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U and Th content in the Central Apennines continental crust: a contribution to the determination of the geo-neutrinos flux at LNGS

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Ultra-Low Delta-v Objects and the Human Exploration of Asteroids

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Ultraviolet and visible photometry of asteroid (21) Lutetia using the Hubble Space Telescope

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Ultraviolet Spectroscopy of Asteroid (4) Vesta

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Unbiased Inclination Distributions for Objects in the Kuiper Belt

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Unbound or Distant Planetary Mass Population Detected by Gravitational Microlensing

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Undisturbed Mesosphere Optical Properties from Wide-Angle Frequent Twilight Sky Polarimetry

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Unprecedented accurate abundances: signatures of other Earths?

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Unstable Planetary Systems Emerging Out Of Gas Disks

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Upper limits for undetected trace species in the stratosphere of Titan

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Upper Limits on the Number of Small Bodies in Sedna-Like Orbits by the TAOS Project

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Upsilon Andromedae b in polarized light: New constraints on the planet size, density and albedo

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Uranus and Neptune: Shape and Rotation

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Using Kepler transit observations to measure stellar spot belt migration rates

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Using Kuiper Belt Binaries to Constrain Neptune's Migration History

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Using Satellites to Probe Extrasolar Planet Formation

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
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Using Star Spots to Measure the Spin-orbit Alignment of Transiting Planets

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Using Stellar Densities to Evaluate Transiting Exoplanetary Candidates

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Using the Sun to estimate Earth-like planets detection capabilities II. Impact of plages

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Using the Sun to estimate Earth-like planets detection capabilities.I. Impact of cold spots

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