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Cited by 417

The DOI matches its Crossref record; 36 of the 36 references it cites were found in a registry or an index.

The Origin of Planetary Impactors in the Inner Solar System

Open access
Strom, Robert G., Malhotra, Renu, Ito, Takashi, Yoshida, Fumi, Kring, David A.·2005·Science

Abstract

Insights into the history of the inner solar system can be derived from the impact cratering record of the Moon, Mars, Venus, and Mercury and from the size distributions of asteroid populations. Old craters from a unique period of heavy bombardment that ended ∼3.8 billion years ago were made by asteroids that were dynamically ejected from the main asteroid belt, possibly due to the orbital migration of the giant planets. The impactors of the past ∼3.8 billion years have a size distribution quite different from that of the main belt asteroids but very similar to that of near-Earth asteroids.

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Crossref · 10.1126/science.1113544

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Metadata

Authors
Strom, R. G., Malhotra, R., Ito, T., Yoshida, F., & Kring, D. A.
Venue
Science
Published
2005-09-16
Volume
309
Issue
5742
Pages
1847-1850
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2145892001
Cited by
417
References
36
FWCI
14.25
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Origin of Planetary Impactors in the Inner Solar System. https://app.cochat.ai/papers/10.1126/science.1113544
The paper
Strom, R. G., Malhotra, R., Ito, T., Yoshida, F., & Kring, D. A. (2005). The Origin of Planetary Impactors in the Inner Solar System. Science. https://doi.org/10.1126/science.1113544

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.