Correction to “Using lunar boulders to distinguish primary from distant secondary impact craters”
G. D. Bart, H. J. Melosh
Abstract
Open-access reader
G. D. Bart, H. J. Melosh
Abstract
Open-access reader
[1] In the paper “Using lunar boulders to distinguish primary from distant secondary impact craters” by Gwendolyn D. Bart and H. J. Melosh (Geophysical Research Letters, 34, L07203, doi:10.1029/2007GL029306, 2007), incorrect data were given in Table 1 under the column “Mean of 5 Largest (m).” The corrected table appears here. Please note: The publisher is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.
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[1] In the paper “Using lunar boulders to distinguish primary from distant secondary impact craters” by Gwendolyn D. Bart and H. J. Melosh (Geophysical Research Letters, 34, L07203, doi:10.1029/2007GL029306, 2007), incorrect data were given in Table 1 under the column “Mean of 5 Largest (m).” The corrected table appears here. Please note: The publisher is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.
Key concepts: Impact crater, Table (database), Primary (astronomy), Geology, Column (typography), Astrobiology, Information retrieval, Remote sensing