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Table 3

Properties of candidates with θ > 90°.

Meteor no. Mass ratio Angle θ Radial distance Time0 Time−1 Time+1 Distance from Earth
0C613xxx (°) (km) (h) (h) (h) (million km)
069, 070 3.75 105.7 6.1 37.9 1.7 422 4.8
153, 154 2.16 124.7 48.7 118.8 13.4 1042 15.0
308A, 308B 1.38 107.8 10.6 123.2 2.9 5000 15.5
350, 351 5.0 112.1 28.4 89.7 7.9 1015 11.3
360A, 360B 62.0 100.7 10 38.5 2.8 531 4.9
455, 456 2.22 154.6 67.2 163.4 18.4 1442 20.6

Notes. The three Time columns show the times necessary to reach radial distance between the two particles: Time0 in the case of zero ejection velocity, and Time and Time+ in the extreme cases of 1 m s−1 ejection velocities (+towards the Sun, − away from the Sun).

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