  The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) has been
observing gamma-ray lines from the Sun and the Galaxy since its launch in
February 2002. Here I summarize the status of RHESSI observations of solar
lines (nuclear de-excitation, neutron capture, and positron annihilation), the
lines of $^{26}$Al and $^{60}$Fe from the inner Galaxy, and the search for
positron annihilation in novae.
