SOLUTION: Planet​ A's satellite has an elliptical orbit described by X`2/(4963)`2+ Y`2/4796`2=1 ​(All units are in​ miles.) The coordinates of the center of Planet A

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Question 1110580: Planet​ A's satellite has an elliptical orbit described by
X`2/(4963)`2+ Y`2/4796`2=1
​(All units are in​ miles.) The coordinates of the center of Planet A are(21,0). Complete parts a and b below.
. The perigee of the​ satellite's orbit is the point that is nearest Planet​ A's center. If the radius of Planet A is approximately 4063 ​miles, find the distance of the perigee above Planet​ A's surface.
The​ perigee's distance above Planet​ A's surface is
879 miles.
b. The apogee of the​ satellite's orbit is the point that is the greatest distance from Planet​ A's center. Find the distance of the apogee above Planet​ A's surface.
The​ apogee's distance above Planet​ A's surface is __________miles.

Found 2 solutions by KMST, ikleyn:
Answer by KMST(5328) About Me  (Show Source):
You can put this solution on YOUR website!
As we do not know the radius or diameter of the satellite,
we are left to assume that its position and distances to the planet's surface are measured to the center of the satellite.
All distances are in miles, so the length unit is omitted from the calculations.

If the coordinates of the center of the satellite, S%28x%2Cy%29 ,
satisfy equation x%5E2%2F4963%5E2+%2B+y%5E2%2Fb%5E2=1 , with b%3C4963 ,
the orbit would look like this:
, with OV=OW=4963%3EOC=b .
If the planet center is at a point P%28p%2C0%29 with p%3E0
V would be the pericenter or periapsis,
and W would be the apocenter or apoapsis.
Those are the points where the satellite is closest and farthest from the planet, respectively.
(If the planet were Earth, those points would be called perigee and apogee).
A sketch showing those points and the planet on the coordinate plane
(drawn not to scale for clarity) is shown below:

with OP=21 and OV=OW=4963 .

If the radius of the planet is PB=PA=4063 ,
knowing from the sketch that OV=OP%2BPA%2BAV ,
when the satellite is closest to the planet, at V ,
we calculate its distance to the planet surface as
AV=OV-OP-PA%2B4963-21-4063=879 .
That distance is highlight%28879miles%29 .

When the satellite is farthest to the planet, at W ,
its distance from the planet surface is
WB=WO%2BOP-PB=4963%2B21-4063=921 .
That distance is highlight%28921miles%29 .

NOTE:
As the problem provides to data that would be unnecessary
for anyone familiar with orbits and ellipses,
and calculations show the data to be contradictory,
the solution above assumes no knowledge of focal distance of an ellipse, or physics.
Otherwise, the problem makes no sense to me,
and I believe it would feel just as wrong to anyone who has studied physics, pre-calculus/calculus, and/or astrophysics,
but feel free to get second and further opinions.
I assume that it is a problem for students who have not studied ellipses or physics,
and any knowledge of physics or ellipses should be ignored when solving the problem.

The equation given would make the semi-major axis and semi-minor axis
a=4963 and b=4796 respectively.
In turn, those values would make the focal distance of the ellipse
c=sqrt%284963%5E2-4796%5E2%29=sqrt%281629753%29=1276.617797
(with as many decimal places as my calculator and computer will give me).
Physics say that should be equal to the distance between O%280%2C0%29
and the center of the planet, P .
That should be 21 if the center of the planet is at P%2821%2C0%29 .



Answer by ikleyn(52781) About Me  (Show Source):
You can put this solution on YOUR website!
.
I read the given equation as

        X%5E2%2F4963%5E2 + Y%5E2%2F4796%5E2 = 1.


Based on the given equation, the orbit is elliptical, centered at (0,0), and with semi-axes a = 4963 (major semi-axis) and b = 4796.


Linear eccentricity c = sqrt%28a%5E2+-+b%5E2%29 = sqrt%284961%5E2-4796%5E2%29 = 1268.82


It is the distance from the ellipse center to the focus, where the planet should be located.


It contradicts to the given data regarding the planet center at (21,0).


The conclusion and the Diagnosis :


        The input data is not consistent with the basics of celestial mechanics.