From our own perspective on Earth, we’ve identified the presence of spiral arms.
By viewing the Milky Way in infrared wavelengths of light, we can see through the galactic dust and view the distribution of stars and star-forming regions behind them. As revealed by the 2 micron all-sky survey (2MASS), the densest collections of galactic dust can be seen tracing out our spiral arms. (Credit: 2MASS/IPAC/Caltech & UMass)
However, being stuck within the Milky Way itself, we exclusively view it edge-on.
The European Space Agency’s space-based Gaia mission has mapped out the three-dimensional positions and locations of more than one billion stars in our Milky Way galaxy: the most of all-time. Looking toward the center of the Milky Way, Gaia reveals both light-blocking and luminous features that are scientifically and visually fascinating. (Credit: ESA/Gaia/DPAC)
Even our best spaceborne views leave much ambiguity in our galaxy’s overall structure.
Quantum gravity attempts to combine Einstein’s general theory of relativity with quantum mechanics. Quantum corrections to classical gravity are visualized as loop diagrams, as the one shown here in white. Alternatively, it’s possible that gravity is always classical and continuous, and that quantum field theory, not general relativity, needs to be modified. A fundamental incompatibility between quantum physics and General Relativity has long been recognized, but has yet to be satisfactorily resolved. (Credit: SLAC National Accelerator Laboratory)
Electromagnetism, both nuclear forces, and even the Higgs force are mediated by known bosons. What about gravity? Does it require gravitons?
If you examine the Universe extremely closely, by probing the fundamental entities with it on the smallest possible scales, you’ll discover that reality is fundamentally quantum in nature. Matter itself is made up of indivisible, uncuttable quantum entities: particles like quarks, leptons, and bosons. These quanta have charges (color charge, electric charge, weak isospin and weak hypercharge, and “mass/energy” as a gravitational charge), and it’s the exchange of quanta between these charged particles (gluons, photons, W-and-Z bosons, etc.) that mediate these forces. There’s even a Higgs force as well.
However, one type of quantum that’s never been detected is the graviton: the theoretical particle that mediates the gravitational force. Even though it’s predicted to exist (and to have a spin of 2, unique among all particles) and, just like light is composed of photons, gravitational waves should be composed of gravitons, those predictions rely on an unproven assumption: that gravity is fundamentally a quantum force in nature. Is that assumption necessarily true? It isn’t in Einstein’s General Relativity, and that prompted…
The excellent popular science book, Waves in an Impossible Sea: How everyday life emerges from the cosmic ocean, written by Matt Strassler (left), has been selected as Starts With A Bang’s best science book of 2024. (Credit: Matt Strassler)
Matt Strassler’s journey into fundamental physics culminates in a brilliant explanation of the Higgs field. Enjoy this exclusive interview.
It’s rare that a book comes along that changes the way experts in their field think about the fundamentals, while simultaneously being accessible and informative to those without expert knowledge themselves. That’s why, as 2024 winds down, it’s a no-brainer selection to choose Matt Strassler’s incomparable new book, Waves in an Impossible Sea: How everyday life emerges from the cosmic ocean, as this year’s best science book. (Yes, even in a year where I myself wrote my own book!) Strassler, a world-renowned expert in particle physics in his own right (and longtime science blogger), takes the reader on a whirlwind tour of physics from a conceptual point of view.
Even classic topics such as Galileo’s relativity and Newtonian gravity are presented in novel, accessible ways, with common historical terms like “Newton’s first law” replaced by the more intuitive ones such as the “coasting law.” Strassler takes the reader on similar journeys through other classical topics such as mass, waves, and fields before entering the more unfamiliar world of the quantum, which suddenly seems more…
The Google Willow chip is the first quantum chip to have more than 100 qubits, with 105 qubits to it. Its most significant advance is in quantum error-correction, but contrary to claims made by the founder and lead of Google Quantum AI, it has nothing at all to do with parallel universes. (Credit: Google/Hartmut Neven)
By improving quantum error correction, quantum computations are now faster than ever. But parallel universes? That’s utter nonsense here.
