Why auroras glow green, red and purple
Energetic particles make oxygen and nitrogen in the upper atmosphere emit light. The gas, its energy state and altitude help determine the...
SPACEEVEFrom the newsroom
Extraordinary worlds, surprising connections, and the science behind them.
Energetic particles make oxygen and nitrogen in the upper atmosphere emit light. The gas, its energy state and altitude help determine the...
Moonlight reaches us about 1.3 seconds after leaving the Moon; Andromeda’s light takes roughly 2.5 million years. The same finite speed connects...
Earth turns once relative to distant stars in about 23 hours 56 minutes. Its journey around the Sun explains why the familiar...
The Sun emits a broad mixture of visible wavelengths that our eyes perceive as white. Air, camera settings and scientific image processing...
Saturn keeps its rings when they turn edge-on to Earth. Their changing appearance follows the geometry of a tilted planet, a thin...
Earth’s orbit gives astronomers changing viewpoints on the stars. Measuring the resulting apparent shift turns a small angle into a distance, provided...
Moving air distorts arriving starlight. A planet’s larger apparent disk helps average out brightness changes, while stars near the horizon face a...
An 84-year orbit sets the pace of Uranus’s seasons. Its nearly sideways spin axis makes the poles alternate between prolonged daylight and...
Earth’s gravity remains strong at space-station height. Shared free fall, sideways motion and the absence of a supporting floor explain why astronauts...
The Moon keeps roughly the same face toward Earth, but its daylight follows the Sun. Rotation and changing illumination explain the difference.
A broad dust tail and a straighter ion tail respond differently to the Sun, so they can spread across the sky in...
Mass, distance and an object’s motion matter. A black hole’s event horizon marks the boundary from which even light cannot escape.
Drag to orbit · Arrow keys to rotate · Escape to return