Spin rates of V-type asteroids | Astronomy & Astrophysics (A&A)

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Table A.6

As in Table A.2, but for the NEA population.

Asteroid	Synodic period	U-code	Diameter	Class,	a	e	sin(i)
No.	(LCDB) (h)	(LCDB)	(km)	references	(au)
1981	5.22	3	3.4	V⁽⁶⁾	0.650	1.777	0.6400
3361	3.532	3	0.3	V^(3,17)	0.323	1.210	0.0470
3551	4.93	2	0.9	V^(1,11)	0.487	2.093	0.1650
3908	4.42601	3	1.0	V^(1,7,15)	0.459	1.927	0.0380
4055	7.475	3	2.5	V^{(1,2,5,7,8,10,11,13,14,16,18,19)}	0.326	1.820	0.3950
5604	5.3375	3	0.6	V^(1,5,7,13)	0.405	0.927	0.0840
6611	2.5568	3	0.8	V^(1,12)	0.485	1.696	0.1500
7889	2.741	3	1.7	V^(4,7), R⁽²⁰⁾	1.261	0.346	0.6000
52750	26.43	2+	1.1	V^(4,5)	0.525	1.427	0.1940
55532	46.08	2	1.3	V⁽¹⁸⁾,Sk⁽⁷⁾	1.794	0.696	0.623
137052	9.007	3−	0.9	V^(1,12)	0.810	1.248	0.2570
137199	2.767	3	1.2	V⁽²¹⁾,Q⁽¹⁸⁾	1.457	0.293	0.285
137924	10.57	3−	1.0	V⁽⁵⁾	0.895	0.876	0.4340
152756	2.845	3	0.5	V⁽¹⁸⁾,S⁽⁶⁾	1.451	0.415	0.263
163249	3.7663	3	0.6	V⁽¹⁸⁾	1.344	0.335	0.121
164121	2.343	3	1.7	V^(5,19)	1.11	0.292	0.695
297418	6.314	3	0.4	V⁽⁵⁾	0.467	0.811	0.1800
389694	5.24	2−	0.5	V⁽¹⁸⁾	1.545	0.492	0.327
477762	15.04	2−	0.3	QV	2.06	0.495	0.205
1996 JA1	5.227	3	0.2	V⁽⁹⁾	0.701	2.567	0.3680
1997 GL3	7.572	2	0.3	V^(1,12)	0.782	2.276	0.1160

References. ⁽¹⁾ Neese (2010), ⁽²⁾ Hasselmann et al. (2012), ⁽³⁾ Wisniewski (1991), ⁽⁴⁾ Duffard et al. (2004), ⁽⁵⁾ Thomas et al. (2014), ⁽⁶⁾ Binzel et al. (2001), ⁽⁷⁾ Binzel et al. (2004), ⁽⁸⁾ Hardersen et al. (2018), ⁽⁹⁾Spahr et al. (1997), ⁽¹⁰⁾Carvano et al. (2010), ⁽¹¹⁾Binzel et al. (1989), ⁽¹²⁾Bus & Binzel (2002), ⁽¹³⁾DeMeo et al. (2009), ⁽¹⁴⁾Hicks et al. (2014), ⁽¹⁵⁾Popescu et al. (2018), ⁽¹⁶⁾Lazzaro et al. (2004), ⁽¹⁷⁾Hasegawa et al. (2018), ⁽¹⁸⁾Lin et al. (2018), ⁽¹⁹⁾Sanchez et al. (2013), ⁽²⁰⁾Dandy et al. (2003), ⁽²¹⁾Carry et al. (2016).

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