move a point up and down along a sphere I have a problem where i have a sphere and 1 point that can be anywhere on that sphere's surface. The Sphere is at the center point (0,0,0).
I now need to get 2 new points, 1 just a little below the and another little above this in reference to the Y axis. If needed or simpler to solve, the points can be about 15º above and below the original point, this viewing the movement on a 2D circle.
Thank you in advance for any given help. 
EDIT:
This is to be used on a world globe where the selected point will never be on the top or bottom.
EDIT:
I'm using the latitude and longitude suggested by rlgordonma and user1551
what I'm doing is adding and subtracting a fixed value to ϕ
These 2 apear correctly, at least they apear to look in place: 
The original point is in the middle of the 2 bars.
The sphere has R=1 all the coords i'm putting here are rounded because they are to big (computer processed)

coord: (0.77, 0.62, 0,11) 

coord: (0.93, -0.65, 0.019)
these don't:

coord: (-0.15, 0.59, 0.79)

coord: (-0.33, 0.73, -0.815)
there are other occasions for both but i didn't want to put all here.
calcs:
    R = 1
    φ = arctan(y/x)
    θ = arccos(z/1)
//to move up only one is used
    φ = φ + π/50
//to move down only one is used
    φ = φ - π/50

    (x,y,z)=(sinθ cosφ, sinθ sinφ, cosθ)

 A: What you need is a conversion between the spherical coordinate system and the Cartesian coordinate system. If $r$ denotes the radius of the sphere, $\theta=\text{polar angle}=\frac\pi2-\text{latitude}\in[0,\pi]$ ($0$ = North pole, $\pi$ = South pole) and $\varphi=\text{longitude}\in[0,2\pi)$, then the conversion from spherical coordinates to Cartesian coordinates is given by
\begin{equation}
(r,\theta,\varphi)\mapsto(x,y,z)=(r\sin\theta\cos\varphi,\,r\sin\theta\sin\varphi,\,r\cos\theta).\tag{1}
\end{equation}
To convert back from spherical coordinates to Cartesian coordinates to spherical coordinates, do the following:
\begin{align}
r&=\sqrt{x^2+y^2+z^2},\\
\theta&=\operatorname{acos}(z/r),\\
\varphi&=\operatorname{atan2}(y,x),
\end{align}
where atan2 is the quadrant-aware variation of the arc-tangent function. (Certainly you don't need the first equation in your case, as $r$ is a constant.) If you need to report the longtitude in your software, you should check the range of the implementations of acos and atan2 on your computer. If, e.g., the range of atan2 on your computer is $[-\pi,\pi)$, then you should compute $\varphi$ as the remainder of $\operatorname{atan2}(y,x)+2\pi$ modulo $2\pi$.
If you swing the point upward along a meridian by $15^\circ=\pi/12$ radians, the adusted spherical coordinates become
$$
\begin{cases}
(r,\theta-\frac\pi{12},\varphi)&\text{ if }\, \frac\pi{12}\le\theta\le\pi,\\
(r,\frac\pi{12}-\theta,-\varphi)&\text{ if }\, 0\le\theta<\frac\pi{12}.
\end{cases}
$$
Put these new spherical coordinates into $(1)$, you get the Cartesian coordinates of the adjusted point. Similarly, if you swing the point downward by $15^\circ$ along a meridian, the adusted spherical coordinates become
$$
\begin{cases}
(r,\theta+\frac\pi{12},\varphi)&\text{ if } 0\le\theta\le\pi-\frac\pi{12},\\
(r,2\pi-\theta-\frac\pi{12},-\varphi)&\text{ if } \pi-\frac\pi{12}<\theta\le\pi.
\end{cases}
$$
A: The conversion between Cartesian and spherical coordinates is 
$$ (x,y,z) = (R \sin{\theta} \cos {\phi},R \sin{\theta} \sin {\phi}, R \cos{\theta})$$
where $R$ is the radius of the earth/sphere, $\theta = $  $+90^{\circ}$- latitude, and $\phi=$ longitude.
A: Building on the other answers; there are multiple competing "standard" ways to assign axis labels and angles to locations on the sphere.  From your description and the recommendations in the other answers, I am assuming that $x$ and $z$ are in the plane of the equator and $y$ is the axis of rotation.  The polar angle is being measured from North.  You should double check all your conversions from lat/long.
I recommend that you use trigonometric sum and difference identities to convert your quantities rather than the simple approach of just arcsin and then sin, etc.  In addition to helping with the problem of keeping track of the quadrant of your coordinates, using identities directly preserves precision better especially if you are near $0$ or $90$.
For instance, you shouldn't actually be recalculating your $x$ and $z$ coordinates; since the $\lambda$ (or $\phi$, longitude if you prefer) is not changing, $\frac xz$ is not changing, so you should calculate a single scaling factor (one for each displacement) and apply it to both.
In case you don't already realize this, your coordinates are already essentially the (scaled) sin and cos of the spherical rotation angles.  So, for instance, instead of labelling $y$ just consider it $\cos \theta$.
(Just noticed that the other answers are using $z$ for the rotation axis, which is the norm; I changed my terms because you said $y$ was the rotation axis.  I think you might have an error from copying the recommendations without swapping the axis labels.)
p.s. Sorry to anyone who doesn't like my notation.  $\phi$ and $\theta$ may be more common for mathematical work on the sphere, but those that actually navigate on the (non-spherical) earth tend to use $\lambda$ and $\phi$.  Yes, I realize $\phi$ is in both but different places.  We also measure bearing angles differently.
