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  • PBS Space Time

    The NEW Crisis in Cosmology

    10/11/2026 | 22 mins.
    PBS Member Stations rely on viewers like you. To support your local station, go to: http://to.pbs.org/DonateSPACE↓ More info below ↓Uploaded 16-03-21https://www.patreon.com/pbsspacetimeI have good news and bad news. Bad news first: two years ago we reported on the Crisis in Cosmology. Since then, it’s only gotten worse. And actually, the good news is also that the crisis in cosmology has actually gotten worse, which means we may be onto something!The most exciting thing for any scientist is when something they thought they knew turns out to be wrong. So it’s no wonder that many cosmologists are starting to get excited by what has become known as the Hubble tension, or the crisis in cosmology. The “crisis” is the fact that we have two extremely careful, increasingly precise measurements of how fast the universe is expanding which should agree with each other, and yet they don’t. Original Crisis in Cosmologyhttps://youtu.be/72cM_E6bsOsSabine Hossenfelder's episode "Do we travel through time at the speed of light?"https://youtu.be/iBTez-nTKesCheck out the Space Time Merch Storehttps://www.pbsspacetime.com/shopSign up for the mailing list to get episode notifications and hear special announcements!https://mailchi.mp/1a6eb8f2717d/spacetimeHosted by Matt O'DowdWritten by Matt Caplan and Matt O'Dowd Graphics by Leonardo Scholzer, Yago Ballarini, Pedro Osinski, Adriano Leal and Stephanie FariaGFX Visualizations: Katherine KorneiDirected by Andrew KornhaberAssistant Producer: Setare GholipourExecutive Producers: Eric Brown and Andrew KornhaberStandard Candle Definitionhttps://astronomy.swin.edu.au/cosmos/s/Standard+CandleEnd Credits Music by J.R.S. Schattenberg: https://www.youtube.com/channel/UCRl6-nb4iOnsij-vnpAjp0QSpecial Thanks to Our Patreon SupportersBig BangRick DeWittSandy WuMatthew MillerBrodie RaoScott GrayAhmad JodehRadu NegulescuAlexander TamasMorgan HoughJuan BenetFabrice EapMark RosenthalDavid NicklasQuasar SupportersHank SChristina OegrenMark HeisingVinnie FalcoHypernovawilliam bryanScott GorlickNick BerardPaul Stehr-GreenLeo EmersonmuON MarketingRussell PopeBen DeloL. Wayne AusbrooksNicholas NewlinAdrian PosorMark Matthew BoskoАнтон КочковAlec S-LJohn R. SlavikMathewDanton SpiveyDonal BotkinJohn PollockEdmund FokschanerJoseph SalomoneMatthew O'Connorchuck zegarJordan Youngm0nkJohn HofmannTimothy McCullochGamma Ray Burst SupportersAndrew MacleodDiana SDouglas DraneBen CampbellLawrence Tholl, DVMFaraz KhanAlmog CohenAlex EdwardsNickÁdám KettingerSylvain LeducAnthony KahngMD3Endre PechDaniel JenningsCameron SampsonPratik MukherjeeGeoffrey ClarionNateDarren DuncanLily kawaiiRuss CreechJeremy ReedDerek DavisEric WebsterSteven SartoreDrJYouDavid JohnstonJ. KingMichael BartonChristopher BarronJames RamseyDrew HartJustin JermynMr TAndrew MannJeremiah Johnsonfieldsa eleanoryPeter MertzKevin O'ConnellRichard DeightonIsaac SuttellDevon RosenthalOliver FlanaganDawn M FinkBleys GoodsonDarryl J LyleRobert WalterBruce BIsmael MontecelSimon OliphantMirik GogriMark Daniel CohenBrandon LattinNickolas Andrew FreemanShane CalimlimTybie FitzhughRobert IlardiAstaurusEric KieblerCraig StonahaMartin SkansMichael ConroyGraydon GossFrederic SimonTonyfaceJohn RobinsonA GKevin LeeAdrian HatchYurii KonovaliukJohn FunaiCass CostelloGeoffrey ShortBradley JenkinsKyle HoferTim StephaniLuaanAlecZeroCodyMalte UblKing ZeckendorffNick VirtueScott GossettMartin J LollarDan WarrenPatrick SuttonJohn GriffithDaniel LyonsDFaulkGrowingVioletKevin WarneAndreas NautschBrandon labonte Learn more about your ad choices. Visit megaphone.fm/adchoices
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  • PBS Space Time

    Do Black Holes Have to Remain Black?

    10/11/2026 | 21 mins.
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    The primary characteristic that defines black holes is in the name. Black holes are black. The gravitational pull at the event horizon is so powerful that not even light can escape. In this case, black means absence of light. We also think of black as indicating absence of colour. But it turns out there is a way to make a coloured black hole—as long as by colour you mean quantum chromodynamic charge.

