Dark Matter Versus G - Revision history

BobdeHilster: /* Mass of the Galaxy */

2019-01-28T12:40:09Z

Mass of the Galaxy

← Older revision		Revision as of 08:40, 28 January 2019
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	The mass of the galaxy can be calculated from any point in Figure <xr id="fig:my-plot-blue-curve"/> using the following equation:		The mass of the galaxy can be calculated from any point in Figure <xr id="fig:my-plot-blue-curve"/> using the following equation:

	<math>M_g =\frac{v_o^2 R_o}{G_o}</math>		Equation 8: <math>M_g =\frac{v_o^2 R_o}{G_o}</math>

	~~Equation8gives~~ a value of <math display="inline">1.2 * 10^{38}</math> Kg for any point on the curve. This value is using Newton's equation and an adjusted value of G.		Equation 8 gives a value of <math display="inline">1.2 * 10^{38}</math> Kg for any point on the curve. This value is using Newton's equation and an adjusted value of G.

	<math>G_o =\frac{v_o^2 R_o}{M_g}</math>		Equation 9: <math>G_o =\frac{v_o^2 R_o}{M_g}</math>

	The Visible mass of the galaxy can be calculated by taking the estimated number of stars in our galaxy ( <math display="inline">~2.15 * 10^{12}</math> stars) and multiplying it by the mass of our sun ( <math display="inline">2 * 10^{30}</math> Kg). The value is: <math display="inline">2.3 * 10^{42}</math> Kg.		The Visible mass of the galaxy can be calculated by taking the estimated number of stars in our galaxy ( <math display="inline">~2.15 * 10^{12}</math> stars) and multiplying it by the mass of our sun ( <math display="inline">2 * 10^{30}</math> Kg). The value is: <math display="inline">2.3 * 10^{42}</math> Kg.

BobdeHilster: /* Using Newton's Equation with Shielding */

2019-01-28T12:38:29Z

Using Newton's Equation with Shielding

← Older revision		Revision as of 08:38, 28 January 2019
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	Equation1provides the opportunity to either select more mass (Dark Matter) or conclude that G is changing value as you move through the galaxy. By using Equation1, an equation for G can be obtained.		Equation1provides the opportunity to either select more mass (Dark Matter) or conclude that G is changing value as you move through the galaxy. By using Equation1, an equation for G can be obtained.

	<math>G = \frac{v^2 R}{M_g}</math>		Equation 4: <math>G = \frac{v^2 R}{M_g}</math>

	<math>G_o =\frac{v_o^2 R_o}{M_g}</math>		Equation 5: <math>G_o =\frac{v_o^2 R_o}{M_g}</math>

	<math>G_s =\frac{v_s^2 R_s}{M_g}</math>		Equation 6: <math>G_s =\frac{v_s^2 R_s}{M_g}</math>

	<math>G_s =\frac{v_o^2 R_o}{v_s^2 R_s}</math>		Equation 7: <math>G_s =\frac{v_o^2 R_o}{v_s^2 R_s}</math>

	~~Equation4is~~ the basic equation for G. ~~Equation5is~~ for a given distant star and ~~Equation6is~~ for our solar system. Finally, ~~Equation7is Equation5divided~~ by ~~Equation6to~~ provide a ratio for the value of Go relative to Gs <math display="inline">(6.67 * 10^{-11} N m^2/Kg^2</math> . The mass of the galaxy is assumed to be constant.		Equation 4 is the basic equation for G. Equation 5 is for a given distant star and Equation 6 is for our solar system. Finally, Equation 7 is Equation 5 divided by Equation 6 to provide a ratio for the value of Go relative to Gs <math display="inline">(6.67 * 10^{-11} N m^2/Kg^2</math> . The mass of the galaxy is assumed to be constant.

	To obtain the value of G, The blue curve of ~~Figure1was~~ placed on a grid and values of velocity and distance were obtained. The data is plotted in Figure <xr id="fig:my-plot-blue-curve"/> .		To obtain the value of G, The blue curve of Figure 1 was placed on a grid and values of velocity and distance were obtained. The data is plotted in Figure <xr id="fig:my-plot-blue-curve"/> .

