[geocentrism] Re: Two spin axes of Earth?
- From: "philip madsen" <pma15027@xxxxxxxxxxxxxx>
- To: <geocentrism@xxxxxxxxxxxxx>
- Date: Mon, 12 Nov 2007 07:39:43 +1000
Is
there any reason why this phenomena would not also be the same for an
orbiting Sun about the Earth? Dynamic equivalence perhaps?
Jack
That is a very well placed intuitive question Jack.
From a HC mainstream scientific viewpoint where the sun is "known" ??? to have
a mass millions of times greater than our miniscule planet, I can not see any
possible answer, except a glance that indicates you are of the flat earth
variety person.... or at any rate a believer in Spirits..
Philip.
----- Original Message -----
From: Jack Lewis
To: geocentrism@xxxxxxxxxxxxx
Sent: Monday, November 12, 2007 12:26 AM
Subject: [geocentrism] Re: Two spin axes of Earth?
Dear Regner,
Thank you for your unexpected speedy reply!
In essence the elliptical orbit of the Earth is determined not by direct
observation but by indirect calculations of the centre of mass between the
Sun and the Earth. It is also by measuring the Sun's changing diameter. Is
there any reason why this phenomena would not also be the same for an
orbiting Sun about the Earth? Dynamic equivalence perhaps?
Jack
----- Original Message -----
From: "Regner Trampedach" <art@xxxxxxxxxx>
To: <geocentrism@xxxxxxxxxxxxx>
Sent: Sunday, November 11, 2007 1:38 PM
Subject: [geocentrism] Re: Two spin axes of Earth?
> The Earth's orbit is an ellipse with a small eccentricity (deviation from
> circle) of 0.0167 (circle is 0.0).
> First of all; an ellipse has two focal points ("centres")
> and a circle of course only has one. An ellipse can be drawn with two pins
> stuck into the paper, and a loop of thread around both, pulling the loop
> out to a triangle with your pen. Draw around the two pins with the loop
> taught and the result will be an ellipse. For close pins and a long loop
> you will get small eccentricity and close to an ellipse (small
> eccentricity).
> Second; the Sun-Earth centre-of-mass (about 450 km from the Sun's centre
> only 0.06% of the Sun's radius) will be at one focal point (one of the
> pins
> in your drawing) of the ellipse described by the Earth's orbit. The two
> focal points are symmetric about the actual centre of the ellipse. The
> main
> elliptical effect of a small eccentricity will be the offset by the focal
> point. And I can assure you that the Earth orbit I plotted is not a
> circle,
> although it is close.
> The Sun-Earth distance (the instantaneous radius of the Earth orbit) can
> be measured directly by the parallax method from opposite sides of the
> Earth.
> Variation in the Sun-Earth distance can also be measured by observing the
> change in apparent size of the Solar disk. The diameter of the orbit, on
> the
> other hand, cannot be measured, and also makes little sense when dealing
> with
> ellipses.
>
> Kind Regards,
>
> Regner Trampedach
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