The orbital and absolute magnitude distribution of the near-Earth objects (NEOs) is difficult to compute, partly because only a modest fraction of the entire NEO population has been discovered so far, but also because the known NEOs are biased by complicated observational selection effects. To circu
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Near-Earth object velocity distributions and consequences for the Chicxulub impactor
โ Scribed by S.V. Jeffers; S.P. Manley; M.E. Bailey; D.J. Asher
- Publisher
- John Wiley and Sons
- Year
- 2001
- Tongue
- English
- Weight
- 266 KB
- Volume
- 327
- Category
- Article
- ISSN
- 0035-8711
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