After the large knock, big parts of extremely heavy interstellar gas and dust began to roll up, condense and signifier galaxies. Within these galaxies, smaller revolving molecular clouds, composed preponderantly of H and He, began to organize, and within these clouds stars were born. Our Sun is one of the many stars in our galaxy. With mass 2×1023 kilogram, radius 696000 kilometer and brightness 3.86×1026 Watts, it is composed of 70 % Hydrogen, 28 % Helium and 2 % metals ( elements that are non hydrogen or He ) . Stars of similar multitudes have similar leading developments so the life of stars like our Sun, get downing from their birth in molecular clouds, is highly interesting for uranologists.
Molecular clouds have big densenesss ( 300 molecules/cm3 ) and highly low temperatures ( 10-30 K ) , leting the combine of atoms to organize molecules1, and are capable to two forces: an inward gravitative attractive force and an outwards gas/thermal pressure1. When the inward gravitative forces become larger than the outwards force per unit area forces the cardinal parts, which are capable to higher gravitative attractive force, are forced to contract2. This consequences in the prostration of the cloud and an addition in its temperature ( alteration in gravitative possible energy ( I”Egp ) increases atom kinetic energy ( KE ) leting more atom hits and the release of thermic energy in the signifier of photons1 ) . In order to contract, the cloud needs to stay cool as increasing thermic force per unit area would hinder leading formation. The release of thermic energy by photons keeps the cloud at the coveted temperature, leting it to go on contracting1.
When the cloud is compressed sufficiently so that its average denseness is highly light, the action of gravitative forces causes the homogenous medium to interrupt up into several condensations3. This atomization of molecular clouds demonstrates why stars frequently form in bunchs. The single clouds continue undertaking until they reach the ‘hydrostatic equilibrium line’2. The turning densenesss of the clouds inhibit the flight of photons and therefore the release of thermic energy.1 This causes a rise in temperature which increases the gas force per unit area of the cloud. Therefore, fast contraction ceases as the Centres of each cloud atomization become protostars, undertaking really easy.
A protostar is a new star before it begins to bring forth any atomic energy in its nucleus and set up a province of hydrostatic equilibrium. This province is achieved when its “ inward gravity attractive force precisely balances the outward force per unit area forces at every point within the star ” 4. Due to the preservation of the initial cloud ‘s angular impulse, an accumulation disc of gas and dust signifiers around the protostar5. Material from the disc can accrete onto the star, increasing the rate of protostar contraction. Gravitational attractive force causes affair to be pulled towards the protostar ‘s Centre and as a consequence, its cardinal parts contract more quickly, organizing a nucleus. Once the nucleus signifiers, it accretes affair from the environing envelope. The altering gravitative possible energy of this affair produces heat, doing the dust grains and gas to radiate infrared wavelengths4. As the star continues to contract, its “ self gravity ” 4 additions, so the internal force per unit areas increase to develop hydrostatic equilibrium. The star is now a really aglow pre-main sequence star.
Now in a province of hydrostatic equilibrium, the star ‘s thermic energy content approximately equals its gravitative binding energy6. At the star ‘s Centre, the gas force per unit area increases to counter balance the star ‘s increasing weight due to the accumulation of mass from the accumulation disc. The pre-main sequence star easy collapses until there is adequate energy in the nucleus to light thermonuclear reactions, doing it a “ existent star ” .
The star has now become a chief sequence star. The bulk of known stars, including our Sun, prevarication on the chief sequence line of the Hertzsprung-Russell diagram which is a secret plan of leading brightness versus temperature, with the chief sequence shown as a diagonal line running from the underside right to the top left manus corner. Stars spend on mean 80 % of their lives in the chief sequence phase firing H to helium in their nucleuss.
