WEBVTT

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Welcome back to the Deep Dive. It's great to

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be here. Today we're pointing our lens, our most

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powerful lens, at a name that I think everyone

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knows. A name that's basically synonymous with

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space itself. Oh, absolutely. The Hubble Space

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Telescope. Exactly. But we're not just talking

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about the telescope. We're talking about the

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man, Edwin Hubble. And his personal story is

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just full of these incredible detours and remarkable

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turns. It really is. It's a common mistake to

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sort of conflate the man and the machine. But

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Edwin Hubble, the man, is, well, he's arguably

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the most important observational astronomer since

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Galileo. That's a huge statement. Since Galileo.

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I think it holds up. You have to understand,

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before his work. Our own galaxy, the Milky Way,

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was the entire cosmos. That was it. The whole

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universe. The whole thing. After him, we suddenly

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lived in this vast ocean of billions of other

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galaxies. He laid the groundwork, the observational

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foundation, for what we now call modern cosmology

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and extragalactic astronomy. Okay, so let's unpack

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that. That is a monumental legacy. Our mission

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for this deep dive is to synthesize his life

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and the foundational discoveries that really

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made that transformation possible. We've got

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our shared sources here, and they detail his,

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well, highly unusual path to science, some crucial

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detours during wartime, and most importantly,

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two primary revolutionary scientific discoveries.

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That's right. The first one is maybe the easiest

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to grasp. But it's no less profound. It's the

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conclusive proof that those nebulae, those fuzzy

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patches in the sky. Yeah, that everyone thought

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were just gas clouds. Exactly. He proved they

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weren't gas clouds inside our galaxy at all.

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They were entirely separate stellar systems,

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other galaxies, far, far outside the Milky Way.

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And the second discovery, which really launched

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us into the Big Bang era, is the empirical proof

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of what we now call Hubble's Law. The stunningly

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simple linear relationship between a galaxy's

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distance from us and its apparent speed moving

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away from us this was the first real observation

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that implied the expansion of the entire universe

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though as we'll get into hubble himself was famously

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and perhaps surprisingly skeptical of that interpretation

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he was and we absolutely have to explore that

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along with the complex history and you know the

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controversies around who discovered what first

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it's a fascinating story It seems like it's essential

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because his personal history really provides

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the context for his scientific rigor, doesn't

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it? It absolutely does. Before Hubble became

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the man who expanded the universe, he was a star

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athlete and, believe it or not, a reluctant law

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student. The journey to the top of Mount Wilson

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and that 100 -inch telescope was anything but

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a straight line. Okay, let's start there. Let's

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start with the unexpected prodigy. Edwin Powell

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Hubble, born 1889, Marshfield, Missouri. His

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family moves to Illinois in 1900. Mm -hmm. And

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when you look at his early years, high school,

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college, the sources are overwhelming. He was

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famous for being physically dominant, not some

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kind of intellectual prodigy. Right, which is

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so counterintuitive for a figure like this. What's

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fascinating is that the records actually highlight

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his spelling issues, which is a surprisingly

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human detail for a cosmic giant. I love that.

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But otherwise, he was a great student. It's just

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that the public recognition, the fame, it was

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all about his physical prowess. He was a phenomenon

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in high school sports. And that physical discipline,

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you can see how he later translated it into astronomical

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dedication. And we're not just talking about,

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you know, playing on a team. We're talking about

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elite. truly dominant performance. Oh, absolutely.

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The sources say he excelled in baseball, football,

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and track and field. This wasn't a hobby. This

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speaks to a kind of underlying drive and focus

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that's just off the charts. You give us an example.

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Well, there's this one detail that just jumps

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out. At a single high school track meet in 1906,

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one meet. He won seven first place finishes and

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a third place. Seven firsts in one day. In one

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day. Think about the sheer scale of that in all

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these different disciplines, running, jumping,

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throwing. It's just a hyper -focused, incredibly

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driven personality. And he carried that right

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into college at the University of Chicago. He

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wasn't just on the basketball team. No, he was

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leading it. He played multiple positions, center,

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shooting guard, whatever was needed. And in 1907,

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he led the university's team to their first ever

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Big Ten conference title. It's just a bizarre

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juxtaposition, isn't it? You have... one of the

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foundational figures of 20th century science.

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And at the same time, he's a Big Ten basketball

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champion. It is strange, but I think that competitive

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rigor, that ability to perform under pressure

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and just focus on a goal, that's the same trait

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we see resurface years later when he's locked

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in the freezing cold dome at Mount Wilson, staring

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through an eyepiece for hours. That makes sense.

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The discipline to endure those long nights of

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observation is probably the same kind of mental

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muscle you need for high -level athletics. I

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think so, yes. But okay. Despite this huge focus

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on sports, his academic interests were still

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pointing in the right direction. His undergraduate

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studies were in mathematics, astronomy, and philosophy.

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Right, so the intellectual foundation was definitely

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being built. He got his Bachelor of Science in

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1910. And there's another really important connection

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here that often gets missed. What's that? His

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exposure to truly rigorous experimental physics.

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For a year during his undergrad, Hubble served

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as a student laboratory assistant for Robert

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Millikan. Wow. Robert Millikan, who, of course,

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went on to win the Nobel Prize for his oil drop

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experiment for measuring the charge of an electron.

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The very same. Yeah. That experience had to have

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profoundly shaped Hubble's methodology. It would

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have emphasized precise measurement, empirical

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evidence above all the theoretical guesswork.

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It must have embedded this philosophy of show

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me the data. Absolutely. He was learning from

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one of the best experimentalists on the planet

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how to design observations that minimized error

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and maximize certainty. That training is so crucial

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because later in his life, Hubble becomes the

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ultimate empiricist. He trusts what he observes

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through the telescope far more than what any

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theorist predicts on a blackboard but then right

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when he's on this path comes this huge confusing

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detour the promise and the pivot his path was

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just abruptly shifted by a promise he made to

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his dying father right his father passed away

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in 1913 and hubble feeling this deep sense of

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duty followed his father's wish that he pursues

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a career in law So this leads him to accept a

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Rhodes Scholarship. At the Queen's College, Oxford.

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And instead of focusing on physics or astronomy,

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which was clearly his passion, he studies jurisprudence.

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Law school in England. It seems so completely

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opposed to celestial mechanics. It was a total

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abandonment of his passion, at least for a time.

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While he was there, he did broaden his studies.

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He added literature and Spanish, eventually got

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an MA degree. But the core focus was legal training.

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It's just hard to imagine the man who discovered

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the expanding universe arguing torts. It really

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is. Though maybe that legal training, that focus

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on evidence and logical argument, maybe that

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subtly reinforced his scientific approach. That's

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a great point. It's all about examining evidence,

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building a case, and avoiding claims you can't

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substantiate. That's good science and it's good

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law. So when he comes back to the Midwest after

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his father's death, his lack of passion for law

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becomes, well, pretty obvious. His actions speak

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volumes. Instead of opening a legal practice,

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he takes what you might call a teaching interlude.

