I've been trying to get the correct normals for a sphere I'm messing with using a vertex shader. The algorithm can be boiled down simply to
vert.xyz += max(0, sin(time + 0.004*vert.x))*10*normal.xyz
This causes a wave to roll across the sphere.
In order to make my normals correct, I need to transform them as well. I can take the tangent vector at a given x,y,z, get a perpendicular vector (0, -vert.z, vert.y), and then cross the tangent with the perp vector.
I've been having some issue with the math though, and it's become a personal vendetta at this point. I've solved for the derivative hundreds of times but I keep getting it incorrect. How can I get the tangent?
Breaking down the above line, I can make a math function
f(x,y,z) = max(0, sin(time + 0.004*x))*10*Norm(x,y,z) + (x,y,z)
where Norm(..) is Normalize((x,y,z) - CenterOfSphere)
After applying f(x,y,z), unchanged normals
What is the correct f '(x,y,z)?
I've accounted for the weirdness caused by the max in f(...), so that's not the issue.
Edit: The most successful algorithm I have right now is as follows:
Tangent vector.x = 0.004*10*cos(0.004*vert.x + time)*norm.x + 10*sin(0.004*vert.x + time) + 1
Tangent vector.y = 10*sin(0.004*vert.x + time) + 1
Tangent vector.z = 10*sin(0.004*vert.x + time) + 1
2nd Tangent vector.x = 0
2nd Tangent vector.y = -norm.z
2nd Tangent vector.z = norm.y
Normalize both, and perform Cross(Tangent2, Tangent1). Normalize again, and done (it should be Cross(Tangent1, Tangent2), but this seems to have better results... more hints of an issue in my math!).
This yields this
Get tangent/normal by derivate of function can sometimes fail if your surface points are nonlinearly distributed and or some math singularity is present or if you make a math mistake (which is the case in 99.99%). Anyway you can always use the geometric approach:
1. you can get the tangents easy by
U(x,y,z)=f(x+d,y,z)-f(x,y,z);
V(x,y,z)=f(x,y+d,z)-f(x,y,z);
where d is some small enough step
and f(x,y,z) is you current surface point computation
not sure why you use 3 input variables I would use just 2
but therefore if the shifted point is the same as unshifted
use this instead =f(x,y,z+d)-f(x,y,z);
at the end do not forget to normalize U,V size to unit vector
2. next step
if bullet 1 leads to correct normals
then you can simply solve the U,V algebraically
so rewrite U(x,y,z)=f(x+d,y,z)-f(x,y,z); to full equation
by substituting f(x,y,z) with the surface point equation
and simplify
[notes]
sometimes well selected d can simplify normalization to multipliyng by a constant
you should add normals visualization for example like this:
to actually see what is really happening (for debug purposses)
Related
I am having readings of Yaw, pitch, Roll, Rotation matrix, Quaternion and Acceleration. These reading are taken with frequency of 20 (per second). They are collected from the mobile device which is moving in 3D space from one position to other position.
I am setting reference plane by multiplying inverse matrix to the start postion. The rest of the readings are taken by considering the first one as a reference one. Now I want to convert these readings to 3D cartesian system.
How to convert it? Can anyone please help?
Ok basically yaw, pitch and roll are the euler angles, with them you got your rotation matrix already.
Quaternions are aquivalent to that, with them you can also calculate the rotation matrix you need.
If you have rotation matrices R_i for every moment i in your l=20secs interval. Than these rotations are relative the the one applied at R_(i-1) you can calculate their rotation relative to the first position. So A_i = R_1*...*R_i but after all you could also just safe the new direction of travel (safes calculations).
So asuming that the direction of travel is d_0 = (1,0,0) at first. You can calculate the next by d_i = R_i*d_(i-1) (always norm d_(i-1) because it might get smaller or bigger due to error). The first position is p and your start speed is v_0 = (0,0,0) and finally the acceleration is a_i. You need to calculate the vectorial speed v_i for every moment:
v_i = v_(i-1) + l*a_i*A_i*d_0 = v_(i-1) + l*a_i*d_i
Now you basically know where you are moving, and what kind of speed you use, so your position p_i at the moment i is given by:
`p_i = p_0 + l * ( v_1 + v_2 + ... + v_i)`
For the units:
a_i = [m/s^2]^3
v_i = [m/s]^3
p_i = [m]^3
Precision
Now some points to the precision of your position calculation (just if you want to know how good it will work). Suppose you have an error e>= ||R_i*v-w|| (where w is the correct vector). in the data you calculate the rotation matrices with. Your error is multipling itself so your error in the i moment is e_i <= e^i.
