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1
A system of natural philosophy: being a course of lectures ...
Therefore as LT encreases the additious force will bear a greater proportion to
the earths gravitation towards the sun ; ' and as LT decreases the addititious force
will bear a less proportion to that gravitation. But since TS is given, the earths ...
2
System of Natural Philosophy
Therefore as LT encreases the additious force will bear a greater proportion to
the earths gravitation towards the sun j and as LT decreases the addititious force
will bear a less proportion to that gravitation. But since TS is given, the earths ...
3
A commentary on Newton's Principia: with a supplementary ...
U hi Similarly the attraction on M is parallel to M R = ^Q^p^ • Let (m) = mean
addititious force of S on P. (n) = mean addititious force of S on E. Now since the
addititious force (Sect. XI.) ce distance, m . M O .*. the whole addititious force of S
on M ...
John Martin Frederick Wright, 1833
4
Commentary on Newton's Principia. With a suppl
Let (m) = mean addititious force of S on P. (n) = mean addititious force of S on E.
Now since the addititious force (Sect. XL) cc distance, .•• the whole addititious
force of S on M = — ^-tt — » and m. MO PO addititious force in the direction M R ...
John Martin F. Wright, 1828
5
The Rudiments of Mathematics ... The third edition
The former 'addititious or affirmative, before which you prefix the sign of addition+
5 the latter is subductitious or negative, before which you prefix the sign of
subtraction — . In computing the worth of such a person, if the addititious
quantities ...
William LUDLAM, M. FRYER (Teacher of Mathematics.), 1809
6
The First Three Sections of Newton's Principia, with an ...
As P moves from perigee to apogee, the ablatitious force tends to increase, and
the addititious force tends to diminish the obtuse angle TPy, which the tangent Py
makes with PT; also the velocity at any point, and therefore the axis major ...
Sir Isaac Newton, John E. EVANS, 1855
7
The American Journal of Science
Resolving this force into two others in the directions ME and ES, the proportion
for the former or addititious force will read SM : ME: 2m 2 the addititious force ME
=mm. To find the mean addititious force for the whole of the moon's orbit, we may
...
8
The American Journal of Science and Arts
Resolving this force into two others in the directions ME and ES, the proportion
for the former or addititious force will read SM : ME::m : the addititious force ME =
=SMrn" mean addititious force for the whole of the moon's orbit, we may
substitute ...
9
American Journal of Science
Resolving this force into two others in the directions ME and ES, the proportion
for the former or addititious force will read SM : ME1Im : the addititious force the
moon's orbit, We may substitute for m its mean value above _ _ S ><EB” _
obtained ...
10
A treatise on conic sections: and the application of algebra ...
9. To consider the effect of the central disturbing force on the eccentricity of P's
orbit. As P moves from perigee to apogee, the ablatitious force tends to increase,
and the addititious force tends to diminish the obtuse angle TPy, which the
tangent ...