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He ends up teaching Spanish, physics, and math

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at a high school in Indiana. New Albany High

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School. And, of course. And, of course, he coached

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the boys' basketball team. You can't keep him

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away from the court. It's just a wonderful image,

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isn't it? The future titan of cosmology explaining

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the quadratic formula and then diagramming a

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pick -and -roll play. It is. But thankfully for

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the history of science, this was a very short

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-lived phase. Right. This period probably just

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solidified for him how much he wanted to be doing

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research. I think so. And the academic community

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saw it too. A former professor from the University

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of Chicago basically intervened, using Hubble's

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clear talent to guide him back onto the scientific

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track. And that brings us to his formal return

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to astronomy. He enters graduate school at the

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University of Chicago's Yerkes Observatory. And

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this time, the focus is absolute. He earns his

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Ph .D. in 1921. And listen to the title of his

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dissertation, Photographic Investigations of

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Faint Nebulae. It's prophetic. It's the exact

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subject that would define his entire life's work.

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His intention was already centered on figuring

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out what those fuzzy patches really were. Precisely.

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What was it about Yerkes Observatory that made

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it the perfect place for him to start this work?

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What kind of tools did they have? Yerkes was

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a world -class institution established by George

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Ellery Hale, a name we'll hear again. It had

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groundbreaking equipment. The most famous instrument

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was the 40 -inch refractor telescope, which was

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enormous. But critically, he also got experience

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with an innovative... 26 -inch reflector telescope.

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And reflectors, which use mirrors instead of

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lenses, are much better for capturing the incredibly

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faint light you need for deep sky photography.

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That gave him a crucial skill set. And just as

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his academic path is getting back on track, it's

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interrupted again by a global conflict, World

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War I. Yes, he actually rushes to finish his

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Ph .D. requirements so he can enlist in the U

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.S. Army. He was commissioned into the 86th Division,

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rises to the rank of major, which again speaks

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to his leadership abilities. Absolutely. The

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division was sent overseas in 1918, but the armistice

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was signed soon after. So our sources say that

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while some of the personnel were used as replacements

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elsewhere, the 86th Division itself never actually

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saw combat. So he served honorably. He got the

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distinction of being a major. But his observational

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career was able to begin pretty much right after

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the war ended. Exactly. And there's one more

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crucial detail. After the war, he actually spent

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a year in the UK at Cambridge sort of reengaging

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with his scientific studies before he accepted

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the one offer that would change astronomy forever.

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The year 1919. This is the pivot point. This

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is the moment Edwin Hubble meets the instrument

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that will define his legacy. The call to California.

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That call came directly from George Ellery Hale,

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the man who built Yerkes. Hale was now the founder

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and director of the Carnegie Institution's Mount

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Wilson Observatory. He recognized Hubble's talent.

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He saw Hubble's rigor and his potential and offered

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him a staff position. Hubble accepted, and he

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stayed at Mount Wilson until he died in 1953.

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And his timing was just perfect. His arrival

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lined up exactly with the completion of the most

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powerful observational tool in human history

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up to that point. It was the perfect storm of

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talent meeting opportunity. The 100 -inch or

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2 .5 -meter Hooker telescope had just been completed.

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And to put that in context... This was the world's

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largest telescope for decades. It gathered so

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much more light than any previous instrument.

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It offered the resolution you needed to finally

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distinguish faint individual stars inside those

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distant nebulae. Without the Hooker telescope,

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Hubble's work would have been impossible. They

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would have just remained fuzzy patches. The 100

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-inch Hooker was his work... It enabled both

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of the revolutionary discoveries we're going

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to talk about. But he didn't stop there. He was

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always at the cutting edge. Absolutely. He was

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always pushing the limits. Shortly before his

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death in 1953, he became the first astronomer

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to use the brand new, even bigger, 200 -inch

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Hale telescope at Palomar Observatory. So there's

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this incredible historical symmetry. His career

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is basically defined by his use of the two most

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powerful instruments built in the first half

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of the 20th century. It is a perfect alignment.

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Okay, let's pivot back now to another one of

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those surprising detours. It really proves the

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versatility of his mind. His skills were so transferable

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that they became vital during the next global

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conflict, World War II. This is a really remarkable

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chapter. During the war... Hubble puts his astronomy

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career on hold and serves as a civilian at the

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U .S. Army's Aberdeen Proving Ground in Maryland.

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He goes from tracking distant galaxies to...

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To tracking high -velocity projectiles. He was

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the chief of the external ballistics branch of

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the Ballistic Research Laboratory. Ballistics,

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the physics of projectiles in flight. It seems

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like a world away from extragalactic astronomy.

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It does, but the underlying skills of observation,

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precise measurement, and calculation are identical.

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That's the key connection. So what was his job?

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He was directing huge amounts of research focused

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on exterior ballistics. His mandate was to apply

00:12:36.940 --> 00:12:40.080
scientific rigor to increase the effective firepower

00:12:40.080 --> 00:12:43.539
of bombs, rockets, and other projectiles. It

00:12:43.539 --> 00:12:46.500
required incredibly detailed high -speed observation

00:12:46.500 --> 00:12:49.159
under very difficult conditions. And he didn't

00:12:49.159 --> 00:12:51.340
just manage the research. He actually used his

00:12:51.340 --> 00:12:54.120
training in optics and photography to invent

00:12:54.120 --> 00:12:57.159
new tools for this. He was a true innovator in

00:12:57.159 --> 00:12:59.100
the lab, just like he was on the mountaintop.

00:12:59.399 --> 00:13:01.620
The most outstanding development that's credited

00:13:01.620 --> 00:13:04.080
to him from this period was the high -speed clock

00:13:04.080 --> 00:13:07.019
camera. A clock camera. That implies extremely

00:13:07.019 --> 00:13:09.840
precise timing. Exactly, which is critical for

00:13:09.840 --> 00:13:11.879
measuring the trajectory and speed of ordnance.

00:13:12.350 --> 00:13:14.909
This invention was a game changer. What did it

00:13:14.909 --> 00:13:17.289
allow them to do? It allowed researchers to precisely

00:13:17.289 --> 00:13:19.889
study the flight characteristics of bombs and

00:13:19.889 --> 00:13:22.509
low -velocity projectiles. By capturing their

00:13:22.509 --> 00:13:24.870
exact movements, their rotation, their stability

00:13:24.870 --> 00:13:27.009
in flight with extremely high time resolution,

00:13:27.370 --> 00:13:29.909
they could gather the empirical data they needed

00:13:29.909 --> 00:13:32.070
to redesign the ordnance for better accuracy

00:13:32.070 --> 00:13:34.389
and performance. So he took the observational

00:13:34.389 --> 00:13:36.970
rigor he used to measure the expansion of space.

00:13:37.389 --> 00:13:40.190
And applied it to the expansion of military might.

