The detection of benzene in Titan's atmosphere led to the emergence of polycyclic aromatic
hydrocarbons (PAHs) as potential nucleation agents triggering the growth of Titan's orange …

In this review I summarize the current state of knowledge about the composition of Titan's
atmosphere and our current understanding of the suggested chemistry that leads to that …

Photochemical hazes are important opacity sources in temperate exoplanet atmospheres,
hindering current observations from characterizing exoplanet atmospheric compositions …

The observed mass–radius relationship of low-mass planets informs our understanding of
their composition and evolution. Recent discoveries of low-mass, large-radius objects (" …

UV radiation can induce photochemical processes in exoplanet atmospheres and produce
haze particles. Recent observations suggest that haze and/or cloud layers could be present …

Very little experimental work has been done to explore the properties of photochemical
hazes formed in atmospheres with very different compositions or temperatures than those of …

The photochemical haze produced in the upper atmosphere of Titan plays a key role in
various atmospheric and surface processes on Titan. The surface energy, one important …

Titan, the biggest moon of Saturn, has a thick atmosphere which presents similarities with
the one thought to be on Earth at its beginning. The study of Titan's photochemical haze is …

New observing capabilities coming online over the next few years will provide opportunities
for characterization of exoplanet atmospheres. However, clouds/hazes could be present in …

Photochemistry induced by stellar UV flux should produce haze particles in exoplanet
atmospheres. Recent observations indicate that haze and/or cloud layers exist in the …