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. Author manuscript; available in PMC: 2020 Jun 3.
Published in final edited form as: Minor Planet Bull. 2013 Oct-Dec;40(4):208–212.

Table I.

Observing circumstances. Asteroids with (H) after the name are members of the Hungaria group/family. The phase angle (α) is given at the start and end of each date range, unless it reached a minimum, which is then the second of three values. If a single value is given, the phase angle did not change significantly and the average value is given. LPAB and BPAB are each the average phase angle bisector longitude and latitude, unless two values are given (first/last date in range).

Number Name 2013 (mm/dd) Pts Phase LPAB BPAB Period P. E. Amp A.E.
1355 Magoeba (H) 05/27–06/05 127 33.9,34.6 187 −10 2.977 0.005 0.15 0.01
11/22–11/25^ 259 5.7,7.2 56 −8 2.972 0.002 0.10 0.01
2150 Nyctimene (H) 05/27–06/07 272 28.2,29.7 193 +4 6.124 0.005 0.66 0.02
4436 Ortizmoreno (H) 05/31–06/05 310 6.4,7.7 235 +11 8.24 0.02 0.09 0.01
4497 Taguchi (H) 05/31–06/03 207 7.8,8.8 231 +7 3.563 0.003 0.11 0.01
5211 Stevenson 06/09–06/14 240 24.1,25.0 226 +34 14.18 0.01 0.33 0.02
8893 1995 KZ 06/04–06/14 668 21.0,22.2 245 +33 22.27 0.02 0.39 0.02
19204 1992 ME 06/03–06/08 332 22.3,21.0 262 +27 19.55 0.10 0.08 0.01
24478 2000 WC145 06/15–06/23 326 17.7,18.9 238 +31 16.13 0.03 0.43 0.03
26074 Carlwirtz (H) 06/06–06/19 330 30.7,31.8 227 +33 2.5493* 0.0003 0.11 0.01
41185 1999 VJ200 06/19–06/20 74 12.2,12.4 241 +21 3.92 0.15 0.39 0.03
125742 2001 XT117 06/04–06/19 712 20.4,22.6 244 +21 60.8# 0.2 1.15 0.05
^

2009

*

period of binary primary

#

dominant period of a tumbler