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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 465, Issue 4, pp. 4099 - 4105
The Hoffmeister family is a C-type group located in the central main belt. Dynamically, it is important because of its interaction with the nu(1C) nodal... 
Minor planets | Asteroids: individual: Hoffmeister | Celestialmechanics | Asteroids: general | PALLAS | minor planets, asteroids: individual: Hoffmeister | celestial mechanics | minor planets, asteroids: general | ASTRONOMY & ASTROPHYSICS | Physics - Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2016, Volume 458, Issue 1, pp. 1117 - 1126
Ceres is the largest and most massive body in the asteroid main belt. Observational data from the Dawn spacecraft reveal the presence of at least two impact... 
Minor planets, asteroids: individual: ceres | Celestialmechanics | Minor planets, asteroids: general | celestial mechanics | minor planets, asteroids: general | EVOLUTION | minor planets, asteroids: individual: Ceres | ASTRONOMY & ASTROPHYSICS | Physics - Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2015, Volume 450, Issue 4, pp. 3742 - 3749
In the last two decades, new computational tools have been developed in order to aid space missions to orbit around irregular small bodies. One of the... 
Gravitation | Minor planets, asteroids: general | Celestialmechanics | Methods: numerical | DENSITY | celestial mechanics | minor planets, asteroids: general | gravitation | methods: numerical | ASTRONOMY & ASTROPHYSICS | Space Physics | Physics | Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 06/2018, Volume 477, Issue 1, pp. 1308 - 1317
The Nele group, formerly known as the Iannini family, is one of the youngest asteroid families in the main belt. Previously, it has been noted that the... 
DENSITY | minor planets, asteroids: general | celestial mechanics | BELT | minor planets, asteroids: individual: Nele | ASTRONOMY & ASTROPHYSICS | Physics - Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 4, pp. 3731 - 3738
Asteroid families are groups of minor bodies produced by high-velocity collisions. After the initial dispersions of the parent bodies fragments, their orbits... 
Minor planets, asteroids: General | Celestial mechanics | celestial mechanics | minor planets, asteroids: general | CHRONOLOGY | SEARCH | DYNAMICAL EVOLUTION | ASTRONOMY & ASTROPHYSICS | PALLAS | EROSION | REGION | Physics - Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
Icarus, ISSN 0019-1035, 06/2016, Volume 271, pp. 57 - 66
•We identified the Koronis family in the domain of proper elements and used SDSS-MOC4 and WISE data to identify members of the Koronis halo.•We studied how the... 
Asteroids, dynamics | Asteroids | Celestial mechanics | ASTEROID SPECTROSCOPIC SURVEY | BELT | ASTRONOMY & ASTROPHYSICS | PHASE-II | Orbits | Escape velocity | Dynamics | Parents | Fragments | Estimates | Inclination | Ejection | Physics - Earth and Planetary Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2015, Volume 451, Issue 1, pp. 244 - 256
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2017, Volume 470, Issue 3, pp. 2687 - 2701
Here, we study the dynamical effects of the solar radiation pressure (SRP) on a spacecraft that will survey the near-Earth rotating asteroid (101955) Bennu... 
Gravitation | Celestialmechanics | Minor planets, asteroids: individual: Bennu | Methods: numerical | gravitation | STABILITY | ASTRONOMY & ASTROPHYSICS | ENVIRONMENT | celestialmechanics | 433 EROS | minor planets, asteroids: individual: Bennu | MODEL | methods: numerical | Physics - Space Physics | Physics | Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2017, Volume 467, Issue 1, pp. 1016 - 1023
The Rafita asteroid family is an S-type group located in the middle main belt, on the righthand side of the 3J:-1A mean-motion resonance. The proximity of this... 
MASSIVE ASTEROIDS | ORIGIN | celestial mechanics | minor planets, asteroids: general | BELT | BEHAVIOR | ASTRONOMY & ASTROPHYSICS | DYNAMICS | PHASE-II | CLOSE ENCOUNTERS | SPECTROSCOPIC SURVEY | Physics - Space Physics | Physics | Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 01/2017, Volume 464, Issue 3, pp. 3552 - 3560
One of the most accurate models currently used to represent the gravity field of irregular bodies is the polyhedral approach. In this model, the mass of the... 
TARGET | 21-LUTETIA | SMALL BODIES | ROTATING 2ND-DEGREE | VESTA | EQUILIBRIUM POINTS | PERIODIC-ORBITS | celestial mechanics | gravitation | ORDER GRAVITY FIELDS | ASTRONOMY & ASTROPHYSICS | ROSETTA MISSION | 433 EROS | minor planets, asteroids: individual: Lutetia | Physics - Earth and Planetary Astrophysics | Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2010, Volume 515, p. A9
Context. The precise and accurate modelling of a terrestrial planet like Venus is an exciting and challenging topic, all the more interesting because it can be... 
Planets and satellites: individual: Venus | Celestial mechanics | EARTH | EVOLUTION | RADAR | SPIN | ASTRONOMY & ASTROPHYSICS | Physics - Earth and Planetary Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2016, Volume 455, pp. 2279 - 2288
The Erigone family is a C-type group in the inner main belt. Its age has been estimated by several researchers to be less then 300 Myr, so it is a relatively... 
Analytical chemistry | Chemical Sciences
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2018, Volume 481, Issue 2, pp. 1707 - 1717
We discuss the asteroid population evolving close by or into the ν 6 secular resonance in the main asteroid belt. Using the analytical method of Yoshikawa, we... 
Astrophysics | Physics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2016, Volume 463, pp. 705 - 711
$v_W$ leptokurtic asteroid families are families for which the distribution of the normal component of the terminal ejection velocity field $v_W$ is... 
Physics - Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 07/2017, Volume 468, Issue 4, pp. 4982 - 4991
Non-linear secular resonances of g-type, i.e. involving the frequency of precession g of the asteroid pericentre, can affect the proper eccentricities of... 
minor planets, asteroids: general | celestial mechanics | FAMILIES | ASTRONOMY & ASTROPHYSICS | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2019, Volume 486, Issue 2, pp. 2557 - 2569
The main goal of our work is to study the orbital dynamics of a spacecraft near the (87) Sylvia system. Here, we consider a non-homogeneous mass distribution... 
gravitation | minor planets, asteroids: individual: Sylvia | celestial mechanics | ENVIRONMENT | SIZE | EQUILIBRIUM POINTS | MAIN-BELT ASTEROIDS | ORIGIN | SHAPE | MOTION | MODELS | ASTRONOMY & ASTROPHYSICS | SATELLITES | Sciences of the Universe | Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. A39
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 471, Issue 4, pp. 4820 - 4826
The Maria asteroid family is a group of S-type asteroids. Its location adjacent to the left side of the 3J:-1A mean-motion resonances could be the reason for... 
Minor planets | Gravitation | Asteroids: general | Celestial mechanics | celestial mechanics | minor planets, asteroids: general | CHRONOLOGY | gravitation | DIGITAL SKY SURVEY | MAIN BELT | ASTRONOMY & ASTROPHYSICS | OBJECTS | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2015, Volume 455, pp. 2279 - 2288
The Erigone family is a C-type group in the inner main belt. Its age has been estimated by several researchers to be less then 300 My, so it is a relatively... 
Physics - Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
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