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. 2013 Dec 1;13(12):1155–1165. doi: 10.1089/ast.2013.1028

Table 4.

Probabilities and Estimated Viable Transfers to the Planets in the Solar System

    Probability (%) 3.5 Gyr total Mass (kg) transferred
from Earth
Orbit
40±0.3
80,000,000±600,000
2.7×1013
 
Sun
1.5±0.06
3,000,000±100,000
1.0×1012
 
Mercury
0.37±0.03
730,000±60,000
2.5×1011
 
Venus
13±0.2
26,000,000±300,000
8.9×1012
 
Earth
40±0.3
79,000,000±600,000
2.7×1013
 
Mars
0.18±0.02
360,000±40,000
1.2×1011
 
Jupiter
0.041±0.01
83,000±20,000
2.8×1010
 
Saturn
0.0069±0.004
14,000±8,000
4.7×109
 
Ejected
5±0.1
10,000,000±200,000
3.4×1012
from Mars
Orbit
75±0.4
600,000,000±3,000,000
2.0×1014
 
Sun
1.3±0.06
10,000,000±300,000
3.4×1012
 
Mercury
0.03±0.009
240,000±50,000
8.1×1010
 
Venus
1.5±0.06
12,000,000±400,000
4.1×1012
 
Earth
2.6±0.08
21,000,000±500,000
7.0×1012
 
Mars
16±0.2
130,000,000±1,000,000
4.3×1013
 
Jupiter
0.04±0.01
320,000±60,000
1.1×1011
 
Saturn
<0.0025
<20,000
<6.8×109
  Ejected 3.8±0.1 31,000,000±600,000 1.0×1013

The 3.5 Gyr total is the number of transferred objects we expect. Mass transferred assumes each object is ∼340,000 kg (i.e., a 3 m sphere with density of 3 g/cm3). No Mars-to-Saturn transfers were seen in the simulations, so we show the upper limits.