Table 2: List of the 22 V-type asteroids currently known outside the Vesta dynamical family. We report number, name, proper a, e, i, absolute magnitude H, if they are in (R, which stands for resonant) or close (C, for Circulating) to a nonlinear secular resonance (see codes in Table 1), and, if they are close to one of the resonances, what is the period of circulation of the resonant argument.
Ast. # Ast. name a e i H Sec. res. Circulation period

809 Lundia 2.28311 0.1450 6.7363 12.10 z₂ R

956 Elisa 2.29811 0.1575 6.4076 12.03 z₂, ${\gamma }_2$ R, C > 4 Myr

2113
Ehrdni 2.47377 0.0726 6.0790 12.66

2442 Corbett 2.38765 0.0972 5.4225 12.54 ${\sigma}_7$ C > 1 Myr

2566 Kirghizia 2.45003 0.1044 4.4219 12.20 ${\sigma}_7$ , 9J-7S-2A C > 4 Myr, C > 0.05 Myr

2579 Spartacus 2.21037 0.0807 5.8947 13.03

2640 Hallstrom 2.39777 0.1253 6.5286 12.85 4J-2S-1A, ${\sigma}_{6}$ , ${\sigma}_7$ R, C > 4 Myr, C > 4 Myr,

2653 Principia 2.44350 0.1145 5.0773 12.24

2704 Julian Loewe 2.38485 0.1173 5.0888 12.75 ${\sigma}_7$ C > 1 Myr

2763 Jeans 2.40355 0.1790 4.3185 11.99

2795 Lepage 2.29574 0.0747 6.5979 12.75 ${\gamma }_2$ C > 4 Myr

2851 Harbin 2.47819 0.1204 7.7933 11.98 ${\gamma}_{5a}$ C > 3 Myr

2912 Lapalma 2.28927 0.1175 6.7421 12.45 ${\gamma}_7$ C > 1 Myr

3849 Incidentia 2.47422 0.0653 5.3938 12.63 ${\gamma}_{5b}$ , ${\gamma}_{6b}$ C > 5 Myr, C > 5 Myr

3850 Peltier 2.23457 0.1061 4.7323 13.46 ${\sigma}_4$ C > 4 Myr

3869 Norton 2.45241 0.1009 5.2787 12.54

4188 Kitezh 2.33538 0.1118 5.6413 12.67 ${\sigma}_{5a}$ C > 3 Myr

4278 Harvey 2.26689 0.1473 5.2499 13.62 ${\psi}_2$ , ${\sigma}_{5b}$ C > 2 Myr, C > 6 Myr

4434 Nikulin 2.44110 0.1033 5.5261 12.88 ${\gamma}_{6c}$ C > 2 Myr

4796 Lewis 2.35523 0.1413 3.0955 13.22 ${\sigma}_{6}$ , ${\sigma}_7$ C > 4 Myr, C > 4 Myr

4977 Rauthgundis 2.29229 0.0928 5.9408 13.99 ${\gamma }_2$ C > 2 Myr

5379 Abehiroshi 2.39599 0.0728 3.3537 12.55 ${\gamma}_{5c}$ , ${\gamma}_{6c}$ C > 4 Myr, C > 4 Myr

**Table 2:** List of the 22 V-type asteroids currently known outside the Vesta dynamical family. We report number, name, proper *a, e, i*, absolute magnitude H, if they are in (R, which stands for resonant) or close (C, for Circulating) to a nonlinear secular resonance (see codes in Table 1), and, if they are close to one of the resonances, what is the period of circulation of the resonant argument.
Ast. #	Ast. name	a	e	i	H	Sec. res.	Circulation period
809	Lundia	2.28311	0.1450	6.7363	12.10	z₂	R
956	Elisa	2.29811	0.1575	6.4076	12.03	z₂, ${\gamma }_2$	R, C > 4 Myr
2113	Ehrdni	2.47377	0.0726	6.0790	12.66
2442	Corbett	2.38765	0.0972	5.4225	12.54	${\sigma}_7$	C > 1 Myr
2566	Kirghizia	2.45003	0.1044	4.4219	12.20	${\sigma}_7$ , 9J-7S-2A	C > 4 Myr, C > 0.05 Myr
2579	Spartacus	2.21037	0.0807	5.8947	13.03
2640	Hallstrom	2.39777	0.1253	6.5286	12.85	4J-2S-1A, ${\sigma}_{6}$ , ${\sigma}_7$	R, C > 4 Myr, C > 4 Myr,
2653	Principia	2.44350	0.1145	5.0773	12.24
2704	Julian Loewe	2.38485	0.1173	5.0888	12.75	${\sigma}_7$	C > 1 Myr
2763	Jeans	2.40355	0.1790	4.3185	11.99
2795	Lepage	2.29574	0.0747	6.5979	12.75	${\gamma }_2$	C > 4 Myr
2851	Harbin	2.47819	0.1204	7.7933	11.98	${\gamma}_{5a}$	C > 3 Myr
2912	Lapalma	2.28927	0.1175	6.7421	12.45	${\gamma}_7$	C > 1 Myr
3849	Incidentia	2.47422	0.0653	5.3938	12.63	${\gamma}_{5b}$ , ${\gamma}_{6b}$	C > 5 Myr, C > 5 Myr
3850	Peltier	2.23457	0.1061	4.7323	13.46	${\sigma}_4$	C > 4 Myr
3869	Norton	2.45241	0.1009	5.2787	12.54
4188	Kitezh	2.33538	0.1118	5.6413	12.67	${\sigma}_{5a}$	C > 3 Myr
4278	Harvey	2.26689	0.1473	5.2499	13.62	${\psi}_2$ , ${\sigma}_{5b}$	C > 2 Myr, C > 6 Myr
4434	Nikulin	2.44110	0.1033	5.5261	12.88	${\gamma}_{6c}$	C > 2 Myr
4796	Lewis	2.35523	0.1413	3.0955	13.22	${\sigma}_{6}$ , ${\sigma}_7$	C > 4 Myr, C > 4 Myr
4977	Rauthgundis	2.29229	0.0928	5.9408	13.99	${\gamma }_2$	C > 2 Myr
5379	Abehiroshi	2.39599	0.0728	3.3537	12.55	${\gamma}_{5c}$ , ${\gamma}_{6c}$	C > 4 Myr, C > 4 Myr

Source LaTeX | All tables | In the text

	1 Introduction
	2 Secular resonances in the Vesta family region
	3 Evolution in the z₂ secular resonance under the Yarkovsky effect
	4 Mechanisms of migration from the Vesta family to the z₂ secular resonance
	5 Discussions
	References