Young massive clusters (YMCs) are dense aggregates of young stars that form the
fundamental building blocks of galaxies. Several examples exist in the Milky Way Galaxy …

Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows
that are subject to dissipative processes. The spin and orbital motions undergo a coupled …

Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of
planetary formation and evolution. The wealth of photons from the host star gives detailed …

Saturn is orbited by dozens of moons, and the intricate dynamics of this complex system
provide clues about its formation and evolution. Tidal friction within Saturn causes its moons …

▪ Abstract We know that giant planets played a crucial role in the making of our Solar
System. The discovery of giant planets orbiting other stars is a formidable opportunity to …

Io is the volcanically most active body in the Solar System and has a large surface heat flux,,.
The geological activity is thought to be the result of tides raised by Jupiter, but it is not known …

The inner moons of Jupiter and Saturn migrate outwards due to tidal energy dissipation
within the planets, the details of which remain poorly understood. We demonstrate that …

We present the discovery of KELT-1b, the first transiting low-mass companion from the wide-
field Kilodegree Extremely Little Telescope-North (KELT-North) transit survey. A joint …

The distribution of eccentricities e of extrasolar planets with semimajor axes a> 0.2 AU is
very uniform, and values for e are relatively large, averaging 0.3 and broadly distributed up …

Context. Ultra-short period planets undergo strong tidal interactions with their host star which
lead to planet deformation and orbital tidal decay. Aims. WASP-103b is the exoplanet with …