Then because you apply l and a_i to it, it becomes:
f_i <= l*a_i*e^i
But you are also adding up the error when you add up the speed, so now its g_i <= f_1+...+f_i. And yeah you also add up for the position (both sums over i):
h_i <= g_1+...+g_i = ΣΣ (l*a_i*e^i) = l* ΣΣ (a_i*e^i)
So this is basically the maximum difference from your position p_i to the correct position w (||p_i - w|| <= h_i).
This is still not taking in account that you don't get the correct acceleration from your device (I don't know how they normally do this), because correct would be:
a_i = ||∫a_i(t) dt|| (where a_i(t) is vectorial now)
And you would need to calculate the difference in direction (your rotation matrix) as:
Δd_i = (∫a_i(t) dt)/a_i (again a_i(t) is vectorial)
So apart from the errors you get from the error in your rotations from your device (and from floating point arithmetic), you have an error in your acceleration, I won't calculate that now but you would substitute a_i = a_i + b_i.
So I'm pretty sure it will be far off from the real position. You even have to take in account that you're speed might be non zero when it should be!
But that beeing said, I would really like to know the precision you get after implementing it, that's what always keept me from trying it.
I have started to develop unit trajectories for a game server and for now I'm trying to retrieve the position of a unit at a given time. It is easy when the trajectory is just a straight line, but it is far more complicated when unit chases another unit.
I've done flash app to illustrate the problem. Black trajectory is for unit which travels in a single direction. Blue chases black and red chases blue. What I want is to precalculate whole trajectory for blue and red to be able to retrieve their position in a constant time.
Is it possible? Thanks for any help!!
Here's a paper A classic chase problem solved from a
physics perspective by Carl E. Mungan that solves a particular version in which the chaser is initially perpendicular to the chased object's trajectory. I believe this is an inessential element of the solution since that perpendicularity disappears along the rest of the trajectory.
It is an autonomous system of differential equations in the sense that time does not appear explicitly in the coefficients or terms of the equations. This supports the idea that the family of solutions given in the paper is general enough to provide for non-perpendicular initial conditions.
The paper provides further links and references, as well as a useful search term, "curves of pursuit".
Let's state a slight different, slightly more general initial condition than Mungan's. Suppose the chased object ("ship") is initially located at the origin and travels up the positive y-axis (x=0) with constant speed V. The chasing object ("torpedo") is initially located at (x0,y0), and although instantaneous reorienting directly at the "ship", also travels at some constant speed v.
The special case where x0 is zero results in a linear pursuit curve, i.e. a head-on collision or a trailing chase accordingly as y0 is positive or negative. Otherwise by reflection in the y-axis one may assume without loss of generality that x0 > 0. Thus rational powers of x-coordinates will be well-defined.
Assume for our immediate purpose that speeds V,v are unequal, so that ratio r = V/v is not 1. The following is a closed-form solution (1) for the "torpedo" curve similar to Mungan's equation (10):
(1+r) (1-r)
[ (x/H) (x/H) ]
(y/H) = (1/2) [ ----- - ----- ] + C (1)
[ (1+r) (1-r) ]
in which the constants H,C can be determined by the initial conditions.
Applying the condition that initially the torpedo moves toward the ship's location at the origin, we take the derivative with respect to x in (1) and cancel a factor 1/H from both sides:
r -r
dy/dx = (1/2) [ (x/H) - (x/H) ] (2)
Now equate the curve's slope dy/dx at initial point (x0,y0) with that of its line passing through the origin:
r -r
(x0/H) - (x0/H) = 2y0/x0 = K (3)
This amounts to a quadratic equation for positive B = (x0/H)^r:
B^2 - K*B - 1 = 0 (4)
namely B = [K + sqrt(K^2 + 4)]/2 (but use the alternative form if K < 0 to avoid cancellation error), which allows H to be determined from our knowledge of x0 and r:
H = x0/(B^(1/r)) (5)
Knowing H makes it a simple matter to determine the additive constant C in (1) by substituting the initial point (x0,y0) there.
