Table 1.
Open in new tab

The ER-specific percentages of asteroids that reach below each of the first six qs values. The percentages corresponding to the total NEA population are weighted according to the contribution of each ER, averaged in the range |$17\lt H\lt 25\, \mathrm{mag}$| (Granvik et al. 2018).

Source|$q_\mathrm{ s}=0.05\, \mathrm{au}$||$q_\mathrm{ s}=0.1\, \mathrm{au}$||$q_\mathrm{ s}=0.15\, \mathrm{au}$||$q_\mathrm{ s}=0.2\, \mathrm{au}$||$q_\mathrm{ s}=025\, \mathrm{au}$||$q_\mathrm{ \mathrm{ s}}=0.3\, \mathrm{au}$||$q_\mathrm{ s}=0.35\, \mathrm{au}$||$q_\mathrm{ s}=0.4\, \mathrm{au}$|
Region(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)
2:1 complex26.2530.2133.6136.7139.6442.1044.5147.21
3:1 complex76.5378.6280.8282.6784.2185.7787.0588.39
5:2 complex23.8425.4327.0428.6530.6332.8635.4338.46
Hungaria80.6182.8084.6086.3187.8189.3390.5391.74
Phocaea92.4494.0295.1996.1796.8597.3897.9498.42
ν6 complex82.8784.7086.7688.4690.0591.3692.6893.86
NEA population79.1181.1283.1984.9586.5187.9889.2790.55
Source|$q_\mathrm{ s}=0.05\, \mathrm{au}$||$q_\mathrm{ s}=0.1\, \mathrm{au}$||$q_\mathrm{ s}=0.15\, \mathrm{au}$||$q_\mathrm{ s}=0.2\, \mathrm{au}$||$q_\mathrm{ s}=025\, \mathrm{au}$||$q_\mathrm{ \mathrm{ s}}=0.3\, \mathrm{au}$||$q_\mathrm{ s}=0.35\, \mathrm{au}$||$q_\mathrm{ s}=0.4\, \mathrm{au}$|
Region(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)
2:1 complex26.2530.2133.6136.7139.6442.1044.5147.21
3:1 complex76.5378.6280.8282.6784.2185.7787.0588.39
5:2 complex23.8425.4327.0428.6530.6332.8635.4338.46
Hungaria80.6182.8084.6086.3187.8189.3390.5391.74
Phocaea92.4494.0295.1996.1796.8597.3897.9498.42
ν6 complex82.8784.7086.7688.4690.0591.3692.6893.86
NEA population79.1181.1283.1984.9586.5187.9889.2790.55
Table 1.
Open in new tab

The ER-specific percentages of asteroids that reach below each of the first six qs values. The percentages corresponding to the total NEA population are weighted according to the contribution of each ER, averaged in the range |$17\lt H\lt 25\, \mathrm{mag}$| (Granvik et al. 2018).

Source|$q_\mathrm{ s}=0.05\, \mathrm{au}$||$q_\mathrm{ s}=0.1\, \mathrm{au}$||$q_\mathrm{ s}=0.15\, \mathrm{au}$||$q_\mathrm{ s}=0.2\, \mathrm{au}$||$q_\mathrm{ s}=025\, \mathrm{au}$||$q_\mathrm{ \mathrm{ s}}=0.3\, \mathrm{au}$||$q_\mathrm{ s}=0.35\, \mathrm{au}$||$q_\mathrm{ s}=0.4\, \mathrm{au}$|
Region(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)
2:1 complex26.2530.2133.6136.7139.6442.1044.5147.21
3:1 complex76.5378.6280.8282.6784.2185.7787.0588.39
5:2 complex23.8425.4327.0428.6530.6332.8635.4338.46
Hungaria80.6182.8084.6086.3187.8189.3390.5391.74
Phocaea92.4494.0295.1996.1796.8597.3897.9498.42
ν6 complex82.8784.7086.7688.4690.0591.3692.6893.86
NEA population79.1181.1283.1984.9586.5187.9889.2790.55
Source|$q_\mathrm{ s}=0.05\, \mathrm{au}$||$q_\mathrm{ s}=0.1\, \mathrm{au}$||$q_\mathrm{ s}=0.15\, \mathrm{au}$||$q_\mathrm{ s}=0.2\, \mathrm{au}$||$q_\mathrm{ s}=025\, \mathrm{au}$||$q_\mathrm{ \mathrm{ s}}=0.3\, \mathrm{au}$||$q_\mathrm{ s}=0.35\, \mathrm{au}$||$q_\mathrm{ s}=0.4\, \mathrm{au}$|
Region(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)(per cent)
2:1 complex26.2530.2133.6136.7139.6442.1044.5147.21
3:1 complex76.5378.6280.8282.6784.2185.7787.0588.39
5:2 complex23.8425.4327.0428.6530.6332.8635.4338.46
Hungaria80.6182.8084.6086.3187.8189.3390.5391.74
Phocaea92.4494.0295.1996.1796.8597.3897.9498.42
ν6 complex82.8784.7086.7688.4690.0591.3692.6893.86
NEA population79.1181.1283.1984.9586.5187.9889.2790.55
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