The Origin Of Dense Star Clusters By Paul Nethercott

1. The Origin Of Dense Star ClustersBy Paul Nethercott R-136a Rigel Sun Dwarf October, 2010 www.creation.com

2. Pismis 24-1 www.creation.com

3. R= Search area radius, metres r = Orbital radius, metres [1] Area Probability [2] R= Search area radius, metres r = Orbital radius, metres A = Australia’s surface area, square centimetres PA= Bullseye’s surface area. Australian, Area Probability [3] R= Target circle radius, metres Australian, Target Radius [4] v = Star’s velocity in space, metres/second T = Seconds Search Time, Seconds [4] V= Star’s velocity in space, metres/second T = Seconds Search Time [5] M = Stars mass, kilograms P = Nebula density, kilograms/cubic metre V = Volume, cubic metres Solar Nebulae Volume R = Orbital radius, metres R1 = Star 1 radius, metres R2 = Star 2 radius, metres Binary Stars cannot form if F > 1 or = 1 [6] Solar Nebulae Overlap Ratio www.creation.com

4. [7] Solar Nebulae Radius [8] Rs = Metres [average] between stars centres Solar Separation Radius [9] Star Clusters Volume, Cubic metres R= Radius, metres [10] Vs = Empty space around a star, cubic metres Rc = Clusters radius, metres n = Number of stars in cluster Solar Space Volume [11] Stars cannot form if W > or = 1 Solar Nebulae Space Overlap Ratio [12] Solar Nebulas Radius, Overlap Metres www.creation.com

5. The Origin Of Dense Star Clusters Arches Cluster R 136a NGC 3603 Quintuplet Star Cluster

6. The Origin Of The Arches Star Cluster • The Problem of overlapping accretion nebulas. • Actual observed radius versus maximum allowed radius

7. The Origin Of NGC 3603 and R 136a • The Problem of overlapping accretion nebulas. • Actual observed radius versus maximum allowed radius

8. Binary Star Formation, Turning Force Orbital Velocity, Metres/Second Force Needed Per Second, Newtons Total Force Needed, Newtons • Third Star’s Mass, Kilograms • Second Star One Million Kilometres Power needed, Watts • Third Star’s Turning Time, Seconds Distance [Y] with velocity v Orbital Period, Seconds www.creation.com

9. Hypothetical Third Star, Mass And Size Force Per Second, Newtons • Third Star’s Mass, Kilograms Total Turning Force, Newtons • Third Star’s Volume, Cubic Metres • Second Star One Million Kilometres • Third Star’s Radius, Metres • Third Star www.creation.com

10. Binary Star Formation, Explosives Needed Total Force Needed, Newtons E = Free fall kinetic energy, Joules [15] [26] E = Orbital kinetic energy, Joules Force Needed Per Second, Newtons [17] [18] Eh = Excess heat energy, Joules Second Planet’s Mass, Kilograms [16] Y = Final orbital radius, metres v= Final velocity, meters per seconds Orbital period, Seconds [14] Nuclear energy conversion rate Power, Watts [19] [24] Radius explosive sphere Turning Time Second [21] [25] Mass Of TNT, Tri Nitro Toluene Kilograms Uranium [20] Mass Of Uranium Kilograms [23] G = G constant = 6.673 x 10-11 M = Mass of the primary, kilograms X = Starting orbital radius, metres. Y = Final orbital radius, metres v= Final velocity, meters per seconds [13] www.creation.com TNT, Tri Nitro Toluene

11. The Tolman-Oppenheimer-Volkoff Equation Excess Kinetic Energy [35] Escape Velocity [37] Binary Star Formation, Hydrostatic Equilibrium [29] Gas Molecule Speed [30] [36] [31] • Hydrostatic Gas Equilibrium [33] • The Oppenheimer-Volkoff Equation • Hydrostatic Gravity Equilibrium [34] • Temperature Increase [32] • Equation of State for Hydrostatic Equilibrium • Schwarzschild radius: www.creation.com