Abstrakti
Flux and impact angles were calculated for asteroid collisions with Earth and the Moon, using the latest population models for the distribution of near-Earth objects (NEOs) and precession models to determine the impact probabilities. The calculations predict that the flux of impacts to the poles for Earth is 22% greater than the flux at the equator, and 55% greater for the Moon. Impacts near the equator typically have shallower impact angles with a mode near 30° above the horizontal. Conversely, impacts near the poles are typically steep with a mode close to 65°. Our new analysis updates the previously published results by Le Feuvre & Wieczorek incorporating: (1) an updated debiased distribution of NEOs, and (2) updated collision probabilities that account for Lidov-Kozai precession. The new impact distributions provide an important update to risk models, showing a 7% increase in average population risks from sub-300 m impactors, compared to previous atmospheric entry distributions, mostly due to faster impact velocities.
| Alkuperäiskieli | englanti |
|---|---|
| Artikkeli | 88 |
| Lehti | Planetary Science Journal |
| Vuosikerta | 2 |
| Numero | 3 |
| Sivumäärä | 17 |
| ISSN | 2632-3338 |
| DOI - pysyväislinkit | |
| Tila | Julkaistu - kesäk. 2021 |
| OKM-julkaisutyyppi | A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä, vertaisarvioitu |
Lisätietoja
Erratum published 2023 January 31. DOI 10.3847/PSJ/aca1a7Tieteenalat
- 115 Avaruustieteet ja tähtitiede
Siteeraa tätä
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver