Within the disc of gas and dust that surrounded the protoSun
there was a radial temperature...
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Within the disc of gas and dust that surrounded the protoSunthere was a radial temperature gradient outwards to the edge of thedisc. Describe the sequence of events that led to the beginning ofplanet formation (i.e. when planetary embryos were colliding). andthe effect the temperature gradient had on this process. (About 150words)
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Answer The sequence of events that led to the beginning of planet formation Step IFrom dust to planetesimals When a molecular cloud collapsed under its own gravity to form a star the material formed a disklike structure in orbit around the central object due to the conservation of angular momentum Planetesimals formed due to the collective gravity of massive swarms of small particles concentrated at some locations local maxima of the gas density
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