00:13:40.639 --> 00:13:43.379
The results of his studies were explicitly credited

00:13:43.379 --> 00:13:45.639
with improving the design and effectiveness of

00:13:45.639 --> 00:13:48.779
the nation's ordinance. It was high impact, practical

00:13:48.779 --> 00:13:51.340
physics, a world away from the philosophical

00:13:51.340 --> 00:13:54.960
debates of cosmology. And this work earned him

00:13:54.960 --> 00:13:58.889
significant recognition. It did. In 1946, he

00:13:58.889 --> 00:14:01.750
received the Legion of Merit Award for his distinguished

00:14:01.750 --> 00:14:05.169
civilian service. It just highlights the incredible

00:14:05.169 --> 00:14:08.370
breadth of his genius. He was capable of calculating

00:14:08.370 --> 00:14:11.070
the size of the universe and, at the same time,

00:14:11.110 --> 00:14:13.850
optimizing the aerodynamics of a bomb. Okay,

00:14:13.909 --> 00:14:15.990
let's return to Mount Wilson and to the work

00:14:15.990 --> 00:14:18.370
that truly defined him. We need to set the scene

00:14:18.370 --> 00:14:21.769
here. Before the 1920s, the astronomical community

00:14:21.769 --> 00:14:23.669
was in the middle of what's often called the

00:14:23.669 --> 00:14:26.440
Great Debate. What was that about? The core of

00:14:26.440 --> 00:14:28.399
the debate was about the size of the universe.

00:14:28.659 --> 00:14:31.399
The established scientific view, which was championed

00:14:31.399 --> 00:14:33.580
by figures like Harlow Shapley, was that the

00:14:33.580 --> 00:14:36.179
entire cosmos was contained within our own Milky

00:14:36.179 --> 00:14:38.019
Way galaxy. That was it. That was the universe.

00:14:38.340 --> 00:14:40.679
That was the universe. And all those blurry,

00:14:40.759 --> 00:14:43.039
fuzzy patches you could see in telescopes, the

00:14:43.039 --> 00:14:46.519
nebulae, like Andromeda, they were believed to

00:14:46.519 --> 00:14:49.659
be gas clouds or maybe forming star systems,

00:14:49.860 --> 00:14:53.700
but inside our galaxy. Distant, but internal.

00:14:54.440 --> 00:14:56.080
It's important to note, though, that the idea

00:14:56.080 --> 00:14:59.620
of external galaxies or island universes wasn't

00:14:59.620 --> 00:15:02.860
new. Immanuel Kant had suggested it back in 1755.

00:15:03.159 --> 00:15:05.100
Right. But without empirical proof, it was just

00:15:05.100 --> 00:15:07.340
philosophy. That is the crucial distinction here.

00:15:07.539 --> 00:15:09.460
Hubble is the one who turned that philosophy

00:15:09.460 --> 00:15:12.740
into hard observational fact. And to do that,

00:15:12.779 --> 00:15:15.419
he needed a reliable measuring stick for cosmic

00:15:15.419 --> 00:15:18.740
distance. And that stick was the cepheid variable

00:15:18.740 --> 00:15:21.440
star. Exactly. Can you walk us through the genius

00:15:21.440 --> 00:15:24.220
of using cepheids? They were discovered by Henrietta

00:15:24.220 --> 00:15:27.200
Swan Leavitt in 1908. How do they work as a standard

00:15:27.200 --> 00:15:29.019
candle? Cepheid variables are extraordinary.

00:15:29.179 --> 00:15:31.460
They're a type of star that pulsates, it regularly

00:15:31.460 --> 00:15:34.299
expands and contracts, and that causes its brightness

00:15:34.299 --> 00:15:36.940
to oscillate, to go up and down. Leavitt's brilliant

00:15:36.940 --> 00:15:39.379
discovery was that there is a direct lockstep

00:15:39.379 --> 00:15:42.059
relationship between how long it takes for the

00:15:42.059 --> 00:15:44.879
star to complete one pulsation cycle, its period,

00:15:45.139 --> 00:15:48.330
and how bright that star truly is. its intrinsic

00:15:48.330 --> 00:15:50.669
luminosity. So the longer the period, the brighter

00:15:50.669 --> 00:15:52.889
the star. Exactly. So they become a standard

00:15:52.889 --> 00:15:55.350
candle. Because as soon as you measure the period

00:15:55.350 --> 00:15:57.909
of its pulse, which is easy to do, you know its

00:15:57.909 --> 00:15:59.509
inherent brightness. You know how bright it's

00:15:59.509 --> 00:16:01.450
supposed to be. Okay, so if you know how bright

00:16:01.450 --> 00:16:04.090
the star should be, and you measure how dim it

00:16:04.090 --> 00:16:06.529
appears from Earth, the difference is purely

00:16:06.529 --> 00:16:09.570
a function of distance. The dimmer it is, the

00:16:09.570 --> 00:16:11.909
farther away it must be. Precisely. It's a simple

00:16:11.909 --> 00:16:14.029
geometric principle. The challenge was applying

00:16:14.029 --> 00:16:16.399
it. The older telescopes just couldn't gather

00:16:16.399 --> 00:16:19.019
enough light to resolve these individual, very

00:16:19.019 --> 00:16:21.679
faint, sephiide stars in those distant nebulae.

00:16:21.740 --> 00:16:24.539
The 100 -inch Hooker telescope was the first

00:16:24.539 --> 00:16:26.700
instrument powerful enough to do it. And this

00:16:26.700 --> 00:16:30.379
brings us to the great revelation of 1924. Hubble

00:16:30.379 --> 00:16:32.940
is meticulously photographing Andromeda, the

00:16:32.940 --> 00:16:35.620
Triangulum Nebula. What happens when he finally

00:16:35.620 --> 00:16:38.720
finds and measures a septide in Andromeda? In

00:16:38.720 --> 00:16:42.340
late 1923 and early 1924, he finally manages

00:16:42.340 --> 00:16:45.379
to resolve individual stars and confirm a Cepheid

00:16:45.379 --> 00:16:47.919
in what was then called the Andromeda Nebula.

00:16:48.159 --> 00:16:51.960
He famously scrawled VAR for variable right next

00:16:51.960 --> 00:16:54.039
to the star on his photographic plate. And then

00:16:54.039 --> 00:16:56.139
he measured its period. The distance calculation

00:16:56.139 --> 00:16:59.200
must have been instantly shocking. It was. When

00:16:59.200 --> 00:17:01.299
he plugged the numbers into the period luminosity

00:17:01.299 --> 00:17:03.860
formula, the calculated distance was staggering.

00:17:04.099 --> 00:17:07.059
It was millions of light years away. At the time,

00:17:07.079 --> 00:17:09.079
the entire Milky Way was thought to be maybe

00:17:09.079 --> 00:17:11.519
a few hundred thousand light years across. This

00:17:11.519 --> 00:17:14.059
object was far, far outside the known boundary

00:17:14.059 --> 00:17:16.839
of our galaxy. So that single observation proved,

00:17:17.180 --> 00:17:19.720
conclusively, that the Andromeda Nebula was not

00:17:19.720 --> 00:17:22.339
a nebula at all. It was a separate, colossal

00:17:22.339 --> 00:17:25.299
collection of stars. An entire galaxy outside

00:17:25.299 --> 00:17:27.880
our own. It dismantled the existing cosmological

00:17:27.880 --> 00:17:30.559
model overnight. The universe instantly expanded

00:17:30.559 --> 00:17:33.000
from one single stellar system, the Milky Way,

00:17:33.160 --> 00:17:36.039
to this vast, multi -galactic archipelago. It

00:17:36.039 --> 00:17:38.619
is the definition of a scientific paradigm shift.