Quantum computation is, simultaneously, a remarkable scientific achievement with the potential to solve an array of problems that currently are wholly impractical to solve, and also a breathless source of wild, untrue claims that completely defy reality. In 2021, there were claims that Google’s quantum computing team developed a time crystal that violated the laws of thermodynamics. (The first part is true, the second is not.) In late 2022, a team claimed to demonstrate the existence of wormholes using a quantum computer, which was incorrect across the board. And now, here in 2024, Google has introduced a new quantum chip, Willow, that the founder and lead of Google’s Quantum AI states proves the existence of parallel universes.
Do you sense a pattern here? Are you a little suspicious of such a wild claim? Well, you should be. Whitney Clavin certainly is, as she wrote to me to ask:
“Have you seen all this crazy talk about Google’s quantum computing breakthrough providing evidence for the multiverse?! Google said this! I think you need to write a story…
Traditionally, atoms are viewed as dense nuclei, a mix of protons and neutrons, surrounded by electrons that move in specific orbital paths. This picture is useful in some circumstances, but the full suite of quantum information encoded in an atom is much richer than this. (Credit: Annelisa Leinbach, Thomas Wright)
If atoms are mostly empty space, then why can’t two objects made of atoms simply pass through each other? Quantum physics explains why.
Here on planet Earth, as well as in most locations in the Universe, everything we observe and interact with is made up of atoms. Atoms come in roughly 90 different naturally occurring species, where all atoms of the same species share similar physical and chemical properties, but that differ tremendously from one species to another. Once thought to be indivisible units of matter, we now know that atoms themselves have an internal structure, with a tiny, positively charged, massive nucleus consisting of protons and neutrons surrounded by negatively charged, much less massive electrons. We’ve measured the physical sizes of these subatomic constituents exquisitely well, and one fact stands out: the size of atoms, at around 10^-10 meters apiece, are much, much larger than the constituent parts that compose them.
Protons and neutrons, which compose the atom’s nucleus, are roughly a factor of 100,000 smaller in length, with a typical size of only around 10^-15 meters. Electrons are even smaller, and are assumed to be point-like particles in the sense that they exhibit no measurable size at all, with experiments…
This illustration of our Milky Way shows an ancient galactic stream wrapped around our galaxy’s plane at nearly a 90 degree angle: evidence for a recent and even ongoing merger in our galaxy’s history. (Credit: NASA/JPL-Caltech/R. Hurt (SSC/Caltech))
Even with just a momentary view of our galaxy right now, the data we collect enables us to reconstruct so much of our past history.
When we look out at our home galaxy, the Milky Way, we have to recognize that even though it’s been growing and evolving for 13.8 billion years, we’re only observing it as it is right now: a snapshot in time determined by the light that’s arriving in our instruments right now. However, just like we’re living “right now” in human history but can, through the science of archaeology, learn about historical events that happened many thousands of years ago (before recorded history) or even earlier, we can learn about the Milky Way’s history through the astronomical equivalent: galactic archaeology.
Observation of the red supergiant star, Betelgeuse, revealed a vast plume of gas almost as large as our Solar System and a gigantic bubble boiling on its surface. In 2019–2020, a great plume of material erupted from Betelgeuse. A recent brightening event in 2023 suggested that a supernova might be imminent, so what will we see when it finally happens? (Credit: ESO/L. Calçada)
The closest known star that will soon undergo a core-collapse supernova is Betelgeuse, just 640 light-years away. Here’s what we’ll observe.
The stars in the night sky, as we typically perceive them, are normally static and unchanging to our eyes. Sure, there are variable stars that brighten and fainten, but most of those do so periodically and regularly, with only a few exceptions. One of the most prominent exceptions is Betelgeuse, the red supergiant that makes up one of the “shoulders” of the constellation Orion. Over the past five years, not only has it been fluctuating in brightness, but its dimming in late 2019 and early 2020, followed by a strange brightening in 2023, indicates variation in a fashion never before witnessed by living humans.
The Sombrero galaxy, commonly viewed in optical light (as shown at bottom, via Hubble), displays a vastly different set of featured in mid-infrared light (by JWST, top). At last, we’ve seen beneath the Sombrero’s hat, and can paint a coherent picture of this brilliant object. (Credit: NASA, ESA, CSA, STScI, Hubble Heritage Team (STScI/AURA))
The Sombrero is the closest bright, massive, edge-on galaxy to us. JWST’s new image, taken with MIRI, finally shows what’s under its hat.
