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Jennifer Marohasy's avatar

I've received some requests that I provide more background information, even how the Moon causes two sea tides in each day.

1.Why Two High Tides?

The Moon’s gravity pulls the ocean toward it, creating a bulge of water on the side of Earth facing the Moon. At the same time, on the opposite side, water "lags" due to inertia (Earth is pulled toward the Moon more than the water on the far side), forming a second bulge. As Earth rotates daily, any point on its surface passes through both bulges, giving you two high tides about 12 hours apart. This is why we see two highs even though the Moon only orbits once.

2. How the Sun Complicates Things

The Sun also exerts gravitational pull on Earth’s oceans, but it’s weaker than the Moon’s because the Sun is much farther away (its tidal force is about 46% of the Moon’s). The Sun’s effect combines with the Moon’s, leading to variations in tide strength:

Spring Tides: When the Sun, Moon, and Earth align (during full or new moons), their gravitational pulls reinforce each other, causing higher high tides and lower low tides. These occur roughly every 14–15 days.

3. Neap Tides: When the Sun and Moon are at right angles (first or third quarter moons), their pulls partially cancel out, leading to smaller tidal ranges (less extreme highs and lows). These also happen about every 14–15 days. The Sun’s influence modulates the tides’ amplitude but doesn’t change the twice-daily pattern driven by the Moon and Earth’s rotation.

4. The Lunar Declination Cycle

The Moon’s orbit isn’t perfectly aligned with Earth’s equator—it’s tilted, and its position relative to the equator (called declination) shifts over a 27.3-day cycle. This affects tides because the Moon’s gravitational pull varies in strength depending on whether it’s overhead at the equator, north, or south of it:

When the Moon is near the equator (declination near 0°), the two daily high tides at a given location tend to be similar in height because the tidal bulges are symmetrically aligned with Earth’s rotation.

When the Moon is at maximum declination (up to ±28.5° north or south), one tidal bulge is stronger in the hemisphere where the Moon is overhead, leading to diurnal inequality—the two daily high tides can differ significantly in height, especially at higher latitudes. For example, one high tide might be much higher than the other in places like the Gulf of Mexico.

This cycle repeats every 27.3 days, causing subtle shifts in tidal patterns that are more noticeable in certain coastal areas.

Putting It Together

The two high tides per day come from Earth passing through the Moon’s two tidal bulges as it rotates. The Sun amplifies or dampens these tides based on its alignment with the Moon, creating spring and neap tides. Meanwhile, the Moon’s declination cycle tweaks the relative heights of the two daily tides as its position shifts north or south. Local geography, like bays or channels, can further shape how these forces play out at the specific location of interest.

It is complicated and fascinating, and important stuff if we are to understand natural cycles, including weather and climate cycles. It all begins here.

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Howard Dewhirst's avatar

Yet another CO2 free contributor to climate change.

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