00:17:38.799 --> 00:17:41.660
This was seismic news, and it faced strong resistance

00:17:41.660 --> 00:17:43.859
from the old guard, didn't it? Particularly from

00:17:43.859 --> 00:17:46.079
Harlow Shapley at Harvard. Oh, the resistance

00:17:46.079 --> 00:17:49.339
was fierce. Shapley's model of the Milky Way

00:17:49.339 --> 00:17:51.640
was the established view, and Hubble's finding

00:17:51.640 --> 00:17:54.660
completely undermined it. But the empirical evidence

00:17:54.660 --> 00:17:57.539
from Mount Wilson was just too robust to ignore.

00:17:57.779 --> 00:18:00.000
And Hubble, interestingly, took his findings

00:18:00.000 --> 00:18:02.789
to the public. pretty quickly. He did. His findings

00:18:02.789 --> 00:18:04.670
for Andromeda were first published in the New

00:18:04.670 --> 00:18:08.569
York Times on November 23rd, 1924. It ensured

00:18:08.569 --> 00:18:10.369
immediate public awareness that the universe

00:18:10.369 --> 00:18:12.829
had just gotten a whole lot bigger. And then

00:18:12.829 --> 00:18:14.809
he presented the results formally to the American

00:18:14.809 --> 00:18:18.910
Astronomical Society on January 1st, 1925. And

00:18:18.910 --> 00:18:21.430
that cemented it. He was the man who discovered

00:18:21.430 --> 00:18:24.369
the external galaxies. The speed at which this

00:18:24.369 --> 00:18:26.630
discovery changed the course of science is almost

00:18:26.630 --> 00:18:29.490
unprecedented. And beyond just proving they existed.

00:18:29.980 --> 00:18:32.579
Hubble brought order to this new cosmic zoo.

00:18:32.759 --> 00:18:35.460
He created a classification system. That's right,

00:18:35.500 --> 00:18:38.039
the Hubble sequence. It's often visualized as

00:18:38.039 --> 00:18:40.730
the tuning fork diagram. He categorized galaxies

00:18:40.730 --> 00:18:43.430
based on how they looked, their morphology. You

00:18:43.430 --> 00:18:45.589
had ellipticals, which were smooth and featureless,

00:18:45.789 --> 00:18:49.009
spirals with their beautiful arms, barred spirals,

00:18:49.009 --> 00:18:51.130
which have a central bar structure, and then

00:18:51.130 --> 00:18:54.069
irregulars. And that classification system is

00:18:54.069 --> 00:18:55.930
still the foundation we use today, isn't it?

00:18:56.009 --> 00:18:58.589
It is. Despite all the refinements over the years,

00:18:58.670 --> 00:19:00.789
it's still the fundamental taxonomy for galaxies.

00:19:01.269 --> 00:19:04.130
He didn't just find new things. He started organizing

00:19:04.130 --> 00:19:06.589
the cosmic map for everyone who came after him.

00:19:06.769 --> 00:19:09.029
Okay, so once Hubble established these vast...

00:19:09.069 --> 00:19:12.069
distances, the next crucial question was how

00:19:12.069 --> 00:19:15.069
are these massive structures moving relative

00:19:15.069 --> 00:19:17.970
to us? And this leads to his second monumental

00:19:17.970 --> 00:19:21.349
discovery. The expanding universe. This stage

00:19:21.349 --> 00:19:23.789
required synthesizing two different sets of data.

00:19:24.309 --> 00:19:27.210
First, Hubble and his team, using the suffade

00:19:27.210 --> 00:19:30.230
method and other techniques, painstakingly estimated

00:19:30.230 --> 00:19:32.869
the distances to dozens of these new galaxies.

00:19:33.170 --> 00:19:36.250
By 1929, he had distance estimates for about

00:19:36.250 --> 00:19:38.750
24 of them. So he had the distance part of the

00:19:38.750 --> 00:19:40.750
equation. Where did the velocity part come from?

00:19:40.930 --> 00:19:43.400
That came from pre -existing work. The crucial

00:19:43.400 --> 00:19:45.779
velocity data came from measurements of what's

00:19:45.779 --> 00:19:48.079
called radial velocity, the motion along our

00:19:48.079 --> 00:19:50.019
line of sight. Which you measure from redshift.

00:19:50.430 --> 00:19:52.970
Exactly. And those redshift measurements were

00:19:52.970 --> 00:19:55.710
done primarily by an astronomer named Avesto

00:19:55.710 --> 00:19:58.609
Slipher at the Lowell Observatory. Slipher had

00:19:58.609 --> 00:20:01.109
been observing these nebulae for years and found

00:20:01.109 --> 00:20:03.309
that the vast majority of them were redshifted.

00:20:03.390 --> 00:20:05.490
Meaning they were moving away from us at tremendous

00:20:05.490 --> 00:20:08.910
speeds. At incredible speeds. Hubble relied heavily

00:20:08.910 --> 00:20:11.430
on Slipher's work and later on measurements by

00:20:11.430 --> 00:20:14.109
his own assistant, Milton Humison, to get the

00:20:14.109 --> 00:20:16.809
velocity for each galaxy. So he takes his distances

00:20:16.809 --> 00:20:19.920
and he plots them against the velocity. from

00:20:19.920 --> 00:20:22.380
Slipher and Humason. And what did that graph

00:20:22.380 --> 00:20:25.779
look like in 1929? The result was an elegant,

00:20:25.859 --> 00:20:29.319
terrifyingly simple straight line, a linear relationship.

00:20:29.859 --> 00:20:33.119
This became Hubble's law. It states that a galaxy's

00:20:33.119 --> 00:20:35.519
recessional velocity, how fast it's moving away,

00:20:35.700 --> 00:20:38.319
is directly proportional to how far away it is.

00:20:38.400 --> 00:20:41.160
Right. Mathematically, it's just v equals h -naught

00:20:41.160 --> 00:20:44.180
times dh -naught is the constant of proportionality,

00:20:44.240 --> 00:20:46.119
the Hubble constant. And what does that simple

00:20:46.119 --> 00:20:48.299
relationship imply about the universe as a whole?

