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Table 6:

Properties of the comae of the comets: dust production rate and spectral reflectivity gradient.

Comet
$r_{\rm h}$ Typical Depleted $S^\prime$ Remark
    $Q_{\rm H_2O}$ $Q_{\rm d}$ $Q_{\rm H_2O}$ $Q_{\rm d}$ (%/kÅ)  
  (AU) (mol s-1) (kg s-1) (mol s-1) (kg s-1)    
4P/Faye 2.956O - - $2.2\times10^{26}$ 0.8    
  1.604I - - $6.9\times10^{27}$* 127   L+96
  1.594O - - $6.9\times10^{27}$* 153   L+96
10P/Tempel 2 1.669I $1.8\times10^{27}$ 2 - - 12.4 $\pm$ 2.9  
17P/Holmes 3.116I $1.4\times10^{27}$ 4 $4.4\times10^{26}$ 1    
37P/Forbes 2.270O $2.6\times10^{27}$ 11 $8.1\times10^{26}$ 4 16.1 $\pm$ 3.0  
  2.06I $Q_{\rm d} = 9.81$   NS85      
44P/Reinmuth 2 2.727I $6.3\times10^{27}$ 9 $1.9\times10^{27}$ 3    
50P/Arend 2.374O $4.2\times10^{27}$ 11 $1.3\times10^{27}$ 4 9.3 $\pm$ 3.3  
59P/Kearns-Kwee 2.516O $9.7\times10^{26}$ 5 - - 10.5 $\pm$ 2.1  
  2.27I $Q_{\rm d} = 24.75$   NS85      
63P/Wild 1 2.266O $1.0\times10^{27}$ 4 $3.1\times10^{26}$ 1 27.0 $\pm$ 3.3  
71P/Clark 2.715I $4.9\times10^{27}$ 13 $1.5\times10^{27}$ 5    
84P/Giclas 2.209O $4.4\times10^{27}$ 13 $1.3\times10^{27}$ 5    
106P/Schuster 1.666I $7.5\times10^{27}$ 20 $2.3\times10^{27}$ 8 12.1 $\pm$ 2.9  
112P/Urata-Niijima 2.296I $3.6\times10^{26}$ 4 $1.1\times10^{26}$ 1    
114P/Wiseman-Skiff 1.569O $3.1\times10^{27}$ 17 $9.4\times10^{26}$ 6 14.1 $\pm$ 2.9  
$r_{\rm h}$: heliocentric distance.
I: inbound or O: outbound on the orbit.
$Q_{H{_2}O}, Q_{\rm d}$: water and dust production rates.
*Derived from IUE measurements by Festou et al. (private communication).
$S^\prime [670, 792~{\rm nm}]$: normalized spectral reflectivity gradient.
L+96: Lamy et al. (1996).
NS85: Newburn & Spinrad (1985).

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