Add to ORKGWe estimate the size and orbital distributions of Near Earth Asteroids (NEAs) that are expected to be in the 1:1 mean motion resonance with Venus in a steady state scenario. We predict that the number of such objects with absolute magnitudes H<18 and H<22 is 0.14±0.03 and 3.5±0.7, respectively. We also map the distribution in the sky of these Venus coorbital NEAs and we see that these objects, as the Earth coorbital NEAs studied in a previous paper, are more likely to be found by NEAs search programs that do not simply observe around opposition and that scan large areas of the sky.http://www.sciencedirect.com/science/article/B6WGF-4KMYG2W-2/1/a7a3dcf3c98ddc8cf0d2d1cdbde6853
Near-Earth objects (NEOs) that orbit the Sun on or within Earth's orbit are tricky to detect for Ear...
We have carried out simulations to predict the performance of a new space-based telescopic survey op...
The size distribution of main-belt of asteroids is determined primarily by collisional processes. La...
We estimate the size and orbital distributions of Near Earth Asteroids (NEAs) that are expected to b...
Numerical modeling has long suggested that gravitationally bound (or so-called rubble-pile) near-Ear...
The focus of this work is the current distribution of asteroids in co-orbital motion with Venus, Ear...
Large observational surveys, like those that will be conducted at the Vera C. Rubin Observatory, are...
We are conducting a survey using twilight time on the Dark Energy Camera with the Blanco 4m telescop...
The number of binary asteroids in the near-Earth region might be significantly higher than expected....
We are conducting a survey using twilight time on the Dark Energy Camera with the Blanco 4 m telesco...
An increased ground-based observation program is an essential component of any serious attempt to as...
Aims. We developed a six-part collisional evolution model of the main asteroid belt (MB) and used it...
International audiencePhotometric data on 17 binary near-Earth asteroids (15 of them are certain det...
Photometric data on 17 binary near-Earth asteroids (15 of them are certain detections, two are proba...
Studying the orbital dynamics of small body populations in the Solar System allows us to understand ...
Near-Earth objects (NEOs) that orbit the Sun on or within Earth's orbit are tricky to detect for Ear...
We have carried out simulations to predict the performance of a new space-based telescopic survey op...
The size distribution of main-belt of asteroids is determined primarily by collisional processes. La...
We estimate the size and orbital distributions of Near Earth Asteroids (NEAs) that are expected to b...
Numerical modeling has long suggested that gravitationally bound (or so-called rubble-pile) near-Ear...
The focus of this work is the current distribution of asteroids in co-orbital motion with Venus, Ear...
Large observational surveys, like those that will be conducted at the Vera C. Rubin Observatory, are...
We are conducting a survey using twilight time on the Dark Energy Camera with the Blanco 4m telescop...
The number of binary asteroids in the near-Earth region might be significantly higher than expected....
We are conducting a survey using twilight time on the Dark Energy Camera with the Blanco 4 m telesco...
An increased ground-based observation program is an essential component of any serious attempt to as...
Aims. We developed a six-part collisional evolution model of the main asteroid belt (MB) and used it...
International audiencePhotometric data on 17 binary near-Earth asteroids (15 of them are certain det...
Photometric data on 17 binary near-Earth asteroids (15 of them are certain detections, two are proba...
Studying the orbital dynamics of small body populations in the Solar System allows us to understand ...
Near-Earth objects (NEOs) that orbit the Sun on or within Earth's orbit are tricky to detect for Ear...
We have carried out simulations to predict the performance of a new space-based telescopic survey op...
The size distribution of main-belt of asteroids is determined primarily by collisional processes. La...