	<figure id="fig:my-plot-blue-curve">		<figure id="fig:my-plot-blue-curve">

BobdeHilster: /* The Particle Model Gravity Equation */

2019-01-28T12:36:14Z

The Particle Model Gravity Equation

← Older revision		Revision as of 08:36, 28 January 2019
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	The particle model uses shielding in its equation.		The particle model uses shielding in its equation.

	<math>F = \sum\limits_{(p=1)}^{180} \sum\limits_{(a=1)}^{180} f_i (1-P_r) cos(a) sin(p)</math> ~~(3)~~		Equation 3: <math>F = \sum\limits_{(p=1)}^{180} \sum\limits_{(a=1)}^{180} f_i (1-P_r) cos(a) sin(p)</math>

	Where:		Where:

BobdeHilster: /* Force Equation Using Shielding */

2019-01-28T12:35:24Z

Force Equation Using Shielding

← Older revision		Revision as of 08:35, 28 January 2019
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	The equations which apply to the galaxy while including shielding are as follows:		The equations which apply to the galaxy while including shielding are as follows:

	<math>a=\frac{F}{m}=\frac{v^2}{R}</math>		Equation 2: <math>a=\frac{F}{m}=\frac{v^2}{R}</math>

	Which gives:		Which gives:

BobdeHilster: /* Inventing Dark Matter */

2019-01-28T12:34:35Z

Inventing Dark Matter

← Older revision		Revision as of 08:34, 28 January 2019
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	One equation that can be used to calculate the velocity of an object that orbits another object is shown in Equation 1.		One equation that can be used to calculate the velocity of an object that orbits another object is shown in Equation 1.

	<math>v = \sqrt{\frac{GM}{R}}</math> ~~(1)~~		Equation 1: <math>v = \sqrt{\frac{GM}{R}}</math>

	This equation gives a value of velocity that is too high at large distances. What is needed is that G or M in the equation must be higher or R must be lower. R is the measured distance from the selected star to the center of the galaxy. One could try to re-measure, but the value would probably be about the same. G is Newton's universal gravitational constant and is considered a constant. How can you change that?		This equation gives a value of velocity that is too high at large distances. What is needed is that G or M in the equation must be higher or R must be lower. R is the measured distance from the selected star to the center of the galaxy. One could try to re-measure, but the value would probably be about the same. G is Newton's universal gravitational constant and is considered a constant. How can you change that?

BobdeHilster: /* The Particle Model Gravity Equation */

2019-01-28T12:33:53Z

The Particle Model Gravity Equation

← Older revision		Revision as of 08:33, 28 January 2019
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	The particle model uses shielding in its equation.		The particle model uses shielding in its equation.

	~~<math>F=\Sigma_(p=1)^180 f_i (1-P_r) cos(a) sin(p)</math>~~		<math>F = \sum\limits_{(p=1)}^{180} \sum\limits_{(a=1)}^{180} f_i (1-P_r) cos(a) sin(p)</math> (3)

	<math>F = \sum\limits_{(p=1)}^{180} \sum\limits_{(a=1)}^{180} f_i (1-P_r) cos(a) sin(p)</math>

	Where:		Where:

BobdeHilster: /* The Particle Model Gravity Equation */

2019-01-28T12:31:16Z

The Particle Model Gravity Equation

← Older revision		Revision as of 08:31, 28 January 2019
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	* 'R Squared' is implied in the geometry.		* 'R Squared' is implied in the geometry.

	When ~~Equation3is~~ used to calculate the force throughout the Milky Way galaxy, then the values can be substituted into ~~Equation2~~, and the blue curve should be developed. This calculation is using the Particle Model equation for gravity that includes shielding and does not use G.		When Equation 3 is used to calculate the force throughout the Milky Way galaxy, then the values can be substituted into Equation 2, and the blue curve should be developed. This calculation is using the Particle Model equation for gravity that includes shielding and does not use G.

