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Table 5:

MBC properties.
Objecta ab ec id $T_{\rm J}$e HRf $R({\rm active})$g $\nu({\rm active})$h $\alpha_{\rm pl}({\rm active})$i $m_{R}({\rm active})$j Referencesk
133P/Elst-Pizarro 3.164 0.154 1.369 3.185 15.5 2.64-3.06 349.9-89.1 0.1-0.7 18.3-20.3 1-3
P/2005 U1 (Read) 3.165 0.253 1.267 3.153 20.1 2.42-2.51 26.4-43.9 0.1-0.5 19.3-20.2 4, 5
176P/LINEAR 3.217 0.150 1.352 3.172 15.1 2.59-2.60 10.1-18.6 0.0-0.1 19.2-19.6 3, 6
P/2008 R1 (Garradd) 2.726 0.342 15.903 3.217 >17.8 1.85-1.96 28.2-48.6 0.5-11.3 18.5-21.2 7, 8
a Proper orbital elements for 133P and 176P from the AstDyS website; osculating elements for P/Read and P/Garradd from JPL's Solar System Dynamics Group's Small-Body Database.
b Semimajor axis in AU.
c Eccentricity.
d Inclination in degrees.
e Tisserand invariant, as computed from tabulated orbital elements.
f Absolute R-band magnitude.
g Range of heliocentric distances, in AU, during which activity has been observed.
h Range of true anomalies, in degrees, during which activity has been observed.
i Range of orbit plane angles, in degrees, during which activity has been observed.
j Range of apparent R-band magnitudes when activity has been observed.
k 1) Elst et al. (1996); 2) Hsieh et al. (2004); 3) Hsieh et al. (2009a); 4) Read et al. (2005); 5) Hsieh et al. (2009b); 6) Hsieh & Jewitt (2006b); 7) Garradd et al. (2008); 8) Jewitt et al. (2009).

Source LaTeX | All tables | In the text

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