Re: Semi-minor Axis
- From: Mike Williams <nospam@xxxxxxxxxxxxxxxxxx>
- Date: Sat, 31 Dec 2005 02:38:06 +0000
Wasn't it JG who wrote:
>Hi,
>
>I've been lurking and gaining a great deal of knowledge from this
>newsgroup for quite some time now but I have a very basic question that
>I have not seen asked.
>
>I used to think that Aphelion referred to the semi-major axis of the
>ellipse described by the Earth (or any planet) on its journey around the
>Sun and Perihelion was the semi-minor axis. Having read most of the
>planetary data from 'The Nine Planets' web site I now see that the sum
>of Aphelion and Perihelion is in fact the major axis of that ellipse.
>What I cannot understand is the statement in the Glossary that Aphelion
>is also the 'average' or mean distance of the planet from the Sun.
>
>Surely the maximum distance cannot also be the mean?
>
>What I really want to know is how to calculate the semi-minor axis.
>Given the 'Mean' and the eccentricity I can readily calculate the Major
>as a(1+e) and the Minor as a(1-e) but if the mean is also the Major then
>this doesn't make sense.
The aphelion is not the mean distance, and it doesn't say so in the nine
planets glossary:
http://www.nineplanets.org/help.html
aphelion
the point in its orbit where a planet is farthest from the Sun; when
refering to objects orbiting the Earth the term apogee is used; the
term apoapsis is used for orbits around other bodies. (opposite of
perihelion)
Nine Planets says that the *semimajor axis* is the average distance of
the planet from the Sun. (I'd claim that that depends what you mean by
"average". If you average over time, then you get a result that's longer
than the semimajor axis because the planet moves more slowly when
further from the Sun.)
--
Mike Williams
Gentleman of Leisure
.
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