00:20:48.650 --> 00:20:50.450
It implies that the universe is undergoing a

00:20:50.450 --> 00:20:54.049
uniform systematic expansion. If Galaxy B is

00:20:54.049 --> 00:20:57.029
twice as far away as Galaxy A, it appears to

00:20:57.029 --> 00:21:00.049
be receding at twice the speed. This only makes

00:21:00.049 --> 00:21:02.369
sense if space itself is stretching, carrying

00:21:02.369 --> 00:21:04.970
the galaxies along with it. So there's no center

00:21:04.970 --> 00:21:07.630
to the expansion. Exactly. Every galaxy sees

00:21:07.630 --> 00:21:10.069
every other galaxy receding from it. It's a profound

00:21:10.069 --> 00:21:12.819
idea. But this brings us immediately to the calibration

00:21:12.819 --> 00:21:16.019
problem. It's a huge issue. And it's vital for

00:21:16.019 --> 00:21:18.279
understanding why Hubble himself was so skeptical.

00:21:18.500 --> 00:21:21.200
It is. His initial distance estimates, while

00:21:21.200 --> 00:21:23.779
they were flawless relative to each other, the

00:21:23.779 --> 00:21:26.779
absolute scale was dramatically wrong. Okay,

00:21:26.779 --> 00:21:29.039
wrong. He was off by a factor of about seven.

00:21:29.220 --> 00:21:31.680
His calculated distances were way too small.

00:21:31.859 --> 00:21:34.039
And what caused that error? It was later found

00:21:34.039 --> 00:21:36.579
to be a combination of things. He was confusing

00:21:36.579 --> 00:21:39.000
two different types of Cepheid variable stars,

00:21:39.140 --> 00:21:41.400
which have different properties. And in some

00:21:41.400 --> 00:21:44.220
cases, he was mistaking extremely bright gas

00:21:44.220 --> 00:21:46.740
clouds in other galaxies for the brightest individual

00:21:46.740 --> 00:21:50.140
stars. These mistakes basically meant his yardstick

00:21:50.140 --> 00:21:52.720
was calibrated incorrectly. So his distance scale

00:21:52.720 --> 00:21:54.660
was too small. What was the catastrophic consequence

00:21:54.660 --> 00:21:57.099
of that? Well, if the distances are smaller,

00:21:57.319 --> 00:21:59.700
it means the expansion rate has to be much faster

00:21:59.700 --> 00:22:02.900
to get galaxies to where they are today. calculated

00:22:02.900 --> 00:22:05.980
value for the Hubble constant, H naught, was

00:22:05.980 --> 00:22:09.420
500 kilometers per second per megaparsec. Okay,

00:22:09.480 --> 00:22:12.400
let's pause. A megaparsec is a million parsecs,

00:22:12.400 --> 00:22:16.079
and a parsec is about 3 .26 light years. So that's

00:22:16.079 --> 00:22:18.299
a unit of distance. Right. So he's saying for

00:22:18.299 --> 00:22:21.119
every million parsecs farther away a galaxy is,

00:22:21.319 --> 00:22:23.940
its apparent velocity increases by 500 kilometers

00:22:23.940 --> 00:22:27.529
per second. And that number 500 created a massive

00:22:27.529 --> 00:22:30.390
crisis, didn't it? A huge crisis, because the

00:22:30.390 --> 00:22:32.529
Hubble constant is directly linked to the age

00:22:32.529 --> 00:22:35.029
of the universe. If you run the clock backwards,

00:22:35.289 --> 00:22:38.269
a value of 500 gives you an estimated age for

00:22:38.269 --> 00:22:41.009
the cosmos of only about 2 billion years. Which

00:22:41.009 --> 00:22:43.130
was the problem. It was a catastrophic problem.

00:22:43.390 --> 00:22:46.650
By the 1930s, geologists using radiometric dating

00:22:46.650 --> 00:22:48.869
had already established that rocks on Earth were

00:22:48.869 --> 00:22:52.029
older than 3 billion years old. So Hubble's own

00:22:52.029 --> 00:22:54.869
data, taken at face value, forced this logical

00:22:54.869 --> 00:22:57.710
obsession. The universe appeared to be younger

00:22:57.710 --> 00:23:00.849
than the planets inside it. Precisely. And that

00:23:00.849 --> 00:23:03.269
massive contradiction is the empirical foundation

00:23:03.269 --> 00:23:06.450
for his famous skepticism. His dedication to

00:23:06.450 --> 00:23:08.630
observation meant he could not accept a conclusion

00:23:08.630 --> 00:23:11.250
that contradicted known facts about the age of

00:23:11.250 --> 00:23:13.390
our own planet. This is what fueled his caution

00:23:13.390 --> 00:23:16.029
for decades. And this story is further complicated

00:23:16.029 --> 00:23:19.130
by the Lemaitre priority issue. George Lemaitre

00:23:19.130 --> 00:23:21.670
had theoretically predicted this exact relationship

00:23:21.670 --> 00:23:24.930
before Hubble published it. He did. Lemaitre,

00:23:25.089 --> 00:23:27.809
a Belgian physicist and a Catholic priest, published

00:23:27.809 --> 00:23:30.029
the theoretical prediction for an expanding universe

00:23:30.029 --> 00:23:33.329
in 1927 in French, using Einstein's equations

00:23:33.329 --> 00:23:36.140
of general relativity. He even included some

00:23:36.140 --> 00:23:38.619
initial observational data to support it. That

00:23:38.619 --> 00:23:41.980
was two full years before Hubble's famous 1929

00:23:41.980 --> 00:23:45.740
paper. So historically, Lemaitre has both conceptual

00:23:45.740 --> 00:23:48.299
and chronological priority. This all ties into

00:23:48.299 --> 00:23:50.160
Hubble's own reluctance to even interpret his

00:23:50.160 --> 00:23:52.819
data as true expansion. Right. He was the ultimate

00:23:52.819 --> 00:23:55.220
empiricist, always wary of theoretical speculation.

00:23:55.460 --> 00:23:58.240
He deliberately used the term apparent velocities

00:23:58.240 --> 00:24:00.420
to describe the recession of the galaxies. So

00:24:00.420 --> 00:24:03.460
not real velocities. He was being cautious. He

00:24:03.460 --> 00:24:05.660
wrote in his correspondence that the interpretation

00:24:05.660 --> 00:24:07.980
of this correlation should be left to the very

00:24:07.980 --> 00:24:10.539
few others who are competent to discuss the matter

00:24:10.539 --> 00:24:13.980
with authority, meaning the theorists like Einstein

00:24:13.980 --> 00:24:16.059
and de Sitter. He thought of an observational

00:24:16.059 --> 00:24:18.980
correlation, not necessarily proof that the fabric

00:24:18.980 --> 00:24:21.519
of space was expanding. So what is the modern

00:24:21.519 --> 00:24:24.119
view? Is it a Doppler shift or something else?

00:24:24.480 --> 00:24:26.880
That's a crucial distinction. A traditional Douglas

00:24:26.880 --> 00:24:29.059
shift is when an object moves through space.