Thermonuclear reactions provide the long term energy beginnings for stars.4 Main sequence stars fuse H to helium in their nucleuss via two chief reactions: the Proton-Proton ( p-p ) concatenation and the Carbon Nitrogen Oxygen ( CNO ) rhythm. The presence of each reaction is determined by leading mass ; the p-p concatenation dominates in low mass stars ( & lt ; 1.5 solar multitudes ) , while the CNO rhythm is more outstanding in high mass stars ( & gt ; 1.5 solar multitudes ) with big nucleus temperatures ( & gt ; 1.8 x107 K ) . In our Sun, both reactions take topographic point nevertheless, the p-p concatenation is more of import and occurs 91 % of the time3. In the p-p concatenation reaction 4hydrogen karyon fuse together to organize 1 He karyon:
1H +1H – & gt ; 2H +e++ V
2H + 1H – & gt ; 3He +g
3He + 3He – & gt ; 4He + 1H + 1H
The CNO rhythm still contains 4 H uniting to bring forth 1 He nevertheless it is a six phase procedure and requires the usage of C as a accelerator:
12C + 1H – & gt ; 13N + g
13N – & gt ; 13C + e+ + g
13C + 1H – & gt ; 14N + g
14N + 1H – & gt ; 15O + g
15O – & gt ; 15N + e+ + V
15N + 1H – & gt ; 12C + 4He
It is possible to observe C ‘s function as a accelerator by detecting that the rhythm starts with the reaction of a C and a H karyon and ends with the release of an indistinguishable C karyon, therefore non being used up in the procedure. This procedure dominates in hotter chief sequence stars as the coulombic barriers of C and N are greater than that of protons and He nuclei4 and therefore tonss of heat is required to get the better of the electrostatic/coulomb abhorrent forces on the karyon. Similarly, the CNO rhythm dominates in high mass stars as more monolithic stars have a larger gravitative pull towards the nucleus and therefore they generate the high temperatures which the rhythm requires.
Over clip, as the H copiousness in the nucleus decreases, nucleus temperature and denseness addition to keep the same rate of atomic fusion4 nevertheless, the cardinal denseness of the star stays comparatively changeless. A star like our Sun has adequate H in its nucleus to fuel it for 10 billion years5 nevertheless, merely 10 % of this H is used for energy coevals during the chief sequence stage of the star ‘s lifetime2. As stars fuse H to helium their temperature additions, they expand somewhat and due to the greater energy flow to the surface, they increase in brightness doing them to travel up the chief sequence.
Low mass stars like our Sun remain on the chief sequence, firing H, for about 10 billion old ages. However, one time the He content in the nucleus reaches 12 % , H merger Michigans. As no energy is being produced in the nucleus there is no longer the outwards radiation force per unit area to keep hydrostatic equilibrium with the gravitative forces and the star collapses. The alteration in gravitative possible energy of the atoms due to the cloud ‘s contraction gives rise to an addition in their kinetic energy, therefore bring forthing thermic energy. This heats up a H shell environing the nucleus doing it to get down merger once more. As this H firing shell develops, the star ‘s contraction rate slows and the shell additions in thickness. “ This merger is terminated when thermic instability arises in the shell. The shell narrows, the nucleus “ prostrations ” and the environing envelope quickly expands ” 6 to organize a Red Giant.
A Red Giant has all its mass concentrated in a nucleus of a few Earth radii at temperatures of about 50 million K. This high denseness causes the negatrons in the nucleus to go pervert ( “ occupy the same cell in stage infinite ” 7 ) bring forthing a pervert gas force per unit area which stops the ruddy giant nucleus from fall ining although no atomic reactions are taking place8. The enlargement of the star ‘s envelope as it evolves from a chief sequence star to a ruddy giant means a lessening in surface temperature and an addition in opacity. Opacity is “ the phenomenon of non allowing the transition of electromagnetic radiation ” 9 and so convection carries the star ‘s energy outwards through the spread outing envelope. This causes the star to be really aglow, apparent in its arrangement on the Hertzsprung-Russel diagram.
Figure – The Hertzsprung – Russell diagram
Although the outer beds of the giant are spread outing, the nucleus of the star continues to contract. After a short stage of nucleus contraction, the nucleus temperature becomes high plenty to light He merger. This is called the Helium Flash and He fuses to organize C in the Triple Alpha Process.
4He + 4He – & gt ; 8Be +g
8Be + 4He – & gt ; 12C +g
As the He nucleus is debauched, increasing temperature due to its merger does non do an addition in gas force per unit area and hence the nucleus does non spread out. The increasing temperature does nevertheless increase the rate at which the three-base hit alpha procedure takes topographic point. Finally, the energy released by the He flash raises the nucleus temperature to a point ( about 350 K ) where the negatrons in the gas are no longer devolve and the thermic force per unit area becomes strong plenty to “ force against gravitation ” 10 ensuing in an enlargement of the nucleus. The merger stops in the nucleus but continues in the environing bed, doing it to spread out into a ruddy giant once more and travel up the asymptotic giant branch8. This subdivision is occupied by stars with a helium-filled nucleus surrounded by a helium-fusion shell which is enclosed by a hydrogen-fusing shell11.
