
If space and time are linked, wouldn't time have been working at a different speed in the early universe?
@garethdean6382
@garethdean6382 11 ай бұрын
Yes, but the problem is since that would be a universe-wide effect, it doesn't matter. If the universe's time suddenly doubled in speed tomorrow, nobody would notice as we'd all be moving at the same temporal speed. The only way to notice would be to have some part of the universe move at a different speed so that the difference built up.
@Samantha-xy4ed
@Samantha-xy4ed 11 ай бұрын
He knows what he's talking about
@TheChEiNt
@TheChEiNt 11 ай бұрын
Why are they considered red if it is the ionizing radiation coming from stars that causes the breaks? I guess the models are throwing more older stars than young ones?
@garethdean6382
@garethdean6382 11 ай бұрын
Because the radiation was ionizing (blue) when it was created, but appears lower energy (red) now. The galaxies LOOK red now, so we call them red.
@russchadwell
@russchadwell 11 ай бұрын
Ah, things were just closer together back then.. closer relative to atom size anyway. Mergers were just easier then.
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