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Highest Mass a Star Can Have
I notice that the heat generated by a star's nuclear fusion reactions
counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? Michael |
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Highest Mass a Star Can Have
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Highest Mass a Star Can Have
nightbat wrote
Bruce wrote: In sci.physics (Michael Ejercito) wrote: I notice that the heat generated by a star's nuclear fusion reactions counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? The greater mass the star, the shorter the life. As for an absolute limit, I don't know but it certainly makes sense too me. nightbat For stellar mass upper limits in normal gravity fields see Chandra. For the brave who dare venture into strong constricting gravity fields, see nightbat's posts on the " Black Comet " singularity. the nightbat |
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Highest Mass a Star Can Have
COMMENT:
I'm interested in a related question, which is how small (not how large) can a gas planet be. We had a discussion about this in the forum last March, some of which I'll reprint. But it is made a bit more topical by a recent finding of a 2.5 Jupiter mass planet orbiting a dead neutron star in a globular cluster which is 12.5 billion years old, and therefore thought to represent completely first generation stars. Thus, planets there would have almost no "metalicity" (elements Li and heavier) since they'd be made of post big-bang gas only (carbon, silicon and oxygen are "metals" in this phrasology). Basically they'd be only H and He in the standard primordial ratio, and only traces of anything else. Now our own solar system gas giants are mostly H and He, but being 2nd generation planets they are thought to have "metallic" cores (maybe including a lot of carbon, but, certainly also a lot of silicate rock). But nobody thinks that if the cores of our solar system's gas giants disappeared, that they'd fly apart, do they? So why is everyone shocked when somebody finds a first generation star with a Jupiter-sized planet? But that seems to have been the reaction of professional astronomers a few weeks ago. Last March I calculated how big and massive would an object have to be, in order to have as much gravitational self-energy as (say) a diamond has from chemical self-energy. Objects bigger than this would be bound more tightly from gravity than chemistry ever could bind them, since a diamond's chemical energy per unit of mass is close to maximal for solids. (The negative bond chemical energy in hydrogen gas is 2e8 kJ/kg but it's not fair to use it here, since this energy only holds the atoms together in pairs, and isn't available to hold a collection of atoms together, which the negative potential of gravitational or carbon bond energy is). For silicate rock the chem self energy is about 1.5e7 J/kg. Call this E/M the target chem energy per mass, and symbolize it "U". Gravitational E/M for uniform spheres = 3/5 * G M/R (exercise left to student) Replacing M in the formula above with the density* volume = 4/3 * pi* rho R^3 Grav E/M = 3/5 * (G/R) * 4/3 * pi * rho * R^3 = 4/5 * pi * rho * G * R^2. Set this equal to U and solve for R: R^2 = 5U / (4pi*G*rho) Plug in numbers: U is roughly 1.5 e7 J/kg for silicate rock, and rho for such rocks is about 3500 kg/m^3, and G is 6.67e-11, This gives R of 5e6 meters, which is pretty close to the 6e6 m diameter of our own little silicate ball, the Earth. Which means that the Earth has about the same chemical binding energy/kg as it does gravitational energy. If we run the problem with a rho of 1000 kg/m^3 (pretty close to gas giants and our own sun, so probably not too far off a metal poor figure), R comes out 9.5e6 m, or a little larger than Earth, but with a mass only 3.5e24 kg, which is 60% of Earth's. So, if a planet with typical gas giant density and less than the mass of the Earth can be gravitationally bound as tightly (per gram) as a small rocky planet, then surely a planet 2.5 times Jupiter's mass (this would be about 5e27 kg) would have a large enough binding energy to survive any of the conditions any of the planets survived in our own solar system? |
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Highest Mass a Star Can Have
Michael Ejercito wrote:
I notice that the heat generated by a star's nuclear fusion reactions counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? The upper limit of about 80 solar masses for a star on the main sequence is due to photon pressure. At very high luminosity, the photons literally blow off outer layers of a more massive star. |
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Highest Mass a Star Can Have
Sam Wormley wrote:
Michael Ejercito wrote: I notice that the heat generated by a star's nuclear fusion reactions counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? The upper limit of about 80 solar masses for a star on the main sequence is due to photon pressure. At very high luminosity, the photons literally blow off outer layers of a more massive star. 80 solar masses may be too conservative Ref: http://www.aas.org/publications/baas...s/S006010.html Session 6 - HII Regions & Massive Star Formation. Display session, Wednesday, January 07 Exhibit Hall, [6.10] Star Formation in R136: A Cluster of O3 Stars Revealed by HST Spectroscopy. P. Massey (KPNO/NOAO), D. Hunter (Lowell Obs.) R136 is the extremely populous star cluster at the heart of the 30 Doradus nebula. We have obtained HST/FOS spectra of 65 of the brightest blue stars to investigate the massive star population of this prototype ``super star cluster", probably what a very young globular cluster would resemble. We find that over half the stars in our sample are of spectral type O3, the hottest, most luminous and massive subclass. We have identified more O3 stars in this remarkable cluster than were previously known elsewhere. The age of R136 is very young, 1-2 Myr. Despite the preponderance of so many high mass stars, we find that the IMF is completely normal, with a Salpeter slope (\Gamma=-1.3\pm0.1) extending from 2.8 \cal M_ødot to 100 \cal M_ødot. The most massive stars are well above the highest mass tracks available (120 \cal M_ødot), and a conservative estimate places the highest mass star at \sim 150\cal M_ødot, making this the highest mass unevolved star yet found. Comparing this to other clusters suggests that we have yet to encounter any physical limit to how massive a star may form in nature, that the only limit we see is a statistical one, depending upon the richness (and age) of the cluster. |
