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. Author manuscript; available in PMC: 2020 May 22.
Published in final edited form as: Minor Planet Bull. 2017 Jul-Sep;44(3):223–237.

Table V.

Pole solutions. L = ecliptic longitude; B = ecliptic latitude; P = sidereal period. The longitude and latitude errors are on the order of ±10°. The period error is approximately 2 units of the last decimal place. The a/b column gives the ratio of the two longest axes (X/Y) of the model. The a/c column gives the ratio of the longest axis (X or Y) versus the Z-axis.

Number Name L1 B1 P1 a/b a/c L2 B2 P2 a/b a/c
3103 Eger 211 −76 5.710138 0.75 1.03
4055 Magellan 81 33 7.477559 1.08 1.38 146 87 7.477580 1.20 1.11
40267 1999 GJ4 63 37 4.957067 1.46 2.28
90075 2002 VU94 73 −50 7.878512 1.25 1.76