This paper aims to assess the potential and requirements of photovoltaic arrays to provide
energy for more than 30 mission types to explore 14 celestial bodies in our solar system …

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 …

The Cassini‐Huygens probe gas chromatograph mass spectrometer (GCMS) determined
the composition of the Titan atmosphere from∼ 140 km altitude to the surface. After landing …

This work reviews factors which are important for the evolution of habitable Earth-like
planets such as the effects of the host star dependent radiation and particle fluxes on the …

Aims. We present the results of several multi-station Very Long Baseline Interferometry
(VLBI) experiments conducted with the ESA spacecraft Venus Express as a target. To …

Enceladus is one of the most remarkable satellites in the solar system, as revealed by
Cassini's detection of active plumes erupting from warm fractures near its south pole. This …

Titan organic haze analogues, or “tholins,” produce biomolecules when hydrolyzed at low
temperature over long timescales. By using a combination of high-resolution mass …

The entry of the Cassini-Huygens spacecraft into orbit around Saturn in July 2004 marked
the start of a golden era in the exploration of Titan, Saturn's giant moon. During the Prime …

Titan, the largest satellite of Saturn, is the only one in the solar system with a dense
atmosphere. Mainly composed of dinitrogen with several% of methane, this atmosphere …

Titan's moment of inertia (MoI), estimated from the quadrupole gravity field measured by the
Cassini spacecraft, is 0.342, which has been interpreted as evidence of a partially …