Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

NEOMOD: A New Orbital Distribution Model for Near-Earth Objects

  • Authors: David Nesvorný, Rogerio Deienno, William F. Bottke, Robert Jedicke, Shantanu Naidu, Steven R. Chesley, Paul W. Chodas, Mikael Granvik, David Vokrouhlický, Miroslav Brož, Alessandro Morbidelli, Eric Christensen, Frank C. Shelly, Bryce T. Bolin

David Nesvorný et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 13.

The intrinsic (debiased) absolute magnitude distribution of NEOs from our base model (the black line is the median and the blue line is the best fit) is compared to the magnitude distribution from Harris & Chodas (2021; red line). The gray area is the 3σ envelope obtained from the posterior distribution computed by MultiNest. It contains—by definition—99.7% of our base model posteriors.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse