Table 6
TPM input parameters for the radiometric calculations and the interpretation of the obtained/available mid-/far-IR flux densities.
| Object | HV | A | q | pV | Deff | Orbital period |
|---|---|---|---|---|---|---|
| (mag) | (km) | (days) | ||||
| Ariel (UI) [701] | 0.99 | 0.230 ± 0.025 | 0.43 ± 0.05 | 0.53 | 1159.0 | 2.520 |
| Umbriel (UII) [702] | 1.76 | 0.100 ± 0.010 | 0.39 ± 0.04 | 0.26 | 1170.0 | 4.144 |
| Titania (UIII) [703] | 0.78 | 0.170 ± 0.015 | 0.46 ± 0.05 | 0.37 | 1578.0 | 8.706 |
| Oberon (UIV) [704] | 0.99 | 0.140 ± 0.015 | 0.44 ± 0.05 | 0.31 | 1522.0 | 13.463 |
| Miranda (UV) [705] | 3.08 | 0.200 ± 0.030 | 0.44 ± 0.07 | 0.45 | 474.0 | 1.413 |
Notes. The numbers are taken from Karkoschka (2001): HV are the mean values between Vmax and Vmin with an uncertainty of 0.04 mag, Deff was calculated from the specified radii (both from Table IV). The phase integral q and the Bond albedo A are from Table VII (q and qI0 ∕F, respectively). The geometric albedo pV was calculated via A = p q, with p∕pV ≈ 1.0 (Morrison & Lebofsky 1979).
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