# How do I fit the parameters describing a 3D object so that it best resembles its projection seen by an observer at a particular position?

I have data which are the longitudes (l) and latitudes (b) for the vertices of the edges of a shape as it appears to an observer at a given location (i.e., as it appears on the observer's sky plane).

Question: If I have some general idea what the original 3D object is (a surface of revolution formed from a lemniscate), how do I find the parameters of the 3D shape that best reproduce the 2D image the observer sees?

The data are (in degrees)

data = {{0, 0}, {-5.5, 5.}, {-10.7, 10.}, {-12.9, 15.}, {-15., 20.}, {-16.3, 25.},  {-16., 30.}, {-15.5, 35.}, {-15., 40.}, {-15., 45.}, {-10.6, 50.}, {-3.7, 52.5}, {6.3, 53.5}, {13.8, 50.}, {21.8, 45.}, {25.3, 40.}, {26.7, 35.}, {26.3, 30.}, {25.6, 25.}, {23., 20.}, {18.8, 15.}, {13.8, 10.}, {0, 0}}


In 3-space the observer is located at {xobs,yobs,zobs} = {-8,0,0} and I can assume the 3D object emanates from {0,0,0}

The transformation from general {x,y,z} to the angular position, {l,b}, on the observer's sky plane is given by

long[{x_, y_, z_}, {xobs_, yobs_, zobs_}] := ArcTan[(y - yobs)/(x - xobs)]

lat[{x_, y_, z_}, {xobs_, yobs_, zobs_}] := ArcTan[(z - zobs)/Sqrt[(x - xobs)^2 + (y - yobs)^2]]


As an example, take it that I know the 3D object is a surface of revolution formed from a lemniscate

lemSurface[x_, y_, z_, xa_, ya_, za_, c_] := (x^2 + y^2 + z^2)^2-2c^2(-(xa y - x ya)^2-(xa z - x za)^2-(ya z - y za)^2+(x xa + y ya + z za)^2)


The surface is given implicitly by

lemSurface[x, y, z, xa, ya, za, c]==0


where {xa, ya, za} is the vector around which the lemniscate is rotated and c scales its size.

So my question reduces to: how can I find the values for

xa, ya, za, c


such that the projected image best fits

data ?


One way to find the {x,y,z} coordinates of the edge of the object as it appears to the observer is that these are given implicitly by the requirement that these are

i) on the surface and ii) the observer is in the tangent plane for that coordinate on the surface.

The surface normal is given by

D[lemSurface[x, y, z, xa, ya, za, c], {{x, y, z}}]


The tangent plane at any point on the surface {xs,ys,zs} is then

D[lemSurface[xs, ys, zs, xa, ya, za, c], {{xs, ys, zs}}]).{x-xs,y-ys,z-zs}


so that the {x,y,z} coordinates of the edge of the object seen by the observer are given implicitly by

\[ScriptCapitalR] = ImplicitRegion[lemSurface[x, y, z, xobs, yobs, zobs, xa, ya, za, c] == 0 &&
D[lemSurface[x, y, z, xa, ya, za, c], {{x, y, z}}]).{xobs-x,yobs-y,zobs-z}== 0, {x, y, z}]


I can plot the [ScriptCapitalR] is 3 space via

DiscretizeRegion[\[ScriptCapitalR]]


but this still does not give me the {l,b} coordinates of the projected image or allow me to fit the image of the implicit region to data

• Hi ! You can start by going to the help centre, reading how to properly format your code and editing your post. – Sektor May 13 '15 at 11:53
• related: this answer by @Michael E2 and this by Silvia – kglr May 13 '15 at 12:12
• How are lLem, mLem, and nLem defined? – Virgil May 13 '15 at 12:47
• Sorry -- have no defined these above. – Confused astrophysicist May 13 '15 at 21:09
• lLem, mLem, and nLem are now defined above – Confused astrophysicist May 14 '15 at 4:40