Table 4
Effect of bulk density in our findings.
ρbulk | MN(a) | Mdepression | Mfallback (c) | Mexcavate (d) | Mfallback/Mescape | Mexcavate/Mdepression | DTI ratio (e) |
---|---|---|---|---|---|---|---|
(kg m−3) | (1013 kg) | (109 kg) | (109 kg) | (109 kg) | |||
200 | 0.76 | ![]() |
![]() |
3.68–13.63 | <3.46 | 0.06–0.28 | 2.6–21.0 |
400 | 1.52 | ![]() |
![]() |
3.68–10.53 | <2.23 | 0.03–0.11 | 2.6–15.5 |
600 | 2.28 | ![]() |
![]() |
3.68–9.14 | <1.68 | 0.02–0.06 | 2.6–13.0 |
800 | 3.04 | ![]() |
![]() |
3.68–8.31 | <1.34 | 0.01–0.04 | 2.6–11.5 |
Notes. (a) Nucleus mass with a given bulk density and ellipsoid-like shape (2.75 × 2.00 × 1.65 km; Duxbury et al. 2004).(b) Total depression mass converted from their volumes with a given bulk density. (c) Dust fallback mass during one comet orbit. The central values are determined when αv = 1.0, and the lower and upper values are obtained assuming αv = 0.5 and αv = 1.5, respectively. (d) Total excavated mass during one comet orbit from the explored side (Eq. (16)). (e) Dust-to-ice mass ratio.
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