Since its discovery nearly 250 years ago, the Sombrero galaxy has delighted astronomers.
This image of the Sombrero galaxy, also known as Messier 104, represents what an amateur astronomer can capture with a modest, modern setup, revealing a bright, dusty halo of shining stars with a prominent dust lane crossing the center. (Credit: Carsten Frenzl/flickr)
It appears nearly edge-on, inclined at a mere 6°.
This wide-field view of the Sombrero galaxy shows a 1.5° region of the sky, with two asterisms (or collections of bright stars) nearby: four stars in a hockey-stick configuration (jaws) just to the right of the galaxy, and the tetrahedron-like “stargate” at the lower-right. (Credit: Pat Freeman)
The Sombrero galaxy, shown in visible light and imaged by Hubble, is intrinsically the brightest galaxy within some ~35 million light-years of our Milky Way. One must look to the Virgo Cluster, some 50+ million light-years distant, to find significantly brighter, much more massive galaxies. (Credit: NASA/ESA and The Hubble Heritage Team (STScI/AURA))
This view of the Sombrero galaxy comes from NASA’s Spitzer telescope, showing the inner part of the disk in near-infrared light, while hydrogen glows in red in the mid-infrared in an outer ring. This dual-nature galaxy has its disk-like component better revealed by infrared views. (Credit: NASA/JPL-Caltech/University of Arizona/STScI)
Prominent dust lanes and spiral arms line a central disk.
Each s orbital (red), each of the p orbitals (yellow), the d orbitals (blue) and the f orbitals (green) can contain only two electrons apiece: one spin up and one spin down in each one. The effects of spin, of moving close to the speed of light, and of the inherently fluctuating nature of the quantum fields that permeate the Universe are all responsible for the fine structure that matter exhibits. (Credit: LibreTexts Library/UC Davis)
One of the fundamental constants of nature, the fine-structure constant, determines so much about our Universe. Here’s why it matters.
There’s an enormous existential question that we’ve wondered about ever since we first realized that the Universe does, in fact, obey physical laws at all: why is our Universe the precise way it is, rather than any other way we could’ve imagined? There are only three things that make it so:
the laws of nature themselves,
the fundamental constants governing reality,
and the initial conditions that our Universe was born with.
If our Universe had different laws of nature, then all bets would be off; the cosmos would have been vastly different in almost any way you can fathom. Protons might decay, fundamental quantities like particle masses might not be constant, and the strengths of any fundamental forces might joltingly change at any moment.
If only the initial conditions of our Universe were different, the way the cosmic story unfolded would be the same in terms of broad strokes, but the details would differ between that hypothetical Universe and our own. But for the fundamental constants, some changes would be…
While the web of dark matter (purple, left) might seem to determine cosmic structure formation on its own, the feedback from normal matter (red, at right) can severely impact the formation of structure on galactic and smaller scales. Both dark matter and normal matter, in the right ratios, are required to explain the Universe as we observe it, with dark energy needed to explain how the expansion rate has evolved over time. Structure formation is hierarchical within the Universe, with small star clusters forming first, early protogalaxies and galaxies forming next, followed by galaxy groups and clusters, and lastly by the large-scale cosmic web. (Credit: Illustris Collaboration/Illustris Simulation)
Two parts of our Universe that seem to be unavoidable are dark matter and dark energy. Could they really be two aspects of the same thing?
When it comes to the Universe, what you can easily see isn’t always reflective of all there is. It’s one of the important reasons why theories and observations/measurements need to go hand-in-hand: observations tell you what’s there to the best of our measurement capabilities, and theory allows us to compare what we’d expect to occur versus what’s actually seen. When they match up, that’s generally an indication that we have a pretty good understanding of what’s actually going on. But when they don’t, that’s a sign that one of two things is occurring:
either the theoretical rules we’re applying aren’t quite right for this situation,
or there are additional ingredients out there that our observations haven’t directly revealed.
Many of the biggest mismatches in the Universe — between what we observe and what we would have expected based solely on what we see — point to two additional ingredients: dark matter and dark energy. But these two seemingly unrelated phenomena have something deeply disconcerting in common: they’ve only ever been detected…