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At its heart, the theory suggests that:
• A massive star once passed very close to our Sun.
• The gravitational pull from this passing star created huge tidal waves (just like the
Moon affects tides on Earth, but much more powerful).
• These tidal waves pulled large streams of hot gas out of the Sun.
• This ejected matter eventually cooled down, condensed, and formed the planets,
including Earth.
• It was a catastrophic theory—meaning it depended on a rare, violent event rather
than a slow, natural process.
Key Concepts in the Tidal Hypothesis
To understand this theory better, let’s look at its main components step-by-step:
1. Close Encounter of a Passing Star
The hypothesis begins with a wandering, massive star coming close to the Sun. This is a one-
time cosmic accident, not a regular event. The gravitational field of the star distorts the
Sun's shape and causes powerful tides.
2. Gravitational Tides on the Sun
Just as the Moon causes tides on Earth by pulling at the oceans, this star pulls at the Sun’s
hot, gaseous surface. Due to the massive force of gravity, the Sun’s material stretches out in
the direction of the star, forming long streamers of gas.
3. Formation of Planetary Material
Some of the gas pulled out from the Sun gets ejected into space. Over time, this matter
cools and starts to break up into smaller fragments. These fragments condense into solid
bodies—what we now call planets.
4. Cooling and Condensation
As the ejected gases cool over millions of years, they shrink, become solid, and start moving
around the Sun in orbits. These are the proto-planets, and with time, they develop into the
planets of our solar system.
Support for the Tidal Hypothesis
In the early 20th century, this theory gained popularity for several reasons:
• It explained the similarity of chemical composition between the Sun and the planets.
• It seemed to provide a rational explanation for why all the planets lie more or less in
the same plane and revolve around the Sun in the same direction.