
- Extremely high tides push seawater into estuaries and upriver, forcing rivers to flow backward and depositing salt into surface and groundwater systems, which contaminates freshwater supplies.@science· Earth
Extremely high tides push seawater into estuaries and upriver, forcing rivers to flow backward and depositing salt into surface and groundwater systems, which contaminates freshwater supplies.
- Volcanic aerosols lofted into the stratosphere reflect incoming sunlight and chemically alter the atmosphere, which reduces surface heating and causes acid deposition and disrupted precipitation patterns that harm ecosystems.@science· Earth
Volcanic aerosols lofted into the stratosphere reflect incoming sunlight and chemically alter the atmosphere, which reduces surface heating and causes acid deposition and disrupted precipitation patterns that harm ecosystems.
- Large amounts of moondust raining through the atmosphere would convert kinetic energy into heat—potentially heating and even boiling surface waters—while persistent ring shadows and volcanic/meteoric aerosols would reflect sunlight and trigger rapid cooling, so the net climate effect depends on the balance and timing of heating versus sunlight blockage.@science· Earth
Large amounts of moondust raining through the atmosphere would convert kinetic energy into heat—potentially heating and even boiling surface waters—while persistent ring shadows and volcanic/meteoric aerosols would reflect sunlight and trigger rapid cooling, so the net climate effect depends on the balance and timing of heating versus sunlight blockage.
- If the Moon disintegrated into a diffuse ring or debris its concentrated gravitational pull would vanish, greatly reducing tidal forcing so previously extreme tides would subside and ocean water near coasts would withdraw.@science· Earth
If the Moon disintegrated into a diffuse ring or debris its concentrated gravitational pull would vanish, greatly reducing tidal forcing so previously extreme tides would subside and ocean water near coasts would withdraw.
- When the Moon crosses Earth’s Roche limit differential tidal forces exceed the Moon’s self‑gravity, tearing it into rubble that spreads out to form an orbital ring.@science· Earth
When the Moon crosses Earth’s Roche limit differential tidal forces exceed the Moon’s self‑gravity, tearing it into rubble that spreads out to form an orbital ring.
- As Earth’s gravity grows on the approaching Moon it creates a tidal gradient that stretches the near side into a slight egg shape and flexes lunar rock, and that repeated flexing produces deep moonquakes.@science· Earth
As Earth’s gravity grows on the approaching Moon it creates a tidal gradient that stretches the near side into a slight egg shape and flexes lunar rock, and that repeated flexing produces deep moonquakes.
- Even with the Moon directly overhead Earth’s surface gravity is several times stronger than the Moon’s local pull, so the net gravitational force still keeps you anchored to the ground.@science· Earth
Even with the Moon directly overhead Earth’s surface gravity is several times stronger than the Moon’s local pull, so the net gravitational force still keeps you anchored to the ground.
- If the Moon orbited once every 24 hours it would appear fixed over one longitude, and that steady alignment would create a persistent tidal bulge at that longitude instead of the normal twice‑daily tides.@science· Earth
If the Moon orbited once every 24 hours it would appear fixed over one longitude, and that steady alignment would create a persistent tidal bulge at that longitude instead of the normal twice‑daily tides.
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