The more monolithic the star, the greater the nucleus temperature produced by gravitative contraction before degeneration sets in and the heavier elements it can blend. In high mass stars, the nucleus finally gets hot plenty so that the ternary alpha procedure can blend from C to neon to oxygen to magnesium to silicon and sulphur all the manner up to press. However, no affair how monolithic the star, the heaviest component that can be produced during merger is iron. These elements are so thrown back into the interstellar medium by the supernova detonations of the more monolithic stars and without the triple-Alpha reaction, there would be merely H and He gas in the universe resulting in no solid planets and no life. Unfortunately for our Sun and similar stars, C is the furthest component they can blend as they will ne’er accomplish a high adequate temperature to light C merger.
As the contraction of the nucleus does non bring forth adequate energy for the combustion of C, it contracts to a extremely tight province increasing the rate of He combustion in the procedure. The star so pulsates8 until the He is exhausted from the nucleus doing it to fall in and chuck out its outer beds. The envelope of outer beds separates from the nucleus as a thin shell, spread outing and chilling. This is called a planetal nebula and exists as a “ aura ” around the remnant nucleus of the star. For stars less than 1.4 solar multitudes ( the Chandrasekhar bound ) the staying nucleus becomes a white midget composed of preponderantly C and O. White midget can non hold multitudes greater than 1.4 solar multitudes as the degeneration force per unit area of multitudes greater than this is deficient to forestall farther prostration.
White midget are so heavy that the atoms become wholly ionised ( pervert ) suppressing the random motion of negatrons and forestalling farther prostration. White dwarfs radiance entirely due to the left over kinetic energy of atomic karyon in their inside as thermonuclear reactions do non take topographic point in their nucleuss. The gesture of these karyons finally ceases, doing the white midget to chill and go a black midget.
The survey of leading formation offers great penetration into the formation and construction of the existence. By analyzing the formation of stars of similar size to our Sun, we further our apprehension of our Sun which in bend AIDSs in an apprehension of our solar system and therefore planet Earth. Leading formation is both a important and a genuinely astonishing subject of research.
Bennett. J, Donahue. M, Schneider. N, Voit. M, The Cosmic Perspective, “ Star Birth ” , chapter 16, 2009, Pearson Education Inc.
Bohm-Vitense. E, Introduction to Stellar astrophysics. V 3, “ Leading Structure and Evolution ” , 1992, Cambridge University, Cambridge
Shklovskii. L, Stars -Their Birth, Life & A ; Death, 1978, W.H Freeman & A ; company
Zeilik. M, Gregory. S. A, Smith. E, Introductory Astronomy & A ; Astrophysics 3rd edition, 1992, Saunders College publication
Bailey. J, Introduction to Astronomy Lectures, “ Lecture 13 – Our Star – The Sun ” , “ Lecture 14 – Properties and Evolution of Stars ” , “ Lecture 15 – Leading Birth and Death ” , 2009, UNSW School of Physicss
Chiu. H. Y, Muriel. A, Stellar Evolution, 1972, Cambridge, Mass, MIT Press
“ Electron Degeneracy ” , [ ONLINE ] , hypertext transfer protocol: //www.astro.utoronto.ca/~bclarke/AST199T/definitions.html
Zeilik. M, Gregory. S. A, Introductory Astronomy & A ; Astrophysics 4th Edition, 1998, Thomson Learning Iraqi National Congress, USA
“ Word cyberspace ” , [ ONLINE ] , wordnetweb.princeton.edu/perl/webwn, A© 2010 The Trustees of Princeton University
Bennett. J, Donahue. M, Schneider. N, Voit. M, The Cosmic Perspective, “ Star Stuff ” , chapter 17, 2009, Pearson Education Inc.
“ Asymptotic giant subdivision ( AGB ) ” , [ ONLINE ] , hypertext transfer protocol: //www.daviddarling.info/encyclopedia/A/AGB.html,