00:24:29.339 --> 00:24:32.480
But what we see with distant galaxies, the cosmological

00:24:32.480 --> 00:24:36.059
redshift, is now interpreted as an increase in

00:24:36.059 --> 00:24:38.259
the proper distance between them because the

00:24:38.259 --> 00:24:41.519
fabric of space -time itself is expanding. Can

00:24:41.519 --> 00:24:44.230
you give us an analogy? The classic one is raisin

00:24:44.230 --> 00:24:46.769
bread dough rising in an oven. The raisins are

00:24:46.769 --> 00:24:48.609
the galaxies and they're fixed in the dough,

00:24:48.730 --> 00:24:51.450
which is space. As the dough expands, all the

00:24:51.450 --> 00:24:53.809
raisins move farther apart from each other, but

00:24:53.809 --> 00:24:55.730
they aren't actually moving through the dough.

00:24:56.200 --> 00:24:58.380
I see. So the light traveling from one raisin

00:24:58.380 --> 00:25:00.640
to another gets stretched as the dough expands.

00:25:01.359 --> 00:25:03.980
Exactly. The light waves are stretched, making

00:25:03.980 --> 00:25:07.220
them redder. That's cosmological redshift. It's

00:25:07.220 --> 00:25:09.640
different from a Doppler shift, but for nearby

00:25:09.640 --> 00:25:12.220
galaxies, the math works out to be almost the

00:25:12.220 --> 00:25:14.440
same, which is why it's easy to confuse them.

00:25:15.079 --> 00:25:17.859
But Hubble's caution was justified because his

00:25:17.859 --> 00:25:20.140
observations alone couldn't prove one over the

00:25:20.140 --> 00:25:22.779
other. And he held on to this skepticism for

00:25:22.779 --> 00:25:25.240
his whole career. He kept questioning the Big

00:25:25.240 --> 00:25:28.000
Bang interpretation. He did. Until the end of

00:25:28.000 --> 00:25:29.960
his career, he maintained that a model where

00:25:29.960 --> 00:25:33.759
no true expansion exists was still a viable possibility.

00:25:34.039 --> 00:25:36.480
He was driven by observations that suggested

00:25:36.480 --> 00:25:39.240
a uniform distribution of galaxies, which he

00:25:39.240 --> 00:25:41.740
felt didn't quite fit the sudden explosion idea

00:25:41.740 --> 00:25:44.519
implied by that early high value of his constant.

00:25:44.980 --> 00:25:47.740
This story is just so tied up with Albert Einstein's

00:25:47.740 --> 00:25:49.960
own intellectual journey. Let's talk about what

00:25:49.960 --> 00:25:52.400
Einstein later called his biggest blunder. Yes,

00:25:52.599 --> 00:25:54.960
this just highlights the incredible power of

00:25:54.960 --> 00:25:57.839
observation to overturn even the most deeply

00:25:57.839 --> 00:26:01.940
held theoretical beliefs. Around 1917, Einstein

00:26:01.940 --> 00:26:05.240
had completed general relativity and his equations,

00:26:05.380 --> 00:26:08.039
when applied to the universe as a whole, suggested

00:26:08.039 --> 00:26:10.480
that the cosmos had to be dynamic. It should

00:26:10.480 --> 00:26:13.099
be either expanding or contracting. But Einstein.

00:26:13.690 --> 00:26:16.369
Like pretty much every scientist of his era had

00:26:16.369 --> 00:26:19.250
this philosophical preference for a static, eternal

00:26:19.250 --> 00:26:22.809
universe. He did. And to force his equations

00:26:22.809 --> 00:26:26.049
to produce a static model, he introduced a term

00:26:26.049 --> 00:26:29.880
he called the cosmological constant. It was basically

00:26:29.880 --> 00:26:33.099
a mathematical fudge factor he invented to create

00:26:33.099 --> 00:26:35.180
a repulsive force that would perfectly balance

00:26:35.180 --> 00:26:37.720
gravity and hold the universe still. So the greatest

00:26:37.720 --> 00:26:40.000
theorist of the age introduces this mathematical

00:26:40.000 --> 00:26:43.400
trick to preserve a static universe. Only to

00:26:43.400 --> 00:26:45.359
have the greatest observer of the age, Hubble,

00:26:45.559 --> 00:26:48.019
come along and prove that the universe was decidedly

00:26:48.019 --> 00:26:50.819
not static. It's the ultimate irony. And when

00:26:50.819 --> 00:26:52.700
Einstein learned of Hubble's work? He realized

00:26:52.700 --> 00:26:55.099
his theoretical bias had blinded him. He saw

00:26:55.099 --> 00:26:57.240
the data, Slipper's redshifts and Hubble's plot,

00:26:57.380 --> 00:26:59.279
and understood that the expansion was real. And

00:26:59.279 --> 00:27:01.519
they actually met, right? They did. Einstein

00:27:01.519 --> 00:27:05.119
visited Mount Wilson Observatory in 1931. He

00:27:05.119 --> 00:27:07.339
met with Hubble. He saw the telescope. He talked

00:27:07.339 --> 00:27:10.099
with the observational team. And after that visit,

00:27:10.220 --> 00:27:13.039
he famously and publicly retracted the cosmological

00:27:13.039 --> 00:27:15.839
constant, later calling it the biggest blunder

00:27:15.839 --> 00:27:18.849
of my life. He accepted the expansion based on

00:27:18.849 --> 00:27:21.329
the evidence. Which creates this second layer

00:27:21.329 --> 00:27:24.089
of irony. As Einstein is finally accepting the

00:27:24.089 --> 00:27:26.630
expansion based on Hubble's data, Hubble himself

00:27:26.630 --> 00:27:29.089
is still internally questioning what that data

00:27:29.089 --> 00:27:31.829
really means. It's incredible, isn't it? Hubble

00:27:31.829 --> 00:27:34.190
remains skeptical. He was so troubled by that

00:27:34.190 --> 00:27:36.430
age discrepancy and the uniform distribution

00:27:36.430 --> 00:27:40.309
of galaxies. In a 1941 report based on a six

00:27:40.309 --> 00:27:43.009
-year survey, he explicitly argued that his results

00:27:43.009 --> 00:27:45.609
did not support the pure expanding universe theory.

00:27:46.279 --> 00:27:48.299
He said the uniformity didn't fit the explosion

00:27:48.299 --> 00:27:50.599
idea. It shows this deep intellectual split.

00:27:50.880 --> 00:27:53.700
Hubble is saying, my telescope shows me a universe

00:27:53.700 --> 00:27:56.079
that looks uniform, and my numbers say the universe

00:27:56.079 --> 00:27:58.359
is younger than the Earth, so I have to question

00:27:58.359 --> 00:28:00.859
the expansion interpretation. it's a powerful

00:28:00.859 --> 00:28:03.960
lesson in scientific humility he refused to let

00:28:03.960 --> 00:28:07.180
theory dictate his observations he held open

00:28:07.180 --> 00:28:09.859
the possibility that redshift was caused by in

00:28:09.859 --> 00:28:13.079
his words a hitherto unrecognized principle of

00:28:13.079 --> 00:28:16.259
nature like the tired light theory exactly the

00:28:16.259 --> 00:28:18.960
idea that light simply loses energy as it travels

00:28:18.960 --> 00:28:22.059
vast distances that's been ruled out now but

00:28:22.059 --> 00:28:24.700
his willingness to challenge the prevailing view

00:28:24.700 --> 00:28:27.740
based on conflicting data is what made him such

00:28:27.740 --> 00:28:29.980
a great scientist okay let's Let's address the

00:28:29.980 --> 00:28:33.420
most serious historical controversy, the LeMetre

00:28:33.420 --> 00:28:36.460
redaction issue. For many years, this cast a

00:28:36.460 --> 00:28:39.960
real shadow on Hubble's legacy. It did. For decades,

00:28:40.140 --> 00:28:42.319
there was this deep suspicion surrounding the

00:28:42.319 --> 00:28:44.700
English translation of George LeMetre's 1927

00:28:44.700 --> 00:28:47.740
paper. The original French paper included observational

00:28:47.740 --> 00:28:49.700
evidence supporting the expansion law, including

00:28:49.700 --> 00:28:52.180
his own calculated value for the expansion rate.