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    Hosted by Matt O'Dowd
    Written by Andrea Quaranta & Matt O'Dowd
    Post Production by Leonardo Scholzer, Yago Ballarini & Stephanie Faria
    Directed by Andrew Kornhaber
    Associate Producer: Bahar Gholipour
    Executive Producers: Eric Brown & Andrew Kornhaber
    Executive in Charge for PBS: Maribel Lopez
    Director of Programming for PBS: Gabrielle Ewing
    Assistant Director of Programming for PBS: John Campbell

    Spacetime is a production of Kornhaber Brown for PBS Digital Studios.
    This program is produced by Kornhaber Brown, which is solely responsible for its content.
    © 2024 PBS. All rights reserved.

    End Credits Music by J.R.S. Schattenberg: https://www.youtube.com/user/MultiDroideka

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  • PBS Space Time

    Is There Support For a Vast Multiverse?

    10/11/2026 | 23 mins.
    Learn More About Anydesk: https://anydesk.com/spacetime

    In 1987, Steven Weinberg wrote a cute little paper entitled “Anthropic Bound on the Cosmological Constant”. I say cute little paper because it feels minor in comparison to, say, electroweak unification theory that won him the Nobel Prize. Weinberg was foundational in establishing the standard model of particle physics, and represented an enormous leap in understanding how this universe works. But his little 1987 paper, though more obscure, may tell us something about how the multiverse works, and can even be thought of as evidence for the existence of an enormous number of other universes.

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    Hosted by Matt O'Dowd
    Written by Matt O'Dowd
    Post Production by Leonardo Scholzer, Yago Ballarini & Stephanie Faria
    Directed by Andrew Kornhaber
    Associate Producer: Bahar Gholipour
    Executive Producer: Andrew Kornhaber
    Executive in Charge for PBS: Maribel Lopez
    Director of Programming for PBS: Gabrielle Ewing
    Assistant Director of Programming for PBS: John Campbell

    Spacetime is a production of Kornhaber Brown for PBS Digital Studios.
    This program is produced by Kornhaber Brown, which is solely responsible for its content.
    © 2025 PBS. All rights reserved.

    End Credits Music by J.R.S. Schattenberg: https://www.youtube.com/user/MultiDroideka

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  • PBS Space Time

    How Stars Destroy Each Other

    10/11/2026 | 20 mins.
    PBS Member Stations rely on viewers like you. To support your local station, go to: http://to.pbs.org/DonateSPACE↓ More info below ↓Uploaded 17-08-20Sign Up on Patreon to get access to the Space Time Discord! https://www.patreon.com/pbsspacetimeCheck out the Space Time Merch Storehttps://pbsspacetime.com/Sign up for the mailing list to get episode notifications and hear special announcements!https://mailchi.mp/1a6eb8f2717d/spacetimeOur galaxy is full of dysfunctional stellar relationships. With more than half of all stars existing in binary orbits, it’s inevitable that many stellar remnants will end up in parasitic spirals with their partners. Today we’re going to look at the worst of these - from the novae produced by white dwarfs, to X-ray binaries created by neutron stars and black holes - and much weirder things besides. Hosted by Matt O'DowdWritten by Matt O'DowdGraphics by Leonardo Scholzer, Yago Ballarini, and Pedro OsinskiDirected by: Andrew KornhaberCamera Operator: Bahaar GholipourExecutive Producers: Eric Brown and Andrew KornhaberEnd Credits Music by J.R.S. Schattenberg: https://www.youtube.com/channel/UCRl6-nb4iOnsij-vnpAjp0QSpecial Thanks to our Patrons! Big Bang SupportersRobert DoxtatorAhmad JodehCaed AldwychRadu NegulescuAlexander TamasMorgan HoughJuan BenetFabrice EapMark RosenthalDavid NicklasQuasar SupportersAlec S-LChristina OegrenMark HeisingVinnie FalcoHypernova Supporterswilliam bryanDrew HartJustin JermynJason FinnАнтон КочковJulian TyackeTimothy McCullochSyed AnsarJohn R. SlavikMathewDanton SpiveyDonal BotkinJohn PollockEdmund FokschanerJoseph SalomoneHank SMatthew O'Connorchuck zegarJordan YoungJohn HofmannGamma Ray Burst SupportersMichael BartonChristopher BarronJames RamseyMr TAndrew MannJeremiah Johnsonfieldsa eleanoryCody LubinskyPeter MertzKevin O'ConnellBryan DawleyRichard DeightonIsaac SuttellDevon RosenthalOliver FlanaganDawn M FinkBleys GoodsonDarryl J LyleRobert WalterjechamtBruce BIsmael MontecelM DMark Daniel CohenAndrew RichmondSimon OliphantMirik GogriDavid HughesAria AhmadBrandon LattinYannick WeynsNickolas Andrew FreemanProtius ProtiusBrian BlanchardShane CalimlimTybie FitzhughPatrick SuttonRobert IlardiEric KieblerTatiana VorovchenkoCraig StonahaMichael ConroyGraydon GossFrederic SimonGreg SmithSean WarniahaTonyfaceJohn RobinsonA GKevin LeeAdrian HatchYurii KonovaliukJohn FunaiCass CostelloGeoffrey ShortBradley JenkinsKyle HoferTim StephaniLuaanAlecZeroMalte UblNick VirtueScott GossettDavid BethalaDan WarrenJohn GriffithDaniel LyonsJosh ThomasDFaulkKevin WarneAndreas NautschBrandon Labonte Learn more about your ad choices. Visit megaphone.fm/adchoices
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  • PBS Space Time

