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The Formation of a Star

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Submitted By deeptoot1
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Armando I Cortes
Nov. 17. 2025
Mrs.Lisa Smith
The Formation of a Star
The basic idea of star formation is gravitational collapse – the contraction of a region of gas under the influence of gravity. This is a simple process that would be expected to occur in any region of material dense enough for collisions between atoms to radiate away energy. However, the gas must be dense enough for collisions to occur and the temperature must be low enough for the atomic velocities not to be able to escape the system's gravity, so star formation only occurs in a few areas.

The sites of star formation in the galaxy are mostly located within molecular clouds – expansive, cool clouds of mostly hydrogen and helium gas. Molecular clouds are on average too diffuse to contract gravitationally, but within a cloud are regions of locally higher density, which are the sites of active star formation. It is not known exactly what causes molecular clouds and star-forming regions to be distributed as they are. However, it appears to be related to the spiral-arm structure of spiral galaxies, which is thought to be the result of density waves passing through the disk, compressing matter and igniting star formation in their wake, leaving the trails of young, hot, blue stars in their wake that are the primary feature of spiral galaxies.

The distribution of gas in these regions is probably erratic enough that once a sufficient compression comes through a large number of separated regions will be triggered to contract individually. One a sufficiently dense region begins to contract, the process becomes self-sustaining, as contraction only increases the density and makes contraction more rapid. Any net rotation in the region will be flattened by conservation of angular momentum as the cloud contracts and spins more rapidly, making the contracting region attain the shape of a disk.

The center of mass of the cloud will, of course, be the location of highest density, and as matter rains onto the center it will heat up rapidly to very high temperatures. This 'protostar' will emit strong radiation and winds which, while not immediately enough to stop the influx of matter from the disk, generates powerful outflow jets along the poles of the system, which may also be influenced by magnetic force originating in the disk.

Throughout the process the temperature, density, and pressure in the protostar at the center are increasing, and soon approach figures comparable to normal stars. Once the temperature of the center reaches about 15 million degrees the velocities of the hydrogen nuclei in the center become so fast that they are able to overwhelm their electric repulsion (hydrogen nuclei, protons, are positively charged and repel each other fiercely) and fuse to form a deuterium nucleus, which can collide with a second, similarly produced deuterium to form helium. This releases a huge amount of energy, heating up the core further, up to the point where it is finally hot enough to emit enough radiation to stop the system from collapsing. With the matter infall stopped, most of the light gas molecules such as hydrogen are blown out to the outer areas of the system, leaving a higher abundance of heavier elements in the interior. This disk of dusty matter may or may not form planets, depending on the conditions, and the outer part of system may or may not do so as well. It's not really known what will cause planets to form or not.

This process may vary quite a bit depending on the conditions. If the progenitor cloud region is large and dense enough, the forming star can potentially be enormous, perhaps up to 100 solar masses. Large stars like become so hot in the interior that fusion takes place at millions of times the rate of sunlike stars, causing gas to stream off the surface of the star in great quantities that will collide with the remnant matter in the rest of the cloud, perhaps causing shocks that serve to produce additional star formation.

There's plenty of evidence for star formation at various stages of this process, mostly in infrared light since the gaseous disk that forms around forming stars tends to block all the visible light.

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