00:28:52.359 --> 00:28:54.079
But when the English translation was published

00:28:54.079 --> 00:28:57.039
in 1931, Those key paragraphs were missing. They

00:28:57.039 --> 00:29:00.019
were gone. And the immediate damning conclusion

00:29:00.019 --> 00:29:02.759
that many people drew was that Hubble, or someone

00:29:02.759 --> 00:29:05.059
close to him, must have redacted those sections

00:29:05.059 --> 00:29:07.220
to make sure he kept priority for Hubble's law,

00:29:07.359 --> 00:29:10.019
which he published in 1929. It seemed plausible,

00:29:10.240 --> 00:29:13.059
an attempt to rewrite scientific history in his

00:29:13.059 --> 00:29:16.440
favor. It did, because Lemaitre clearly had theoretical

00:29:16.440 --> 00:29:20.279
and arguably observational priority from 1927.

00:29:20.539 --> 00:29:22.700
If the content was suppressed, it would have

00:29:22.700 --> 00:29:26.240
been a major ethical breach. So how is this finally

00:29:26.240 --> 00:29:29.559
resolved? The resolution came in 2011, thanks

00:29:29.559 --> 00:29:32.559
to the astronomer Mario Lubio. He did some historical

00:29:32.559 --> 00:29:35.059
detective work and found a letter in the LaMetra

00:29:35.059 --> 00:29:37.220
archive that provided the definitive answer.

00:29:37.440 --> 00:29:39.220
And the person who requested the redaction was?

00:29:39.559 --> 00:29:42.180
LaMetra himself. Why on earth would he remove

00:29:42.180 --> 00:29:44.559
his own foundational data from the English translation?

00:29:45.049 --> 00:29:48.009
It was an act of humility and practicality. Lemaître

00:29:48.009 --> 00:29:50.289
felt that his specific observational data from

00:29:50.289 --> 00:29:53.390
1927 had already been superseded by Hubble's

00:29:53.390 --> 00:29:56.970
more extensive and robust data from 1929. He

00:29:56.970 --> 00:29:59.089
saw no reason to reproduce what he considered

00:29:59.089 --> 00:30:02.210
obsolete data in the 1931 translation, which

00:30:02.210 --> 00:30:04.029
he wanted to focus on the theoretical implications.

00:30:04.450 --> 00:30:07.069
So the letter completely cleared Hubble of that

00:30:07.069 --> 00:30:09.569
charge, although the fact of Lemaître's chronological

00:30:09.569 --> 00:30:12.309
priority is still undisputed. Moving on to another

00:30:12.309 --> 00:30:14.920
professional struggle. Hubble spent much of his

00:30:14.920 --> 00:30:17.380
later career chasing an honor that ultimately

00:30:17.380 --> 00:30:20.200
slipped through his fingers. The Nobel Prize.

00:30:20.539 --> 00:30:23.140
This was a determined campaign. At the time,

00:30:23.160 --> 00:30:25.019
the Nobel Committee didn't consider astronomy

00:30:25.019 --> 00:30:27.779
to be part of physics. They saw it more as a

00:30:27.779 --> 00:30:30.559
descriptive observational science. And Hubble

00:30:30.559 --> 00:30:33.440
argued against that. Vigorously. He and his colleagues

00:30:33.440 --> 00:30:35.869
argued that foundational work like... Proving

00:30:35.869 --> 00:30:38.170
the existence of other galaxies and charting

00:30:38.170 --> 00:30:41.210
the expansion of the universe was clearly fundamental

00:30:41.210 --> 00:30:44.089
physics. It was cosmology. The physics of the

00:30:44.089 --> 00:30:47.049
universe. Exactly. He lobbied tirelessly, writing

00:30:47.049 --> 00:30:49.470
letters, trying to change the rules. And the

00:30:49.470 --> 00:30:52.630
heartbreaking twist is that he succeeded, but

00:30:52.630 --> 00:30:55.150
too late. The timing is just tragic. The Nobel

00:30:55.150 --> 00:30:57.630
Committee eventually did decide that astronomical

00:30:57.630 --> 00:30:59.769
work would be eligible for the physics prize.

00:31:00.009 --> 00:31:02.529
But that ruling was enacted shortly after Hubble

00:31:02.529 --> 00:31:06.119
died in September 1953. And since the Nobel Prize

00:31:06.119 --> 00:31:09.000
cannot be awarded posthumously, he missed out

00:31:09.000 --> 00:31:10.960
on the recognition he had campaigned for and

00:31:10.960 --> 00:31:14.019
so fundamentally deserved. He broke the universe

00:31:14.019 --> 00:31:17.279
open for us, only to be deemed ineligible for

00:31:17.279 --> 00:31:19.380
the prize that celebrates exactly those kinds

00:31:19.380 --> 00:31:21.759
of breakthroughs. A truly poignant end to that

00:31:21.759 --> 00:31:23.940
part of his story. Despite the controversies

00:31:23.940 --> 00:31:26.700
and the missed Nobel. Hubble's publications made

00:31:26.700 --> 00:31:28.740
sure his methods and discoveries were codified

00:31:28.740 --> 00:31:31.339
for future generations. Oh, yes. His foundational

00:31:31.339 --> 00:31:34.660
books are still cornerstones of cosmology. You

00:31:34.660 --> 00:31:37.559
look at The Realm of the Nebulae from 1936 and

00:31:37.559 --> 00:31:40.359
The Observational Approach to Cosmology from

00:31:40.359 --> 00:31:43.460
1937. These books didn't just report his data.

00:31:43.579 --> 00:31:45.960
They laid out his entire empirical philosophy

00:31:45.960 --> 00:31:48.119
and standardized the way we classify galaxies.