    The Black Hole Information Paradox

    10/11/2026 | 20 mins.
    Viewers like you help make PBS (Thank you 😃) . Support your local PBS Member Station here: https://to.pbs.org/DonateSPACEUploaded 20-06-18Thank you to Brilliant for sponsoring this episode! To find out more, visit: https://brilliant.org/SpaceTimeWe’ve established by now that black holes are weird. The result of absolute gravitational collapse of a massive body: a point of hypothetical infinite density surrounded by an event horizon. At that horizon time is frozen and the fabric of space itself cascades inwards at the speed of light. Nothing can travel faster than light, and so nothing can escape from below the event horizon- not matter, not light, not even information. You can further support us on Patreon at https://www.patreon.com/pbsspacetimeGet your own Space Time t­-shirt at http://bit.ly/1QlzoBiTweet at us! @pbsspacetimeFacebook: facebook.com/pbsspacetimeEmail us! pbsspacetime [at] gmail [dot] comComment on Reddit: http://www.reddit.com/r/pbsspacetimeHelp translate our videos!https://www.youtube.com/timedtext_cs_panel?tab=2&c=UC7_gcs09iThXybpVgjHZ_7gPrevious Episode:Why Quantum Information is Never Destroyed https://youtu.be/HF-9Dy6iB_4These ideas are pretty mind-blowing, but as crazy as black holes are, they’re also kind of … simple. Don’t get me wrong; the math is complicated. But the objects themselves are simple. In fact every black hole in the universe, no matter how it formed or what happened to it afterwards, can be perfectly described with only three properties. Those properties are mass, angular momentum, and electric charge. Or at least this is the proposition behind the famous no-hair conjecture, or no-hair theorem. Hosted by Matt O'DowdWritten by Matt O'DowdGraphics by Grayson BlackmonAssistant Editing and Sound Design by Mike Petrow and Linda HuangMade by Kornhaber Brown (www.kornhaberbrown.com)Special thanks to our Patreon Big Bang, Quasar and Hypernova Supporters: Big BangCoolAsCatsDavid NicklasAnton LifshitsJoey RednerFabrice EapQuasarTambe BarsbayMayank M. MehrotaMars YenturMark RosenthalDean FuquaRoman PinchukColeslawPurdieHypernovaEdmund FokschanerMatthew O’ConnorEugene LawsonBarry HatfieldMartha HuntJoseph SalomoneChuck ZegarCraig PetersonJordan YoungRatfeastJohn HofmannThanks to our Patreon Gamma Ray Burst Supporters: James HughesFabian OlesenKris FernetJane MeyersJames FlowersGreg AllenDenys IvanovNick VirtueAlexey EromenkoNicholas RoseScott GossettMark VasilePatrick MurraySultan AlkhulaifiAlex SetoMichal-Peanut KarmiErik SteinKevin WarneJJ BagnellAvi GoldfingerJohn PettitFlorian StinglmayrBenoit Pagé-GuitardNathan LenizBrandon LabonteDavid CraneGreg WeissShannan CatalanoBrandon Cook Learn more about your ad choices. Visit megaphone.fm/adchoices
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About PBS Space Time
Space Time explores the outer reaches of space, the craziness of astrophysics, the possibilities of sci-fi, and anything else you can think of beyond Planet Earth with our astrophysicist host: Matthew O’Dowd. For all business inquiries and sponsorship opportunities please reach out to: pbsspacetime@lighthouseagents.com Matt O'Dowd spends his time studying the universe, especially really far-away things like quasars, super-massive black holes, and evolving galaxies. He uses telescopes in space to do it. Matt completed his Ph.D. at NASA's Space Telescope Science Institute, followed by work at the University of Melbourne and Columbia University. He's now a professor at the City University of New York's Lehman College and an Associate at the American Museum of Natural History's Hayden Planetarium. Previous host Gabe Perez-Giz is an astrophysicist who studies black hole physics. He received his Ph.D. from Columbia University and also hosted PBS Infinite Series. patreon.com/pbsspacetime

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