	==Using Newton's Equation with Shielding==		==Using Newton's Equation with Shielding==

BobdeHilster: /* Structure of the Galaxy */

2019-01-28T12:29:42Z

Structure of the Galaxy

← Older revision		Revision as of 08:29, 28 January 2019
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	</figure>		</figure>

	The vertical line is at the center of the core. At that point the number moving left (NL) is assumed to be equal to the number moving right (NR). These particles are there and some of them interact and push, but the net force at the core is zero.		The vertical line is at the center of the core. At that point the number moving left (NL) is assumed to be equal to the number moving right (NR). These particles are there and some of them interact and push, but the net force at the center of the core is zero.

	As you move to right and follow the lower curve there is more loss. There is a big loss through the core and less loss through the open space, and then more loss ~~trough~~ the 1st arm.		As you move to right and follow the lower curve there is more loss. There is a big loss through the core and less loss through the open space, and then more loss through the 1st arm.

	If you start at the far right and follow the top curve, to the left, the number of G1 particles decrease. When you reach the center of the core then NL is again the same as NR. It becomes very clear that there is a compounding effect on the force of gravity as you move from the core though the galactic plane, gaining in one direction and losing in the other.		If you start at the far right and follow the top curve, to the left, the number of G1 particles decrease. When you reach the center of the core then NL is again the same as NR. It becomes very clear that there is a compounding effect on the force of gravity as you move from the core though the galactic plane, gaining in one direction and losing in the other.

BobdeHilster: /* The Particle Model and Shielding */

2019-01-28T12:26:27Z

The Particle Model and Shielding

← Older revision		Revision as of 08:26, 28 January 2019
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	==The Particle Model and Shielding==		==The Particle Model and Shielding==
	The Particle ~~model~~ concept for shielding is based the interaction of G1 with an object. As the G1 enters an object it can pass straight through, it can hit the atom and push it, and it can get trapped by an atom and become an orbital. When it hits or when it gets trapped, the result is fewer G1s leaving; and this is the same as Le Sages shielding.		The Particle Model concept for shielding is based the interaction of G1 with an object. As the G1 enters an object it can pass straight through, it can hit the atom and push it, and it can get trapped by an atom and become an orbital. When it hits or when it gets trapped, the result is fewer G1s leaving; and this is the same as Le Sages shielding.

	==Structure of the Galaxy==		==Structure of the Galaxy==

BobdeHilster: /* Inventing Dark Matter */

2019-01-28T12:25:04Z

Inventing Dark Matter

← Older revision		Revision as of 08:25, 28 January 2019
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	===Inventing Dark Matter===		===Inventing Dark Matter===
	One equation that can be used to calculate the velocity of an object that orbits another object is shown in ~~Equation1~~.		One equation that can be used to calculate the velocity of an object that orbits another object is shown in Equation 1.

	<math>v = \sqrt{\frac{GM}{R}}</math>		<math>v = \sqrt{\frac{GM}{R}}</math> (1)

	This equation gives a value of velocity that is too high at large distances. What is needed is that G or M in the equation must be higher or R must be lower. R is the measured distance from the selected star to the center of the galaxy. One could try to re-measure, but the value would probably be about the same. G is Newton's universal gravitational constant and is considered a constant. How can you change that?		This equation gives a value of velocity that is too high at large distances. What is needed is that G or M in the equation must be higher or R must be lower. R is the measured distance from the selected star to the center of the galaxy. One could try to re-measure, but the value would probably be about the same. G is Newton's universal gravitational constant and is considered a constant. How can you change that?

	So, the scientists are left with M, the total mass of the galaxy and this must increase in some way. You have to give them credit for all the work that they do to show that visible matter is only about 5 percent of the mass needed to get the correct velocity. The other 95 percent is ~~called~~ dark matter.		So, the scientists are left with M, the total mass of the galaxy and this must increase in some way. You have to give them credit for all the work that they do to show that visible matter is only about 5 percent of the mass needed to get the correct velocity. The other 95 percent is dark matter and dark energy.

	==Le Sage and Shielding==		==Le Sage and Shielding==