35 citations · 322 across the 28 of their papers we have counts for
25 papers · 1 filter
Extracting Asteroid Physical Properties from Vera C. Rubin Observatory Science Validation Survey Data: Rotational Periods, Colors, and Taxonomies
V. Carruba, S. Greenstreet, M. Mastropietro +7
The Vera C. Rubin Observatory will enable large-scale characterization of minor bodies through high-cadence, multi-band photometry. Early Science Validation (SV) observations from…
GravDyn: A Python Framework for Gravitational Modeling of Irregular Celestial Bodies Using Polyhedral, mascon, and Series Expansion Methods
Safwan Aljbaae, valerio Carruba, Allan K. de Almeida +4
GravDyn is an open-source Python package for computing gravitational potentials and accelerations around irregular celestial bodies. It implements three approaches within the same…
The invisible threat: assessing the collisional hazard posed by the undiscovered Venus co-orbital asteroids
V. Carruba, R. Sfair, R. A. Araujo +7
Currently, 20 co-orbital asteroids of Venus are known, with only one with an eccentricity below 0.38. This is most likely caused by observational biases since asteroids with larger…
Main belt asteroids taxonomical information from Dark Energy Survey data
Valerio Carruba, Júlio I. B. Camargo, Safwan Aljbaae +2
While proper orbital elements are currently available for more than 1 million asteroids, taxonomical information is still lagging behind. Surveys like SDSS-MOC4 provided preliminar…
Dynamics Around an Asteroid Modeled as a Mass Tripole
L. B. T. Santos, L. O. Marchi, P. A. Sousa-Silva +3
The orbital dynamics of a spacecraft orbiting around irregular small celestial bodies is a challenging problem. Difficulties to model the gravity field of these bodies arise from t…
Numerical investigations of the orbital dynamics around a synchronous binary system of asteroids
L. B. T. Santos, Allan Kardec de Almeida, P. A. Sousa-Silva +5
In this article, equilibrium points and families of periodic orbits in the vicinity of the collinear equilibrium points of a binary asteroid system are investigated with respect to…
Analysis of the dynamics of a spacecraft in the vicinity of an asteroid binary system with equal masses
L. B. T. Santos, P. A. Sousa-Silva, M. O. Terra +8
In this work, we performed a dynamical analysis of a spacecraft around a nearly equal-mass binary near-Earth asteroid with application to the asteroid 2017 YE5, which is also a pos…
Optimization of Artificial Neural Networks models applied to the identification of images of asteroids' resonant arguments
Valerio Carruba, Safwan Aljbaae, Gabriel Caritá +2
The asteroidal main belt is crossed by a web of mean-motion and secular resonances, that occur when there is a commensurability between fundamental frequencies of the asteroids and…
Identifying the population of stable resonant asteroids using large databases
Valerio Carruba, Safwan Aljbaae, Rita de Cassia Domingos +2
Large observational surveys, like those that will be conducted at the Vera C. Rubin Observatory, are expected to discover up to one million new asteroids in the first year of opera…
A Particle-Linkage Model for Elongated Asteroids with Three-Dimensional Mass Distribution
Leonardo B. T. Santos, Luis. O. Marchi, Aljbaae Safwan +3
The goal of the present paper is to develop a simplified model to describe the gravitational fields of elongated asteroids. The proposed model consists of representing an elongated…
Machine Learning applied to asteroid dynamics
V. Carruba, S. Aljbaae, R. C. Domingos +2
Machine Learning (ML) is the branch of computer science that studies computer algorithms that can learn from data. It is mainly divided into supervised learning, where the computer…
Influence of Apophis' spin axis variations on a spacecraft during the 2029 close approach with Earth
S. Aljbaae, J. Souchay, V. Carruba +2
Tumbling asteroids belong to a small group of objects, whose angular velocity vector is unaligned with any of its principal axes of inertia. This leads to challenging efforts to mo…
Artificial Neural Network classification of asteroids in the M1:2 mean-motion resonance with Mars
V. Carruba, S. Aljbaae, R. C. Domingos +1
Artificial neural networks (ANN) have been successfully used in the last years to identify patterns in astronomical images. The use of ANN in the field of asteroid dynamics has bee…
First approximation for spacecraft motion relative to (99942) Apophis
S. Aljbaae, D. M. Sanchez, A. F. B. A. Prado +4
We aim at providing a preliminary approach on the dynamics of a spacecraft in orbit about the asteroid (99942) Apophis during its Earth close approach. The physical properties from…
On the age of the Nele asteroid family
V. Carruba, D. Vokrouhlický, D. +2
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 pericenter longitudes $\varp…
The Hoffmeister asteroid family
V. Carruba, B. Novakovic, S. Aljbaae
The Hoffmeister family is a C-type group located in the central main belt. Dynamically, it is important because of its interaction with the nodal secular resonance with Ce…
Influence of the Centaurs and TNOs on the main belt and its families
Mattia Alvise Galiazzo, Paul Wiegert, Safwan Aljbaae
Centaurs are objects whose orbits are found between those of the giant planets. They are supposed to originate mainly from the TransNeptunian objects, and they are among the source…
The dynamical environment of asteroid 21 Lutetia according to different internal models
Safwan Aljbaae, Thierry G. G. Chanut, Valerio Carruba +3
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 body is assumed to be h…
On the highly inclined leptokurtic asteroid families
V. Carruba, R. C. Domingos, S. Aljbaae +1
leptokurtic asteroid families are families for which the distribution of the normal component of the terminal ejection velocity field is characterized by a positive val…
On the oldest asteroid families in the main belt
V. Carruba, D. Nesvorný, S. Aljbaae +2
Asteroid families are groups of minor bodies produced by high-velocity collisions. After the initial dispersions of the parent bodies fragments, their orbits evolve because of seve…
Footprints of a possible Ceres asteroid paleo-family
V. Carruba, D. Nesvorný, S. Marchi +1
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 craters about 280~km in…
Characterizing the original ejection velocity field of the Koronis family
Valerio Carruba, David Nesvorný, Safwan Aljbaae
An asteroid family forms as a result of a collision between an impactor and a parent body. The fragments with ejection speeds higher than the escape velocity from the parent body c…
On the Erigone family and the secular resonance
Valerio Carruba, Safwan Aljbaae, Othon C. Winter
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 young cluster. Yarko-YO…
Dynamical evolution of the Cybele asteroids
Valerio Carruba, David Nesvorný, Safwan Aljbaae +1
The Cybele region, located between the 2J:-1A and 5J:-3A mean-motion resonances, is adjacent and exterior to the asteroid main belt. An increasing density of three-body resonances…