How the Sun will become a white dwarf
After its giant phases, the Sun will leave a dense, cooling core. Fusion, mass loss and quantum pressure explain how a familiar...
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Extraordinary worlds, surprising connections, and the science behind them.
After its giant phases, the Sun will leave a dense, cooling core. Fusion, mass loss and quantum pressure explain how a familiar...
A rising Moon can look enormous without growing wider in a fixed-zoom photograph. Perception, atmospheric effects and orbital distance each play different...
Oxidized iron minerals colour fine dust that coats and circulates around Mars. Rover samples reveal a more varied planet beneath that familiar...
Earth's weather and shifting crust erase or bury many impact scars. The Moon preserves a longer record, although new impacts and moving...
We live inside the Milky Way's stellar disk. Looking along that crowded plane produces a hazy band, while interstellar dust hides parts...
Sunlit ground can reach about 430 degrees Celsius, but some polar crater floors never receive direct sunlight. MESSENGER's measurements reveal why local...
Warm telescope hardware emits infrared light of its own. Webb’s layered sunshield limits that background, while MIRI needs additional refrigeration to observe...
Earth blocks direct sunlight during a total lunar eclipse, but its atmosphere bends and filters a little light into the shadow. That...
Jupiter’s rapid rotation helps make it about 7% wider across the equator than from pole to pole. Radio measurements reveal how its...
Particles in a meteor stream arrive along nearly parallel paths. Perspective makes their trails appear to spread from a shared region of...
Laser measurements reveal that the Moon’s mean distance grows by about 3.8 centimetres a year. Tidal interactions transfer angular momentum from Earth’s...
A rocket accelerates its own exhaust, producing a force on the vehicle in the opposite direction. Chemical engines also carry the ingredients...
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