Chaotic dynamical systems are characterized by the existence of a predictability horizon, connected to the notion of Lyapunov time, beyond which predictions of the state of the system are meaningless. In order to study the main features of orbit determination in presence of chaos, Spoto and Milani (2016) applied the classical least squares fit...
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2018 (v1)Journal articleUploaded on: December 4, 2022
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March 25, 2019 (v1)Conference paper
National audience
Uploaded on: December 3, 2022 -
July 14, 2018 (v1)Conference paper
Knowing the asteroid belt is the key to provide a reliable history ofour solar system. The main question which has been raised in the lastyears is: given our available data, does our classification ofasteroid into families provide a reliable history of the collisionalevolution of our solar system?We have done huge steps forward, but the real...
Uploaded on: December 3, 2022 -
October 15, 2017 (v1)Conference paper
The first data release of star astrometry by Gaia (Sept. 2016) has given an anticipation of the mission capabilities. By providing positions with uncertainties at the level of few milli-arcsec (mas) a new frame to calibrate ground-based observations has immediately become available, thus disclosing a new possibility of exploitation for archive...
Uploaded on: December 3, 2022 -
October 15, 2017 (v1)Conference paper
Since October 2016, the short term (ST) processing of Solar System Objects (SSOs) by Gaia is up and running, and it has produced almost 600 alerts. A crucial point in the chain is the possibility of performing a short arc orbit determination as soon as the object has been detected, which allows the follow up of the object from the ground.The...
Uploaded on: December 3, 2022 -
September 15, 2019 (v1)Conference paper
Gaia, the billion of stars surveyor, also regularly observe small bodies from our Solar System. Among those, some are not known at the time of their observation by Gaia. Within the Data Processing and Analysis Consortium, a daily processing as been set in place to release information on when, where, and how to observe these potential...
Uploaded on: December 4, 2022 -
December 2018 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
October 16, 2016 (v1)Conference paper
The Gaia ESA space mission will provide astrometric observations of a large number of celestial bodies, with unprecedented accuracy, and in an homogenous reference frame (to become the optical ICRF). The Gaia satellite is monitoring regularly the whole celestial sphere, with one complete scan in about 6month, down to approximately magnitude...
Uploaded on: December 3, 2022