The tricky part will be to determine which point on the "torpedo" trajectory corresponds to a given time t > 0. The inverse of that problem is solved fairly simply. Given a point on the trajectory, find the tangent line at that point using derivative formula (2) and deduce time t from the y-intercept b of that line (i.e. from the current "ship" position):
t = b/V (6)
Therefore determining (x(t),y(t)) where the "torpedo" is located at a given time t > 0 is essentially a root-finding exercise. One readily brackets the desired x(t) between two x-coordinates x1 and x2 that correspond to times t1 and t2 such that t1 < t < t2. A root-finding method can be used to refine this interval until the desired accuracy is achieved. Once a fairly small interval has been refined, Newton's method will provide rapid convergence. We can look at the details of such a procedure in a next installment!
I can set up the problem for you but not solve it.
The black curve is moving at a constant velocity v0, and in a straight line.
The blue curve moves at a constant velocity v1 in the direction of black.
For simplicity, choose coordinates so that at time t=0 the black curve starts at (x=0, y=0) and is moving in the direction x.
Thus, at time t >= 0, the position of the black curve is (v0 t, 0).
Problem statement
The goal is to find x, y of the blue curve for times t >= 0 given the initial position (x(t=0), y(t=0)). The differential equations of motion are
dx / dt = v1 (v0 t - x) / a(t)
dy / dt = v1 (- y) / a(t)
where a(t) = sqrt((v0 t - x)^2 + (y^2)) is the distance between blue and black at time t.
This is a system of two nonlinear coupled differential equations. It seems likely that there is no complete anaytical solution. Wolfram Alpha gives up without trying for the input
D[y[t],t] = -y[t] / sqrt[(t-x[t])^2 + y[t]^2], D[x[t],t] = (t-x[t]) / sqrt[(t-x[t])^2 + y[t]^2]
You could try asking on math.stackexchange. Good luck!
I am new to this forum and not a native english speaker, so please be nice! :)
Here is the challenge I face at the moment:
I want to calculate the (approximate) relative coordinates of yet unknown points in a 3D euclidean space based on a set of given distances between 2 points.
In my first approach I want to ignore possible multiple solutions, just taking the first one by random.
e.g.:
given set of distances: (I think its creating a pyramid with a right-angled triangle as a base)
P1-P2-Distance
1-2-30
2-3-40
1-3-50
1-4-60
2-4-60
3-4-60
Step1:
Now, how do I calculate the relative coordinates for those points?
I figured that the first point goes to 0,0,0 so the second one is 30,0,0.
After that the third points can be calculated by finding the crossing of the 2 circles from points 1 and 2 with their distances to point 3 (50 and 40 respectively). How do I do that mathematically? (though I took these simple numbers for an easy representation of the situation in my mind). Besides I do not know how to get to the answer in a correct mathematical way the third point is at 30,40,0 (or 30,0,40 but i will ignore that).
But getting the fourth point is not as easy as that. I thought I have to use 3 spheres in calculate the crossing to get the point, but how do I do that?
Step2:
After I figured out how to calculate this "simple" example I want to use more unknown points... For each point there is minimum 1 given distance to another point to "link" it to the others. If the coords can not be calculated because of its degrees of freedom I want to ignore all possibilities except one I choose randomly, but with respect to the known distances.
Step3:
Now the final stage should be this: Each measured distance is a bit incorrect due to real life situation. So if there are more then 1 distances for a given pair of points the distances are averaged. But due to the imprecise distances there can be a difficulty when determining the exact (relative) location of a point. So I want to average the different possible locations to the "optimal" one.
Can you help me going through my challenge step by step?
You need to use trigonometry - specifically, the 'cosine rule'. This will give you the angles of the triangle, which lets you solve the 3rd and 4th points.
