Publications by authors named "Emilio Molinari"

The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot Jupiters) have been probed for nearly two decades. They allow us to investigate the chemical and physical properties of planetary atmospheres under extreme irradiation conditions. Previous observations of hot Jupiters as they transit in front of their host stars have revealed the frequent presence of water vapour and carbon monoxide in their atmospheres; this has been studied in terms of scaled solar composition under the usual assumption of chemical equilibrium.

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Article Synopsis
  • To understand exoplanet formation, knowing their chemical composition is key, especially for ultrahot Jupiters like KELT-9b, which have high equilibrium temperatures around 4,050 K.
  • Observations of KELT-9b's atmosphere revealed the presence of neutral and singly ionized iron and titanium, marking the first detection of iron in an exoplanet.
  • These findings can help refine theories of planetary formation by analyzing the atmospheric chemistry of ultrahot Jupiters, which are expected to be nearly cloud-free and in chemical equilibrium.
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Recent analyses of data from the NASA Kepler spacecraft have established that planets with radii within 25 per cent of the Earth's (R Earth symbol) are commonplace throughout the Galaxy, orbiting at least 16.5 per cent of Sun-like stars. Because these studies were sensitive to the sizes of the planets but not their masses, the question remains whether these Earth-sized planets are indeed similar to the Earth in bulk composition.

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Mechanical flexure is a source of major failures in astronomical spectrographs, for which the reimaging of a focal-plane pinhole has to be maintained in position within a fraction of a CCD pixel that has dimensions of the order of 15 microm. The d.o.

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