Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …

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 …

We report new optical constants (refractive index, n, and extinction coefficient, k) for
exoplanet haze analogs from 0.3 to 30 µm. The samples were produced in a simulated N 2 …

Formation of C–N containing compounds from plasma-catalytic coupling of CH4 and N2
over various transition metals (Ni, Pd, Cu, Ag, and Au) is investigated using a multimodal …

In view of the existing controversy around the origin of the photosynthesis and, therefore, the
first photosynthetic pigments, our work focuses on the theoretical study of a hypothetical first …

Hydrogen cyanide (HCN)-derived molecules and polymers are featured in several
hypotheses on the origin of life. Over half a century of investigations into HCN self-reactions …

In this work, we present for the first time infrared spectra of Titan from the Spitzer Space
Telescope (2004–2009). The data are from both the short wavelength–low resolution (SL; …

The localized delivery of new long-lived species to Jupiter's stratosphere by comet
Shoemaker–Levy 9 in 1994 opened a window to constrain Jovian chemistry and dynamics …

The isotopically enriched cyanide anion,(13C≡ 15N)−, has a great potential as the NMR
probe of non-covalent interactions. However, hydrogen cyanide is highly toxic and can …

Human space exploration is crucial for our future beyond Earth, offering vital insights while
overcoming challenges. Unmanned missions are predominant due to the harsh conditions …