Starts With A Bang

A field of stars and colorful cosmic dust clouds scattered across the dark expanse of space.
The Universe is out there, waiting to be discovered

Our mission is to answer the biggest questions of all, scientifically.

What is the Universe made of? How did it become the way it is today? Where did everything come from? What is the ultimate fate of the cosmos?

For most of human history, these questions had no clear answers. Today, they do. Starts With a Bang, written by Dr. Ethan Siegel, explores what we know about the universe and how we came to know it, bringing the latest discoveries in cosmology and astrophysics directly to you.

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Ethan Siegel is an award-winning PhD astrophysicist and the author of four books, including The Grand Cosmic Story, published by National Geographic.

Full Profile
A bald man with a long beard and handlebar mustache gestures with his hands against a backdrop of an upside-down cityscape wearing a purple shirt.
A brief history of the cosmic distance record
Only nearby objects appear to the naked eye. With telescopes of all types, especially in space, we've smashed those records many times over.

Ethan Siegel

A dense star field and distant galaxies with bright galaxy clusters and several white squares highlighting specific points in the image.
A detailed view of Neptune’s largest moon, Triton, showing its icy surface with light and dark regions, photographed against a black background.
Triton is Neptune's largest moon today, but it was once the undisputed king of the Kuiper belt. Here's why the outer solar system matters.
A deep space image showing numerous distant galaxies of various shapes and sizes scattered across a dark background, revealing just how empty is space between these cosmic islands.
There's a lot of room in interplanetary, interstellar, and intergalactic space, but just how low the densities go is truly mind-boggling.
two particles different wavelength speed of light
Contrary to common experience, not everything needs a medium to travel through. Overcoming that assumption removes the need for an aether.
Two people examine scientific equipment in a laboratory, working on a large metallic device surrounded by cables and tools, as they investigate the physics mystery G—the elusive mystery gravitational constant.
Newton's gravitational constant, G, is still known to just 3 significant figures in 2026. New measurements merely highlight our uncertainty.
pluto moons hubble
In 2006, the IAU defined "planet" for the first time, excluding Pluto and all other dwarf planets. In 2026, is it now time for a change?
A vibrant cosmic scene reveals a galaxy with bright jets of energy, hottest stars twinkling vividly amidst scattered stars against a dark backdrop.
From within our own galaxy to behemoths billions of light-years away, supermassive black holes create jets like nothing else in the cosmos.
A colored pixelated grid with rectangular outlines; a legend in the top right labels blue as F115W, green as F200W, and red as F277W—capturing data from the JWST to record a distant galaxy.
It takes incredible energies to accelerate masses near the speed of light. So how do the farthest galaxies speed away from us so quickly?
A color-enhanced image shows Pluto planet in the foreground with its moon Charon in the background, both set against a black space backdrop.
In 2006, Pluto was controversially demoted to "dwarf planet" by the IAU. Unless you ignore most of astrophysics, it won't ever be one again.
Bullet Cluster separation mass gravity x-ray lensing
The first colliding galaxy cluster to reveal dark matter, empirically, turns 20 this year. Here's why it cements dark matter's existence.
A person with hair floating upwards looks out of a spacecraft window at Earth, filled with hope as clouds and oceans shimmer below—a view reminiscent of the Artemis II mission’s journey.
NASA has just sent astronauts back to the Moon for the first time since 1972 with Artemis II. So why would we cut NASA and NSF science now?
Chart illustrating the Standard Model of Elementary Particles, as found in the early universe, divided into quarks, leptons, gauge bosons, and the Higgs boson, with details on mass, charge, and generation.
Today, we have the Standard Model of particles with four fundamental forces governing them. But things weren't always the way they are now.
A colorful nebula with a bright center and symmetrical, wing-like clouds of gas and dust extends outward in space, as seen in a JWST reveal that uncovers stars and galaxies in the universe beyond.
Many facts are well-known to professionals, but are unappreciated or even rejected outright by the public. "How stars work" takes the cake.
universe bulk volume brane dimension
For decades, theorists have been cooking up "theories of everything" to explain our Universe. Are all of them completely off-track?
Antimatter rocket with a glowing blue exhaust travels through deep space, showcasing the marvels of interstellar travel amid distant galaxies and stars.
Our dream of journeying to other star systems has a big obstacle to overcome: the vast interstellar distances. Can antimatter get us there?
Image of a galaxy cluster with bright yellow galaxies at the center, surrounded by blue regions representing dark matter in deep space—a striking view often used for dark matter cosmic test MOND studies.
On cosmic scales, only dark matter (or something equivalent) gives us the Universe we observe. Now, the Sunyaev-Zel'dovich effect agrees.
Colorful nebula with bright stars ignite glowing gas clouds in space, featuring red, yellow, and blue hues against a dark background.
Although a star's "birth" is well-defined, it doesn't correspond to an ignition event in its core. Here's how stars are actually born.
protoplanetary disk
Every time a new star forms, there's an opportunity to form planets alongside and around it. How does it happen, and how long does it take?
An Ishihara color blindness test with colored dots, showing letters “u” and “d” in black, and a magnified section highlighting the dot pattern—inviting viewers to observe proton decay through subtle visual cues.
"Color" with respect to the strong force is just an analogy. Here's how to understand it without colors, group theory, or any advanced math.
A hexagonal storm formation with a dark central vortex on a planet’s surface, showing swirling blue and tan cloud patterns.
From 2004 through 2017, Saturn was imaged many times and from many angles up close by Cassini. This new viral image isn't real; it's AI.
A bright, circular object with concentric rings and a surrounding halo set against a dark background, resembling a gap-clearing planet or other astronomical phenomena.
One parameter, alone, sets the dividing line between rocky planets, gas giants, brown dwarfs, stars, and much more. Here's why mass matters.