  We report an abundance analysis for the highly r-process-enhanced (r-II) star
CS 29497-004, a very metal-poor giant with Teff = 5013K and [Fe/H]=-2.85, whose
nature was initially discovered in the course of the HERES project. Our
analysis is based on high signal-to-noise, high-resolution (R~75000) VLT/UVES
spectra and MARCS model atmospheres under the assumption of local thermodynamic
equilibrium, and obtains abundance measurements for a total of 46 elements, 31
of which are neutron-capture elements. As is the case for the other 25 r-II
stars currently known, the heavy-element abundance pattern of CS 29497-004
well-matches a scaled Solar System second peak r-process-element abundance
pattern. We confirm our previous detection of Th, and demonstrate that this
star does not exhibit an "actinide boost". Uranium is also detected (log e(U)
=-2.20+/-0.30), albeit with a large measurement error that hampers its use as a
precision cosmo-chronometer. Combining the various elemental chronometer pairs
that are available for this star, we derive a mean age of 12.2+/-3.7 Gyr using
the theoretical production ratios from waiting-point approximation models
(Kratz et al. 2007). We further explore the high-entropy wind model (Farouqi et
al. 2010) production ratios arising from different neutron richness of the
ejecta (Y_e), and derive an age of 13.7+/-4.4 Gyr for a best-fitting Y_e=0.447.
The U/Th nuclei-chronometer is confirmed to be the most resilient to
theoretical production ratios and yields an age of 16.5+:-6.6 Gyr. Lead (Pb) is
also tentatively detected in CS 29497-004, at a level compatible with a scaled
Solar r-process, or with the theoretical expectations for a pure r-process in
this star.