The rules states that
c^2 = a^2 + b^2 - 2abCosC
where a, b and c are the lengths of the sides, and C is the angle opposite side c.
In your case, we want the angle between 1-2 and 1-3 - the angle between the two lines crossing at (0,0,0). It's going to be 90 degrees because you have the 3-4-5 triangle, but let's prove:
50^2 = 30^2 + 40^2 - 2*30*40*CosC
CosC = 0
C = 90 degrees
This is the angle between the lines (0,0,0)-(30,0,0) and (0,0,0)- point 3; extend along that line the length of side 1-3 (which is 50) and you'll get your second point (0,50,0).
Finding your 4th point is slightly trickier. The most straightforward algorithm that I can think of is to firstly find the (x,y) component of the point, and from there the z component is straightforward using Pythagoras'.
Consider that there is a point on the (x,y,0) plane which sits directly 'below' your point 4 - call this point 5. You can now create 3 right-angled triangles 1-5-4, 2-5-4, and 3-5-4.
You know the lengths of 1-4, 2-4 and 3-4. Because these are right triangles, the ratio 1-4 : 2-4 : 3-4 is equal to 1-5 : 2-5 : 3-5. Find the point 5 using trigonometric methods - the 'sine rule' will give you the angles between 1-2 & 1-4, 2-1 and 2-4 etc.
The 'sine rule' states that (in a right triangle)
a / SinA = b / SinB = c / SinC
So for triangle 1-2-4, although you don't know lengths 1-4 and 2-4, you do know the ratio 1-4 : 2-4. Similarly you know the ratios 2-4 : 3-4 and 1-4 : 3-4 in the other triangles.
I'll leave you to solve point 4. Once you have this point, you can easily solve the z component of 4 using pythagoras' - you'll have the sides 1-4, 1-5 and the length 4-5 will be the z component.
I'll initially assume you know the distances between all pairs of points.
As you say, you can choose one point (A) as the origin, orient a second point (B) along the x-axis, and place a third point (C) along the xy-plane. You can solve for the coordinates of C as follows:
given: distances ab, ac, bc
assume
A = (0,0)
B = (ab,0)
C = (x,y) <- solve for x and y, where:
ac^2 = (A-C)^2 = (0-x)^2 + (0-y)^2 = x^2 + y^2
bc^2 = (B-C)^2 = (ab-x)^2 + (0-y)^2 = ab^2 - 2*ab*x + x^2 + y^2
-> bc^2 - ac^2 = ab^2 - 2*ab*x
-> x = (ab^2 + ac^2 - bc^2)/2*ab
-> y = +/- sqrt(ac^2 - x^2)
For this to work accurately, you will want to avoid cases where the points {A,B,C} are in a straight line, or close to it.
Solving for additional points in 3-space is similar -- you can expand the Pythagorean formula for the distance, cancel the quadratic elements, and solve the resulting linear system. However, this does not directly help you with your steps 2 and 3...
Unfortunately, I don't know a well-behaved exact solution for steps 2 and 3, either. Your overall problem will generally be both over-constrained (due to conflicting noisy distances) and under-constrained (due to missing distances).
You could try an iterative solver: start with a random placement of all your points, compare the current distances with the given ones, and use that to adjust your points in such a way as to improve the match. This is an optimization technique, so I would look up books on numerical optimization.
If you know the distance between the nodes (fixed part of system) and the distance to the tag (mobile) you can use trilateration to find the x,y postion.
I have done this using the Nanotron radio modules which have a ranging capability.
I am trying to generate a 3d tube along a spline. I have the coördinates of the spline (x1,y1,z1 - x2,y2,z2 - etc) which you can see in the illustration in yellow. At those points I need to generate circles, whose vertices are to be connected at a later stadium. The circles need to be perpendicular to the 'corners' of two line segments of the spline to form a correct tube. Note that the segments are kept low for illustration purpose.
[apparently I'm not allowed to post images so please view the image at this link]
http://img191.imageshack.us/img191/6863/18720019.jpg
I am as far as being able to calculate the vertices of each ring at each point of the spline, but they are all on the same planar ie same angled. I need them to be rotated according to their 'legs' (which A & B are to C for instance).
