Start here · Essential guide
How Stars Are Born, Live and Die
Follow a star from a cold gas cloud through fusion, red giant and supernova stages to a white dwarf, neutron star or black hole, and why mass decides its fate.
Universe and Matter
How stars live and die and how galaxies and the early universe are understood.
Start here · Essential guide
Follow a star from a cold gas cloud through fusion, red giant and supernova stages to a white dwarf, neutron star or black hole, and why mass decides its fate.
See how parallax, Cepheid variables and supernovae form a ladder of methods that lets astronomers measure distances from nearby stars to far-off galaxies.
What the Big Bang model says about an expanding, cooling universe, the main evidence behind it, and the common misunderstandings about an explosion and a center.
Learn how a collapsed stellar core becomes a city-sized neutron star, why some of them sweep beams of radio waves past Earth, and what pulsars reveal.
Explore the shape, size and contents of the Milky Way, from its central bar and spiral arms to its halo, and find out where the Sun sits within it.
A black hole is a region where gravity lets nothing escape. Learn how they form and the evidence from stellar orbits, X-rays, gravitational waves and images.
A light year is the distance light travels in one year, about 9.46 trillion kilometers. Learn why it measures distance, not time, and how it helps us gauge space.
Dark matter is the unseen mass astronomers infer from galaxy rotation, gravitational lensing and the early universe. Learn the evidence and what is still unknown.
Stars twinkle because turbulent air bends their light as it passes through the atmosphere. Learn why planets shine more steadily and why stars in space do not twinkle.
Earth's yearly orbit changes which stars face our night side, so Orion rules winter evenings and Scorpius summer ones. See how it works and why some stars never leave.
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