1. Bivalve shells also fit in this scheme, for example the Softshell Clam Mya arenaria can be modeled as follows.


v=2.5, c=3, a=0.85, b=1.6, h=0.9, k=0, t=0.52..0.52 
Experiment with modeling other bivalves, for example mussels and scallops.
2. If you live near a beach, try identifying shells and modeling them. Otherwise "Nature" stores often have inexpensive but interesting shells for sale.
3. Why is it that a helically coiled shell fits exactly inside a cone?
4. The 9 parameters we use (v, c, a, b, h, k and the beginning and end of the t range) are certainly too many.
Can 3 be enough, as in the Raup video? Think of ways to simplify the set of parameters.
5. Suppose we are down to a set of m parameters. The set of all possible parameter values is then a subset M of R^{m}.
Not every point of M corresponds to the coordinates of an organism. Is there some way to understand which regions of M are forbidden, and why?
6. For a fairly elementary treatment of the 3dimensional rotation group and its subgroups you may consult the beginning of Anthony Knapp's Lie Groups, Lie Algebras, and Cohomology, Princeton University Press, 1988. This is elementary for graduate students.
The point is first to understand why the dilation equation
implies D_{h}(x,y,z) = e^{vh}(x,y,z). We know that since D_{h} is a dilation it must correspond to multiplication by some function f(h).
Since we are assuming a smooth dependence on the parameter h, we can calculate the derivative of f : f'(h)= lim_{a>0} (f(h+a)f(h))/a.
The dilation equation gives f(h+a)=f(h)f(a), so
f'(h)= lim_{a>0} (f(h+a)f(h))/a = lim_{a>0} f(h)(f(a)1)/a = v f(h), where v = lim_{a>0}(f(a)1)/a.
The initial value problem f'(h)=v f(h), f(0)=1 has the unique solution f(h)= e^{vh}.
What happens to the rotations is more complicated but completely analogous. Once we choose coordinates, R_{h} is a 3x3 matrix whose entries vary smoothly with h.The rotation equation is
R'_{t} = lim_{a>0} (R_{(t+a)}R_{t})/a = lim_{a>0} R_{t}(R_{a}I)/a = R_{t}r, where r is the matrix lim_{a>0}(R_{a}I)/a.
Now we have the matrix differential equation R'_{t} = R_{t}r , R_{0}= I.There is an exponential map exp for matrices defined by the same power series as the usual exponential. In terms of this map our equation has the unique solution R_{t} = exp(tr).
Finally one needs to know that the possible matrices r form a vector space spanned by
$$ \left[ \begin{array} {rrr}0 &1 & 0\\ 1 & 0 & 0 \\ 0 &0 & 0\\ \end{array} \right] , \left[ \begin{array} {rrr}0 & 0 & 1\\ 0 & 0 & 0 \\ 1 &0 & 0\\ \end{array} \right] , \left[ \begin{array}{rrr} 0 & 0 & 0\\ 0 & 0 & 1 \\ 0 &1 & 0\\ \end{array} \right] . $$(this is a consequence of the the R_{t} being matrices of rotations) and that we can choose our (x,y,z)coordinates so that
$$ \left[ \begin{array} {ccc}0 &c & 0\\ c & 0 & 0 \\ 0 &0 & 0\\ \end{array} \right] . $$Then it is easy and sort of fun to check explicitly that
$$R_{t} = \exp(tr)= \left[ \begin{array} {ccc}\cos(ct) &\sin(ct) & 0\\ \sin(ct) & \cos(ct) & 0 \\ 0 &0 & 1\\ \end{array} \right] .$$