How Tides Work

Updated June 2026
Tides are the regular rise and fall of sea level caused by the gravitational attraction of the Moon and Sun acting on Earth's ocean. These predictable water level changes occur in cycles ranging from twice daily to monthly, creating dynamic coastal environments and driving powerful currents through narrow waterways.

The Gravitational Foundation of Tides

Tides arise from the differential gravitational pull exerted by the Moon and Sun across Earth's diameter. The side of Earth facing the Moon experiences slightly stronger gravitational attraction than Earth's center, while the far side experiences slightly weaker attraction. This difference creates two tidal bulges: one facing the Moon (direct tide) and one on the opposite side (antipodal tide). As Earth rotates through these bulges every 24 hours and 50 minutes, most locations experience two high tides and two low tides daily.

The Moon dominates tidal forcing because gravitational tidal force depends on the cube of distance, not just mass divided by distance squared. Despite the Sun being 27 million times more massive than the Moon, it is 389 times farther away. The net result is that lunar tidal force is approximately 2.2 times stronger than solar tidal force. This ratio explains why tides follow lunar timing (shifting roughly 50 minutes later each day) rather than solar timing.

Spring tides occur during new and full moon phases when the Sun, Moon, and Earth align, combining their tidal forces. Neap tides occur during quarter moon phases when solar and lunar tidal forces partially cancel each other, producing smaller tidal ranges. The spring-neap cycle repeats every 14.8 days, creating a predictable fortnightly variation in tidal amplitude superimposed on the daily high-low cycle.

Tidal Patterns Around the World

Three tidal patterns exist globally: semidiurnal (two roughly equal highs and lows per day), diurnal (one high and one low per day), and mixed (two unequal highs and lows per day). The dominant pattern at any location depends on the geometry of the ocean basin, the latitude, and the natural resonance frequencies of connected bodies of water. Most Atlantic coastlines experience semidiurnal tides, while parts of the Gulf of Mexico and Southeast Asia experience diurnal tides. The Pacific coast of North America experiences mixed tides.

Tidal ranges vary enormously by location. In the open ocean, tidal range rarely exceeds 1 meter. But coastal geometry can amplify tides through funneling, shoaling, and resonance effects. The Bay of Fundy holds the world record with tidal ranges reaching 16.3 meters, because its natural resonance period (approximately 13 hours) closely matches the semidiurnal tidal period (12.42 hours). This near-resonance amplifies the incoming tidal wave like pushing a child on a swing at exactly the right moment.

Amphidromic points are locations in the ocean where tidal range is essentially zero, with tidal waves rotating around them like the hand of a clock. Each ocean basin contains several amphidromic points, and tidal range generally increases with distance from these points. The co-tidal lines radiating from amphidromic points show how the tidal wave propagates across the basin, typically rotating counterclockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere due to the Coriolis effect.

Tidal Currents and Energy

As tides rise and fall, water must flow horizontally to fill and drain coastal areas, creating tidal currents. In narrow channels, straits, and estuary mouths, tidal currents can reach speeds of 5 meters per second or more. These currents reverse direction with each tide change, creating a predictable cycle of flood (incoming) and ebb (outgoing) flows. The brief period of no flow between directions is called slack water.

Tidal bores occur in certain funnel-shaped estuaries where incoming tides form a wall of water that travels upstream against the river current. Famous tidal bores include the Severn Bore in England, the Qiantang River bore in China (reaching heights of 9 meters), and the Pororoca on the Amazon. These occur when tidal range is large, the estuary narrows significantly upstream, and the river is relatively shallow.

Tidal energy represents a predictable renewable energy source, unlike solar or wind power. Tidal barrage systems (like the Rance facility in France, operational since 1966) trap water behind dams and release it through turbines. Newer tidal stream generators work like underwater wind turbines, extracting energy from tidal currents without dams. Global tidal energy potential is estimated at 1 terawatt, though practical extraction is limited to sites with exceptional tidal ranges or current speeds.

Tides and Coastal Ecosystems

The intertidal zone, the area between high and low tide marks, represents one of Earth's most physically demanding habitats. Organisms here must tolerate regular exposure to air, temperature extremes, wave impact, and desiccation, followed by complete submersion in cold seawater. This creates distinct vertical zonation bands where different species dominate at different tidal heights based on their tolerance to exposure.

Tidal flats, extensive low-gradient areas exposed at low tide, serve as critical feeding grounds for migratory shorebirds that depend on the invertebrates living in tidal sediments. The Wadden Sea in the North Sea and the Yellow Sea tidal flats along the East Asian-Australasian Flyway support millions of migrating birds annually. Loss of tidal flat habitat through coastal development directly threatens these migratory populations.

Key Takeaway

Tides are predictable, gravitationally driven water level changes that create unique ecosystems in the intertidal zone and represent an untapped source of renewable energy, with their strength determined by lunar-solar geometry and coastal topography.