Why Do We Have Seasons?
Seasons result mainly from Earth's axial tilt, which changes sunlight angle and day length in each hemisphere during the yearly orbit.
Explore fascinating ideas from science, mathematics, space, technology, history, and the world around us.
Seasons result mainly from Earth's axial tilt, which changes sunlight angle and day length in each hemisphere during the yearly orbit.
Earth is about 4.54 billion years old, determined mainly through radiometric dating of meteorites and the oldest Earth and Moon materials.
Ecosystems change continuously as organisms use energy, cycle nutrients, compete, cooperate, migrate, and respond to disturbance.
Magma rises because it can be less dense than surrounding rock while expanding gases build pressure; viscosity and gas strongly affect eruption style.
Earth's plates move, magnetic poles wander, Antarctica is a desert, the deepest ocean exceeds Everest's height, and most freshwater is locked in ice or underground.
A day on Venus is longer than a year on Venus.
Understand the forces, discoveries, and ideas shaping our universe.
Magma rises because it can be less dense than surrounding rock while expanding gases build pressure; viscosity and gas strongly affect eruption style.
Beyond a black hole's event horizon, general relativity says every future-directed path leads inward; the predicted singularity signals that present theories are incomplete.
Vaccines safely present an antigen or its instructions so immune cells can build memory and respond faster during a later encounter.
Discover the patterns and ideas hidden behind everyday life.
Probability quantifies uncertainty and helps reason about forecasts, risk, games, medicine, queues, and repeated events.
Prime numbers have exactly two positive divisors and act as the multiplicative building blocks of whole numbers, with important uses in number theory and cryptography.
Pi is the constant ratio of a Euclidean circle's circumference to its diameter and appears wherever circular symmetry or periodic behavior occurs.
Travel from the Moon and Mars to distant stars and black holes.
Exoplanets orbit stars beyond the Sun and are usually detected through transits, stellar motion, or direct imaging rather than by unaided sight.
The Moon is always half illuminated by the Sun; phases occur because its orbit lets us see changing fractions of that sunlit half.
Interstellar travel is consistent with known physics but extraordinarily difficult because even the nearest stars are several light-years away.
Explore AI, the internet, robotics, GPS, and quantum computing.
Robots combine cameras, lidar, radar, ultrasound, touch, and algorithms to estimate objects, depth, movement, and location.
A GPS receiver compares precisely timed signals from multiple satellites to solve for three-dimensional position and clock error.
Quantum computers manipulate qubits using superposition, interference, and entanglement to accelerate selected algorithms.