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Practice Speaking: Read Aloud
ID: #34708
Long Nebular Hypothesis
The most widely accepted model for planet formation, known as the nebular hypothesis, begins with a swirling disc of gas and dust left over material from the birth of a nearby star. At some point in time, gravity triumphs over the pressure supporting this cosmic dust, which then starts to rotate, quickly collapsing under its own gravity.
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The most widely accepted model for planet formation, known as the nebular hypothesis, begins with a swirling disc of gas and dust left over material from the birth of a nearby star. At some point in time, gravity triumphs over the pressure supporting this cosmic dust, which then starts to rotate, quickly collapsing under its own gravity.
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Explanation
The most widely accepted model for planet formation, known as the nebular hypothesis, begins with a swirling disc of gas and dust left over material from the birth of a nearby star. At some point in time, gravity triumphs over the pressure supporting this cosmic dust, which then starts to rotate, quickly collapsing under its own gravity.
Words in Bold -> Plosives
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