I've been thinking this over and thought of the following:
two line segments can be seen as 2 vectors (in illustration A & B)
the corner (in illustraton C) is where a ring of vertices need to be calculated
I need to find the planar on which all of the vertices will reside
I then can use this planar (=vector?) to calculate new vectors from the center point, which is C
and find their x,y,z using radius * sin and cos
However, I'm really confused on the math part of this. I read about the dot product but that returns a scalar which I don't know how to apply in this case.
Can someone point me into the right direction?
[edit]
To give a bit more info on the situation:
I need to construct a buffer of floats, which -in groups of 3- describe vertex positions and will be connected by OpenGL ES, given another buffer with indices to form polygons.
To give shape to the tube, I first created an array of floats, which -in groups of 3- describe control points in 3d space.
Then along with a variable for segment density, I pass these control points to a function that uses these control points to create a CatmullRom spline and returns this in the form of another array of floats which -again in groups of 3- describe vertices of the catmull rom spline.
On each of these vertices, I want to create a ring of vertices which also can differ in density (amount of smoothness / vertices per ring).
All former vertices (control points and those that describe the catmull rom spline) are discarded.
Only the vertices that form the tube rings will be passed to OpenGL, which in turn will connect those to form the final tube.
I am as far as being able to create the catmullrom spline, and create rings at the position of its vertices, however, they are all on a planars that are in the same angle, instead of following the splines path.
[/edit]
Thanks!
Suppose you have a parametric curve such as:
xx[t_] := Sin[t];
yy[t_] := Cos[t];
zz[t_] := t;
Which gives:
The tangent vector to our curve is formed by the derivatives in each direction. In our case
Tg[t_]:= {Cos[t], -Sin[t], 1}
The orthogonal plane to that vector comes solving the implicit equation:
Tg[t].{x - xx[t], y - yy[t], z - zz[t]} == 0
In our case this is:
-t + z + Cos[t] (x - Sin[t]) - (y - Cos[t]) Sin[t] == 0
Now we find a circle in that plane, centered at the curve. i.e:
c[{x_, y_, z_, t_}] := (x - xx[t])^2 + (y - yy[t])^2 + (z - zz[t])^2 == r^2
Solving both equations, you get the equation for the circles:
HTH!
Edit
And by drawing a lot of circles, you may get a (not efficient) tube:
Or with a good Graphics 3D library:
Edit
Since you insist :) here is a program to calculate the circle at junctions.
a = {1, 2, 3}; b = {3, 2, 1}; c = {2, 3, 4};
l1 = Line[{a, b}];
l2 = Line[{b, c}];
k = Cross[(b - a), (c - b)] + b; (*Cross Product*)
angle = -ArcCos[(a - b).(c - b)/(Norm[(a - b)] Norm[(c - b)])]/2;
q = RotationMatrix[angle, k - b].(a - b);
circle[t_] := (k - b)/Norm[k - b] Sin#t + (q)/Norm[q] Cos#t + b;
Show[{Graphics3D[{
Red, l1,
Blue, l2,
Black, Line[{b, k}],
Green, Line[{b, q + b}]}, Axes -> True],
ParametricPlot3D[circle[t], {t, 0, 2 Pi}]}]
Edit
Here you have the mesh constructed by this method. It is not pretty, IMHO:
I don't know what your language of choice is, but if you speak MatLab there are already a few implementations available. Even if you are using another language, some of the code might be clear enough to inspire a reimplementation.
The key point is that if you don't want your tube to twist when you connect the vertices, you cannot determine the basis locally, but need to propagate it along the curve. The Frenet frame, as proposed by jalexiou, is one option but simpler stuff works fine as well.
I did a simple MatLab implementation called tubeplot.m in my formative years (based on a simple non-Frenet propagation), and googling it, I can see that Anders Sandberg from kth.se has done a (re?)implementation with the same name, available at http://www.nada.kth.se/~asa/Ray/Tubeplot/tubeplot.html.
Edit:
The following is pseudocode for the simple implementation in tubeplot.m. I have found it to be quite robust.
