JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs

We present \textit{JWST} images of the well-known planetary nebula NGC\,6720 (the Ring Nebula), covering wavelengths from 1.6$\mu$m to 25 $\mu$m. The bright shell is strongly fragmented with some 20\,000 dense globules, bright in H$_2$, with a characteristic diameter of 0.2~arcsec and density $n_{\rm H} \sim 10^5$--$10^6$\,cm$^{-3}$. The shell contains a thin ring of polycyclic aromatic hydrocarbon (PAH) emission. H$_2$ is found throughout the shell and in the halo. H$_2$ in the halo may be located on the swept-up walls of a biconal polar flow. The central cavity is shown to be filled with high ionization gas and shows two linear structures. The central star is located 2~arcsec from the emission centroid of the cavity and shell. Linear features (`spikes') extend outward from the ring, pointing away from the central star. Hydrodynamical simulations are shown which reproduce the clumping and possibly the spikes. Around ten low-contrast, regularly spaced concentric arc-like features are present; they suggest orbital modulation by a low-mass companion with a period of about 280~yr A previously known much wider companion is located at a projected separation of about 15\,000~au; we show that it is an M2--M4 dwarf. The system is therefore a triple star. These features, including the multiplicity, are similar to those seen in the Southern Ring Nebula (NGC\,3132) and may be a common aspect of such nebulae.