00:31:48.460 --> 00:31:50.680
They laid the groundwork for everything that

00:31:50.680 --> 00:31:52.920
followed. And on a personal level, he married

00:31:52.920 --> 00:31:56.160
Grace Lillian Burke in 1920. just a few months

00:31:56.160 --> 00:31:59.220
before his monumental Andromeda discovery. Grace

00:31:59.220 --> 00:32:01.829
was central to his life. She managed his social

00:32:01.829 --> 00:32:04.609
profile and later was the fierce guardian of

00:32:04.609 --> 00:32:07.049
his intellectual legacy. We know his health began

00:32:07.049 --> 00:32:09.569
to decline in the late 1940s. He had a heart

00:32:09.569 --> 00:32:12.170
attack in 1949. He continued to work on a restricted

00:32:12.170 --> 00:32:14.589
schedule, but his health was precarious. He died

00:32:14.589 --> 00:32:17.490
from a blood clot in the brain, a cerebral thrombosis,

00:32:17.509 --> 00:32:21.210
on September 28, 1953. And this brings us to

00:32:21.210 --> 00:32:24.069
one of the most intriguing and mysterious final

00:32:24.069 --> 00:32:27.390
details of his life. A secret his wife kept until

00:32:27.390 --> 00:32:30.410
her own death decades later. Yes, the final mystery

00:32:30.410 --> 00:32:33.490
of Edwin Hubble. There was no public funeral

00:32:33.490 --> 00:32:37.069
service held for him. An even stranger, his wife,

00:32:37.250 --> 00:32:40.549
Grace, never revealed where he was buried. So

00:32:40.549 --> 00:32:42.890
no one knows. No one knows. She donated all his

00:32:42.890 --> 00:32:45.490
papers, his logbooks, his correspondence. But

00:32:45.490 --> 00:32:47.829
the location of his final resting place remains

00:32:47.829 --> 00:32:50.390
a complete mystery to this day. It's an almost

00:32:50.390 --> 00:32:53.009
mythical ending for a man who charted the boundaries

00:32:53.009 --> 00:32:56.410
of the cosmos. His own final location is one

00:32:56.410 --> 00:32:59.430
of the universe's small secrets. It is. But despite

00:32:59.430 --> 00:33:01.730
that personal secrecy, his professional legacy

00:33:01.730 --> 00:33:04.950
is spectacularly public. It's marked by so many

00:33:04.950 --> 00:33:07.230
enduring honors. The most famous, of course,

00:33:07.309 --> 00:33:09.089
is the Hubble Space Telescope. An instrument

00:33:09.089 --> 00:33:10.970
that continues his work, pushing the limits of

00:33:10.970 --> 00:33:13.049
observation far beyond what he could have ever

00:33:13.049 --> 00:33:15.450
dreamed of with the 100 -inch Hooker Telescope.

00:33:15.589 --> 00:33:17.809
But his name is also stamped all over the place.

00:33:18.630 --> 00:33:21.569
Asteroid 2069 Hubble, the Hubble Crater on the

00:33:21.569 --> 00:33:24.539
Moon, the Edwin Hubble Highway in Missouri. And

00:33:24.539 --> 00:33:26.880
his lifetime awards, including the ones for his

00:33:26.880 --> 00:33:30.039
wartime service, really highlight what a polymath

00:33:30.039 --> 00:33:33.180
he was. The Newcomb Cleveland Prize, the Bruce

00:33:33.180 --> 00:33:36.099
Medal, the Franklin Medal, the Gold Medal of

00:33:36.099 --> 00:33:38.680
the Royal Astronomical Society, and of course

00:33:38.680 --> 00:33:40.920
the Legion of Merit for his ballistics research.

00:33:41.200 --> 00:33:44.099
A stunning list of accomplishments. His story

00:33:44.099 --> 00:33:46.940
is now permanently woven into our popular understanding

00:33:46.940 --> 00:33:48.980
of science, perhaps most famously through Carl

00:33:48.980 --> 00:33:51.299
Sagan. Sagan made sure Hubble's legacy reached

00:33:51.299 --> 00:33:54.240
a massive audience. He featured him prominently

00:33:54.240 --> 00:33:57.359
in his 1980 documentary, Cosmos, in the episode

00:33:57.359 --> 00:34:00.299
about cosmic scale and time. He's truly crossed

00:34:00.299 --> 00:34:03.359
over from being a scientific giant to a cultural

00:34:03.359 --> 00:34:06.140
icon. So as we wrap up this deep dive, let's

00:34:06.140 --> 00:34:08.400
just reflect on the monumental scale of his impact.

00:34:08.989 --> 00:34:11.090
Hubble took humanity from thinking we lived on

00:34:11.090 --> 00:34:14.130
a single contained stellar island to realizing

00:34:14.130 --> 00:34:17.409
we inhabit one galaxy among billions all rushing

00:34:17.409 --> 00:34:19.349
apart from each other in an expanding universe.

00:34:19.550 --> 00:34:21.750
His career is really a testament to the power

00:34:21.750 --> 00:34:24.349
of meticulous observation over even the strongest

00:34:24.349 --> 00:34:26.869
theoretical beliefs. He said it best himself.

00:34:27.090 --> 00:34:29.900
He wrote. We do not know why we are born into

00:34:29.900 --> 00:34:32.239
the world, but we can try to find out what sort

00:34:32.239 --> 00:34:34.800
of a world it is, at least in its physical aspects.

00:34:35.280 --> 00:34:37.960
And that dedication to observation, to exhausting

00:34:37.960 --> 00:34:41.280
the empirical resources first, led him to conclude.

00:34:41.519 --> 00:34:43.659
Not until the empirical resources are exhausted

00:34:43.659 --> 00:34:46.440
need we pass on to the dreamy realms of speculation.

00:34:47.099 --> 00:34:49.800
And that, I think, perfectly frames our final

00:34:49.800 --> 00:34:52.300
thought for you, the listener. We've established

00:34:52.300 --> 00:34:55.320
that Hubble, the man who provided the data, remains

00:34:55.320 --> 00:34:57.400
skeptical of the expansion of the universe until

00:34:57.400 --> 00:35:00.119
the end. He preferred the idea that redshift

00:35:00.119 --> 00:35:03.000
might be a sign of some hitherto unrecognized

00:35:03.000 --> 00:35:06.340
principle of nature. Like tired light. Today,

00:35:06.400 --> 00:35:08.820
physics is far more confident in the metric expansion

00:35:08.820 --> 00:35:12.079
model. So our question is this. What are the

00:35:12.079 --> 00:35:14.519
modern empirical resources that conclusively

00:35:14.519 --> 00:35:17.699
prove the universe is truly expanding, eliminating

00:35:17.699 --> 00:35:20.500
all possibility for Hubble's original skepticism?

00:35:20.909 --> 00:35:23.030
What observations, things like the light curves

00:35:23.030 --> 00:35:25.969
of Type Ia supernovae at extreme distances, or

00:35:25.969 --> 00:35:28.369
the tiny temperature fluctuations in the cosmic

00:35:28.369 --> 00:35:30.690
microwave background, what observations provide

00:35:30.690 --> 00:35:33.389
that final, zero -room -for -doubt evidence that

00:35:33.389 --> 00:35:35.769
Hubble, the ultimate observer, would have required

00:35:35.769 --> 00:35:38.030
to finally change his mind? That is something

00:35:38.030 --> 00:35:38.630
worth exploring.