The plan is to propagate two normals a and b along the curve, so
that at each point on the curve a, b and the tangent to the curve
will form an orthogonal basis which is "as close as possible" to the
basis used in the previous point.
Using this basis we can find points on the circumference of the tube.
// *** Input/output ***
// v[0]..v[N-1]: Points on your curve as vectors
// No neighbours should overlap
// nvert: Number of vertices around tube, integer.
// rtube: Radius of tube, float.
// xyz: (N, nvert)-array with vertices of the tube as vectors
// *** Initialization ***
// 1: Tangent vectors
for i=1 to N-2:
dv[i]=v[i+1]-v[i-1]
dv[0]=v[1]-v[0], dv[N-1]=v[N-1]-v[N-2]
// 2: An initial value for a (must not be pararllel to dv[0]):
idx=<index of smallest component of abs(dv[0])>
a=[0,0,0], a[idx]=1.0
// *** Loop ***
for i = 0 to N-1:
b=normalize(cross(a,dv[i]));
a=normalize(cross(dv[i],b));
for j = 0 to nvert-1:
th=j*2*pi/nvert
xyz[i,j]=v[i] + cos(th)*rtube*a + sin(th)*rtube*b
Implementation details: You can probably speed up things by precalculating the cos and sin. Also, to get a robust performance, you should fuse input points closer than, say, 0.1*rtube, or a least test that all the dv vectors are non-zero.
HTH
You need to look at Fenet formulas in Differential Geometry. See figure 2.1 for an example with a helix.
Surfaces & Curves
Taking the cross product of the line segment and the up vector will give you a vector at right-angles to them both (unless the line segment points exactly up or down) which I'll call horizontal. Taking the cross product of horizontal and the line segment with give you another vector that's at right angles to the line segment and the other one (let's call it vertical). You can then get the circle coords by lineStart + cos theta * horizontal + sin theta * vertical for theta in 0 - 2Pi.
Edit: To get the points for the mid-point between two segments, use the sum of the two line segment vectors to find the average.
I am writing a physics engine/simulator which incorporates 3D space flight, planetary/stellar gravitation, ship thrust and relativistic effects. So far, it is going very well, however, one thing that I need help with is the math of the collision detection algorithm.
The iterative simulation of movement that I am using is basically as follows:
(Note: 3D Vectors are ALL CAPS.)
For each obj
obj.ACC = Sum(all acceleration influences)
obj.POS = obj.POS + (obj.VEL * dT) + (obj.ACC * dT^2)/2 (*EQ.2*)
obj.VEL = obj.VEL + (obj.ACC * dT)
Next
Where:
obj.ACC is the acceleration vector of the object
obj.POS is the position or location vector of the object
obj.VEL is the velocity vector of the object
obj.Radius is the radius (scalar) of the object
dT is the time delta or increment
What I basically need to do is to find some efficient formula that derives from (EQ.2) above for two objects (obj1, obj2) and tell if they ever collide, and if so, at what time. I need the exact time both so that I can determine if it is in this particular time increment (because acceleration will be different at different time increments) and also so that I can locate the exact position (which I know how to do, given the time)
For this engine, I am modelling all objects as spheres, all this formula/algorithm needs to do is to figure out at what points:
(obj1.POS - obj2.POS).Distance = (obj1.Radius + obj2.Radius)
where .Distance is a positive scalar value. (You can also square both sides if this is easier, to avoid the square root function implicit in the .Distance calculation).
(yes, I am aware of many, many other collision detection questions, however, their solutions all seem to be very particular to their engine and assumptions, and none appear to match my conditions: 3D, spheres, and acceleration applied within the simulation increments. Let me know if I am wrong.)
Some Clarifications:
1) It is not sufficient for me to check for Intersection of the two spheres before and after the time increment. In many cases their velocities and position changes will far exceed their radii.
2) RE: efficiency, I do not need help (at this point anyway) with respect to determine likely candidates for collisions, I think that I have that covered.
