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Formation of Stars Like the Sun STAGE 1: AN INTERSTELLAR CLOUD. STAGE 2: A COLLAPSING CLOUD FRAGMENT. STAGE 3: FRAGMENTATION CEASES. STAGE 4: A PROTOSTAR. STAGE 5: PROTOSTELLAR EVOLUTION. STAGE 6: A NEWBORN STAR. STAGE 7: THE MAIN SEQUENCE AT LAST.
The origin of starts is called nebula. The nebula forms from the gaseous cloud with high density. This then collapse to form the pre stage of a star that is protostar then undergo fusion to form a star. Hence the sequence is nebula forms nebula collapses protostar forms fusion begins.
Summary. Many examples of star forming regions are observed in space. Stars form when an interstellar cloud collapses under its own gravity, heats, and breaks into pieces of star-sized masses. The evolution of the protostar can be represented as a path on the Hertzsprung-Russell diagram.
In triggered star formation, one of several events might occur to compress a molecular cloud and initiate its gravitational collapse. Molecular clouds may collide with each other, or a nearby supernova explosion can be a trigger, sending shocked matter into the cloud at very high speeds.
Star Formation Shapes the Appearance of the Universe and Provides the Sites for Planets. Step 1: initial collapse of an interstellar cloud. Step 2: the cloud fragments into clumps . The fragmentation is related to turbulence in the collapsing cloud. ( Step 3: The clumps collapse into a stars.
Star-Forming Nebula These knots contain sufficient mass that the gas and dust can begin to collapse from gravitational attraction. As it collapses, pressure from gravity causes the material at the center to heat up, creating a protostar. One day, this core becomes hot enough to ignite fusion and a star is born.
After millions of years, immense pressures and temperatures in the stars core squeeze the nuclei of hydrogen atoms together to form helium, a process called nuclear fusion. Nuclear fusion releases energy, which heats the star and prevents it from further collapsing under the force of gravity.
These knots contain sufficient mass that the gas and dust can begin to collapse from gravitational attraction. As it collapses, pressure from gravity causes the material at the center to heat up, creating a protostar. One day, this core becomes hot enough to ignite fusion and a star is born.