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Table 2.

Mutual encounters between asteroids used in this work.

Encounter Ref. mass. 1 Reference t0 tn
[10−11M] (MJD) (MJD)
[7,88;17799,52443,7629,11701] 0.649 ± 1.06 (1) 47911 58154
[10;1259,57493] 4.34 ± 0.26 (1) 48023 58083
[15;765,14401] 1.58 ± 0.09 (2) 48138 58317
[16;17799,20837] 1.37 ± 0.38 (2) 47894 58337
[16;91495,151878] 1.37 ± 0.38 (1) 47894 58337
[19;3486,27799] 0.433 ± 0.073 (1) 48087 58172
[29;987,7060] 0.649 ± 0.101 (1) 47985 57450
[41;8212,10332] 0.317 ± 0.06 (3) 48072 58374
[52;124,306] 1.20 ± 0.29 (1) 47204 57982
[7,88;17799,52443,7629,11701] 0.769 ± 0.156 (1) 47911 58154
[89;38057,54846] 0.337 ± 0.092 (3) 47907 58158.
[216;23747,170964] 0.233 ± 0.10 (3) 47894 58130
[704;43993,48500] 1.65 ± 0.23 (1) 48020 58493

Notes. Our notation is such that the asteroid(s) on the left side of the semicolon are considered perturbers, while those on the right side are massless test asteroids. The reference values are weighted averages of previous literature values taken from the work of Carry (2012). The third column contains references that describe the encounters. We note that Galád & Gray (2002) opted not to publish some of these encounters in the referred paper, and such encounters were obtained from the authors’ website directly (http://staryweb.fmph.uniba.sk/index.php?id=2171). The fourth and fifth columns respectively denote the start and end date of the observational time span for the perturbing asteroid. For the test asteroids, we use all of the available astrometry within this timespan.

References. (1) Baer & Chesley (2017); (2) Galád & Gray (2002); (3) Zielenbach, priv. comm.

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