Another clarification, which seems to be coming up a lot:
3) My equation (EQ.2) of incremental movement is a quadratic equation that applies both Velocity and Acceleration:
obj.POS = obj.POS + (obj.VEL * dT) + (obj.ACC * dT^2)/2
In the physics engines that I have seen, (and certainly every game engine that I ever heard of) only linear equations of incremental movement that apply only Velocity:
obj.POS = obj.POS + (obj.VEL * dT)
This is why I cannot use the commonly published solutions for collision detection found on StackOverflow, on Wikipedia and all over the Web, such as finding the intersection/closest approach of two line segments. My simulation deals with variable accelerations that are fundamental to the results, so what I need is the intersection/closest approach of two parabolic segments.
On the webpage AShelley referred to, the Closest Point of Approach method is developed for the case of two objects moving at constant velocity. However, I believe the same vector-calculus method can be used to derive a result in the case of two objects both moving with constant non-zero acceleration (quadratic time dependence).
In this case, the time derivative of the distance-squared function is 3rd order (cubic) instead of 1st order. Therefore there will be 3 solutions to the Time of Closest Approach, which is not surprising since the path of both objects is curved so multiple intersections are possible. For this application, you would probably want to use the earliest value of t which is within the interval defined by the current simulation step (if such a time exists).
I worked out the derivative equation which should give the times of closest approach:
0 = |D_ACC|^2 * t^3 + 3 * dot(D_ACC, D_VEL) * t^2 + 2 * [ |D_VEL|^2 + dot(D_POS, D_ACC) ] * t + 2 * dot(D_POS, D_VEL)
where:
D_ACC = ob1.ACC-obj2.ACC
D_VEL = ob1.VEL-obj2.VEL (before update)
D_POS = ob1.POS-obj2.POS (also before update)
and dot(A, B) = A.x*B.x + A.y*B.y + A.z*B.z
(Note that the square of the magnitude |A|^2 can be computed using dot(A, A))
To solve this for t, you'll probably need to use formulas like the ones found on Wikipedia.
Of course, this will only give you the moment of closest approach. You will need to test the distance at this moment (using something like Eq. 2). If it is greater than (obj1.Radius + obj2.Radius), it can be disregarded (i.e. no collision). However, if the distance is less, that means the spheres collide before this moment. You could then use an iterative search to test the distance at earlier times. It might also be possible to come up with another (even more complicated) derivation which takes the size into account, or possible to find some other analytic solution, without resorting to iterative solving.
Edit: because of the higher order, some of the solutions to the equation are actually moments of farthest separation. I believe in all cases either 1 of the 3 solutions or 2 of the 3 solutions will be a time of farthest separation. You can test analytically whether you're at a min or a max by evaluating the second derivative with respect to time (at the values of t which you found by setting the first derivative to zero):
D''(t) = 3 * |D_ACC|^2 * t^2 + 6 * dot(D_ACC, D_VEL) * t + 2 * [ |D_VEL|^2 + dot(D_POS, D_ACC) ]
If the second derivative evaluates to a positive number, then you know the distance is at a minimum, not a maximum, for the given time t.
Draw a line between the start location and end location of each sphere. If the resulting line segments intersect the spheres definitely collided at some point and some clever math can find at what time the collision occurred. Also make sure to check if the minimum distance between the segments (if they don't intersect) is ever less than 2*radius. This will also indicate a collision.
From there you can backstep your delta time to happen exactly at collision so you can correctly calculate the forces.
Have you considered using a physics library which already does this work? Many libraries use far more advanced and more stable (better integrators) systems for solving the systems of equations you're working with. Bullet Physics comes to mind.
op asked for time of collision. A slightly different approach will compute it exactly...
