The primary volatile 'rock-forming'minerals in the icy satellites of the outer solar system
include water-ice and various hydrated crystals of methane and ammonia. The rich …

The origin of methane at the present surface of Titan is modeled in light of new high-
pressure phase diagrams of ammonia-water compounds and clathrate hydrate. Using …

Icy satellites exhibit an amazing variety of terrains, many of which were formed by extrusions
of aqueous solutions. Aqueous ammonia has been implicated on the basis of theoretical …

In a multifaceted investigation combining local soft X-ray and vibrational spectroscopic
probes with ab initio molecular dynamics simulations, hydrogen-bonding interactions of two …

Remote sensing of icy objects in the outer solar system relies upon availability of
appropriate laboratory measurements. Surface deposits of specific substances often provide …

We present the first reported adaptive optics spectra of Charon in the H and K bands, which
examine the anti-Pluto and sub-Pluto hemispheres. The ice temperature is estimated at 40 …

Although water-and ammonia-ices have been observed or postulated as important
components of the icy surfaces of planetary satellites in the outer Solar System, significant …

From a variety of sources in the literature and from recent, unpublished, high‐spectral‐
resolution data, we can now piece together spectra of both leading and trailing hemispheres …

An equation of state for ammonia-water liquid has been calculated by least-squares fit for
the following range of parameters: 0 to 100 wt% NH3, 170 to 300° K, and 0 to 10 kb …

Half a century ago, Christian Junge, the founding 'father'of atmospheric chemistry
summarized the existing knowledge in his field of research. In 1960 Junge counted only 75 …