Co-orbital Asteroids as the Source of Venus's Zodiacal Dust Ring
arXiv:1904.12404 · doi:10.3847/2041-8213/ab0827
Abstract
Photometry from the Helios and STEREO spacecraft revealed regions of enhanced sky surface-brightness suggesting a narrow circumsolar ring of dust associated with Venus's orbit. We model this phenomenon by integrating the orbits of 10,000,000+ dust particles subject to gravitational and non-gravitational forces, considering several different kinds of plausible dust sources. We find that only particles from a hypothetical population of Venus co-orbital asteroids can produce enough signal in a narrow ring to match the observations. Previous works had suggested such objects would be dynamically unstable. However, we re-examined the stability of asteroids in 1:1 resonance with Venus and found that ~8% should survive for the age of the solar system, enough to supply the observed ring.
arXiv comment18 pages, 7 figures, Published in The Astrophysical Journal Letters
References in corpus (13)
- Cometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites
- Dynamical Model for the Zodiacal Cloud and Sporadic Meteors
- The Geometry of Resonant Signatures in Debris Disks with Planets
- A Study of the Dynamics of Dust from the Kuiper Belt: Spatial Distribution and Spectral Energy Distribution
- Dynamics of Dust Particles Released from Oort Cloud Comets and Their Contribution to Radar Meteors
- Long-Term Stability of Horseshoe Orbits
- Are the Kepler Near-Resonance Planet Pairs due to Tidal Dissipation?
- The Detectability of Exo-Earths and Super-Earths Via Resonant Signatures in Exozodiacal Clouds
- Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets
- Evidence for dust accumulation just outside the orbit of Venus
- Earth Trojan asteroids: A study in support of observational searches
- Transient Co-orbitals of Venus: An Update
- Predictions for the Detection of Earth and Mars Trojan Asteroids by the Gaia satellite
Cited by in corpus (14)
- Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
- The Near-Sun Dust Environment: Initial Observations from Parker Solar Probe
- A Twilight Search for Atiras, Vatiras and Co-orbital Asteroids: Preliminary Results
- Tidal disruption of near-Earth asteroids during close encounters with terrestrial planets
- Horseshoe Co-orbitals of Earth: Current Population and New Candidates
- A Deep and Wide Twilight Survey for Asteroids Interior to Earth and Venus
- Helios spacecraft data revisited: Detection of cometary meteoroid trails by in-situ dust impacts
- An attempt to build a dynamical catalog of Solar System co-orbitals
- Effects of neighbouring planets on the formation of resonant dust rings in the inner Solar System
- Alpha-Meteoroids then and now: Unearthing an overlooked micrometeoroid population
- Dynamics of charged dust in the orbit of Venus
- Modeling Saturn's D68 clumps as a co-orbital satellite system
- Tadpole type motion of charged dust in the Lagrange problem with planet Jupiter
- Trojan asteroids and co-orbital dust ring of Venus