Remember that the position projection equation is:
NEW_POS=POS+VEL*t+(ACC*t^2)/2
If we replace POS with D_POS=POS_A-POS_B, VEL with D_VEL=VEL_A-VEL_B, and ACC=ACC_A-ACC_B for objects A and B we get:
$D_NEW_POS=D_POS+D_VEL*t+(D_ACC*t^2)/2
This is the formula for vectored distance between the objects. In order to get the squared scalar distance between them, we can take the square of this equation, which after expansion looks like:
distsq(t) = D_POS^2+2*dot(D_POS,D_VEL)*t + (dot(D_POS, D_ACC)+D_VEL^2)*t^2 + dot(D_VEL,D_ACC)*t^3 + D_ACC^2*t^4/4
In order to find the time where collision occurs, we can set the equation equal to the square of the sum of radii and solve for t:
0 = D_POS^2-(r_A+r_B)^2 + 2*dot(D_POS,D_VEL)*t + (dot(D_POS, D_ACC)+D_VEL^2)*t^2 + dot(D_VEL,D_ACC)*t^3 + D_ACC^2*t^4/4
Now, we can solve for the equation using the quartic formula.
The quartic formula will yield 4 roots, but we are only interested in real roots. If there is a double real root, then the two objects touch edges at exactly one point in time. If there are two real roots, then the objects continuously overlap between root 1 and root 2 (i.e. root 1 is the time when collision starts and root 2 is the time when collision stops). Four real roots means that the objects collide twice, continuously between root pairs 1,2 and 3,4.
In R, I used polyroot() to solve as follows:
# initial positions
POS_A=matrix(c(0,0),2,1)
POS_B=matrix(c(2,0),2,1)
# initial velocities
VEL_A=matrix(c(sqrt(2)/2,sqrt(2)/2),2,1)
VEL_B=matrix(c(-sqrt(2)/2,sqrt(2)/2),2,1)
# acceleration
ACC_A=matrix(c(sqrt(2)/2,sqrt(2)/2),2,1)
ACC_B=matrix(c(0,0),2,1)
# radii
r_A=.25
r_B=.25
# deltas
D_POS=POS_B-POS_A
D_VEL=VEL_B-VEL_A
D_ACC=ACC_B-ACC_A
# quartic coefficients
z=c(t(D_POS)%*%D_POS-r*r, 2*t(D_POS)%*%D_VEL, t(D_VEL)%*%D_VEL+t(D_POS)%*%D_ACC, t(D_ACC)%*%D_VEL, .25*(t(D_ACC)%*%D_ACC))
# get roots
roots=polyroot(z)
# In this case there are only two real roots...
root1=as.numeric(roots[1])
root2=as.numeric(roots[2])
# trajectory over time
pos=function(p,v,a,t){
T=t(matrix(t,length(t),2))
return(t(matrix(p,2,length(t))+matrix(v,2,length(t))*T+.5*matrix(a,2,length(t))*T*T))
}
# plot A in red and B in blue
t=seq(0,2,by=.1) # from 0 to 2 seconds.
a1=pos(POS_A,VEL_A,ACC_A,t)
a2=pos(POS_B,VEL_B,ACC_B,t)
plot(a1,type='o',col='red')
lines(a2,type='o',col='blue')
# points of a circle with center 'p' and radius 'r'
circle=function(p,r,s=36){
e=matrix(0,s+1,2)
for(i in 1:s){
e[i,1]=cos(2*pi*(1/s)*i)*r+p[1]
e[i,2]=sin(2*pi*(1/s)*i)*r+p[2]
}
e[s+1,]=e[1,]
return(e)
}
# plot circles with radius r_A and r_B at time of collision start in black
lines(circle(pos(POS_A,VEL_A,ACC_A,root1),r_A))
lines(circle(pos(POS_B,VEL_B,ACC_B,root1),r_B))
# plot circles with radius r_A and r_B at time of collision stop in gray
lines(circle(pos(POS_A,VEL_A,ACC_A,root2),r_A),col='gray')
lines(circle(pos(POS_B,VEL_B,ACC_B,root2),r_B),col='gray')
Object A follows the red trajectory from the lower left to the upper right. Object B follows the blue trajectory from the lower right to the upper left. The two objects collide continuously between time 0.9194381 and time 1.167549. The two black circles just touch, showing the beginning of overlap - and overlap continues in time until the objects reach the location of the gray circles.
Seems like you want the Closest Point of Approach (CPA). If it is less than the sum of the radiuses, you have a collision. There is example code in the link. You can calculate each frame with the current velocity, and check if the CPA time is less than your tick size. You could even cache the cpa time, and only update when acceleration was applied to either item.