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Highest Mass a Star Can Have
Sam Wormley wrote:
Sam Wormley wrote: Michael Ejercito wrote: I notice that the heat generated by a star's nuclear fusion reactions counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? The upper limit of about 80 solar masses for a star on the main sequence is due to photon pressure. At very high luminosity, the photons literally blow off outer layers of a more massive star. 80 solar masses may be too conservative Ref: http://www.aas.org/publications/baas...s/S006010.html Astronomy Picture of the Day -- Massive Stars Of 30 Doradus Ref: http://antwrp.gsfc.nasa.gov/apod/ap990930.html http://antwrp.gsfc.nasa.gov/apod/ima.../30dor_hst.jpg |
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Highest Mass a Star Can Have
"Dr. Zarkov" wrote in message ... "Sam Wormley" wrote in message ... Michael Ejercito wrote: I notice that the heat generated by a star's nuclear fusion reactions counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? The upper limit of about 80 solar masses for a star on the main sequence is due to photon pressure. At very high luminosity, the photons literally blow off outer layers of a more massive star. I'm not sure if this is the question the previous poster had in mind, but I thought what he was asking was if there is any upper limit to a collapsing mass such that a star would never even form--where you would just get a collapse to a black hole (like galactic centers?) That was the answer given, but instead of turning into a black hole the star does during the main sequence the exact opposite - it shedds mass off in violent outbursts. The larger the star, the larger the outbursts. Of course, eventually and relatively soon, that star will have consumed it's energysource and due to the massive remaining mass it will become a black hole (unless some unknown prevents it), and very likely the initial black holes central in galaxies were formed like that. The original stellar massed black hole gulped up remaining gas, eventually entire stars, ending up with a mass of million and even billions that of the sun. Simulations indicate that the initial stars in the universe were all singular massive (30 Msun) stars just like this. Clear Skies, Magnus |
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Highest Mass a Star Can Have
PLANETS ORBIT THE SUN TO CONSERVE TOTAL ENERGY THE FORCE OF GRAVITY IS AN ILLUSION Gravitational effect is the result of an acceleration of mass. Galileo demonstrated this. Newton assumed that this was caused by a force of gravity between all masses. Was this a correct assumption? Einstein and many other scientists felt that there must be more to gravitation than an attraction at a distance. Action at a distance was considered to be impossible in the absence of a transfer of energy at the speed of light. Hubble then showed that the distant Galaxies were moving away from the earth and that the universe was expanding in all directions. If this is true , What else must be true? 1. The potential energy of the rest of the universe must be decreasing relative to the mass of the earth. It has long been assumed that the first law of thermodynamics, which says that the total energy of the universe is a constant, was a fact of nature. If this is true what then. 2. The kinetic energy of the universe must be increasing at the same rate that the potential energy is decreasing as the universe expands. How is this possible? Masses must be accelerating, because, kinetic energy change is the result of an acceleration. But all orbital masses are accelerating toward the center of the earth or some other mass. Why would this occur otherwise? 3. Orbital motion could then be the result of the expansion of the universe. The Gravitational illusion could be the result. Based on the first law of thermodynamics The total mass energy of the universe is a constant. (total kinetic (mass) energy plus total potential energy is a constant). m(2 pi L)^2 / t^2 + G (M-m)m / L = A constant. m is any mass say that of the earth. From this equation the equation Delta m (2 pi L)^2 / t^2 = - Delta G (M-m)m/L follows mathematically. From this equation the equation Delta m 4 pi^2 L /t^2 = Delta - G (M-m)m / L^2 or the modified Newton equation for gravity can be derived,but only when L is the orbital distance. The earth orbit is a result of an energy equilibrium, ( the absence of a change of total energy ) and not the result of a force of gravity between masses. Force of gravity is the resulting illusion assumed by Newton to be a force. If a planet (say earth) moved away from the sun its potential energy would decrease as L increased. Its kinetic energy would decrease because it is no longer accelerating toward the sun in orbital motion. Total energy would have to decrease. A very great change of total energy would have to take place. POTENTIAL ENERGY = G(M-m)m/L KINETIC ENERGY = m(2 pi L)^2/t^2 m(2 pi L)^2/t^2 + G(M-m)m/L = A constant = M G= Gravitational constant; M = total energy of the universe (or effective universe) ; m = mass in question. t = time ; L = radial distance. No mechanism exists for this to occur rapidly. So it could not happen. The magnitudes of kinetic and potential energies of planets and moons travelling in orbital motion are equal and any increase or decrease of orbital distance L results in an equal change in magnitude of both.This is the only value of L where no change of total energy will occur if the value of L changes. At any other distance L, an increase of kinetic energy will be at a different rate than potential energy desreases. Orbital motion conserves total energy. Force of gravity isn't needed to explain orbital motion or any other motion at a distance. GRAVITY MECHANICS AND RESEARCH ON ASTRONOMICAL OCEAN TIDES Copyright 1984 to 2002 Allen C. Goodrich An examination of United States Coast and Geodetic Survey Tidal Data, which was gathered by extensive measurements over long periods of time,was compared with astronomical data showing the phases of the moon at corresponding times for many years. This correlation of the two sets of data revealed a very interesting fact, in a manner that had never before been mentioned in the literature. It is invariably and exactly the lowest tide that exists directly under the full and new moons at deep ocean ports. This was a very interesting discovery because current physics,based on the gravitational theory, discussed in the following U.S.Gov. documents: PREDICT THE OCEAN TIDES http://co-ops.nos.noaa.gov/restles1.html SEE PHASES OF THE MOON FROM EARTH http://space.jpl.nasa.gov/ ,would lead one to believe that,except for many possible reasons, the highest tides tend to be under the full and new moons. The dictionary and encyclopedia as well as physics texts predict this with pictures of the earth and oceans bulging on the side facing the full moon. Of course it never happens as the gravitational theory predicts, and many reasons are given for the discrepancies. CONCLUSION: No discrepancies were found in the occurence of exactly the lowest tide directly under the full and new moons, at deep ocean ports. SIGNIFICANCE: One must admit that this is beyond question one of the most important discoveries of modern physics research. It indicates that a change must be made in the theory of gravitation. One can no longer assume that a force between the moon and the water of the earth's oceans, is causing the ocean tides. The force of gravity must be an illusion caused by some other, more basic, reason. What would this be? If the total energy ( kinetic and potential ) of the universe is assumed to be a constant,from this fundamental equation, many interesting things follow. If the rest of the universe is expanding ( potential energy decreasing) relative to masses, the masses must be shrinking ( increasing in kinetic energy ) (gravitation) relative to the rest of the universe. THE FIRST LAW OF MOTION-(GOODRICH) Copyright 1984 to 2002 ALLEN C. GOODRICH A body (m) continues in a state of rest (equilibrium) or motion in a straight or curved line (equilibrium) as long as no change occurs in its total (kinetic and potential) energy, relative to the rest of the effective universe (M-m), Delta mL^2/t^2 = - Delta K(M-m)m/L equilibrium = no change in the total energy relative to the rest of the effective universe (M-m). ^ = to the power of. Orbital motion complies with this equation. This equation is derived from the fundamental equation of the universe which states that the total energy of the universe is a constant. The sum of kinetic and potential energies is a constant. mL^2/t^2 + K(M-m)m/L = A constant. SEE THE UNIVERSE- A GRAND UNIFIED THEORY OF MASS ENERGY SPACE TIME FRAME MECHANICS-APPEARING IN NEWSLETTER "SPECTRUM" OF THE BUFFALO ASTRONOMICAL ASSOCIATION INC. NOV.1996 TO FEB.1997 See http://ourworld.cs.com/gravitymechan.../business.html FUNDAMENTAL EQUATION OF THE UNIVERSE http://ourworld.cs.com/gravitymechan...e/profile.html TIDES AND GRAVITY MECHANICS http://ourworld.cs.com/gravitymechan...ge/resume.html A new theory of gravitation is given, which predicted, stimulated the above research,and is consistent with, the new findings. Choosing a hobby that is in line with ones past experience can be a satisfying and rewarding undertaking. |
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Highest Mass a Star Can Have
"Magnus Nyborg" wrote in message ...
"Dr. Zarkov" wrote in message ... "Sam Wormley" wrote in message ... Michael Ejercito wrote: I notice that the heat generated by a star's nuclear fusion reactions counteract the gravity of the star. Is there a mass limit to stars, such that stars above this mass limit would collapse even though it is still producing heat from nuclear fusion reactions? The upper limit of about 80 solar masses for a star on the main sequence is due to photon pressure. At very high luminosity, the photons literally blow off outer layers of a more massive star. I'm not sure if this is the question the previous poster had in mind, but I thought what he was asking was if there is any upper limit to a collapsing mass such that a star would never even form--where you would just get a collapse to a black hole (like galactic centers?) That was the answer given, but instead of turning into a black hole the star does during the main sequence the exact opposite - it shedds mass off in violent outbursts. The larger the star, the larger the outbursts. Which would be true as long as the nuclear fusion reactions start before the escape velocity exceeds that of the speed of light. A black hole with a higher mass has a lower density than a black hole with a smaller mass. Currently, astrophysicists believe that gas must be compressed to enormous densities to form a star. A sufficiently massive cloud could collapse into a black hole before the nuclear fusion reactions begin. Michael |
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