Table 1
Zodiacal bands identified by COBE and IRAS, and information about the asteroid families with which they have been associated.
COBE | IRAS | Associated asteroid family | ||||||||
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|
|
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Namea | δζ b | namec | ipd | namee | ipf | typeg | ageh | ai | ||
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1 | 8.78 | γ | 9.35 | 490 Veritas | 9.26 | C/Ch/... | 8.3 | 3.169 | ||
2 | 1.99 | α | 1.34 | 656 Beagle | 1.34 | .../.../C | ≲10 | 3.157 | ||
β | 2.11 | 832 Karin | 2.11 | .../.../S | 5.8 | 2.866 | ||||
3 | 15.0 | J/K | 12.0 | 845 Naema | 11.96 | .../C/... | ≳20 | ... | ||
4562 Iannini | 12.17 | .../.../S | ≲5 | 2.644 | ||||||
M/N | 15.0 | 1521 Seinajoki | 15.02 | .../.../... | ... | 2.852 |
Notes.
δζ parameter of the K98 zodiacal emission model. This parameter determines roughly at which ecliptic latitudes, in degrees, the band appears.
Modelled proper inclination of the given IRAS band. The first three are from Grogan et al. (2001), while the last two are from Sykes (1988).
Asteroid family associated with the given IRAS band. These all come from N03, except that for 832 Karin, which comes from N08.
Average proper inclination for the associated asteroid family. These all come from N03, except that for 832 Karin, which comes from N08.
Spectral type/classifications. The first two entries in the triplets correspond to the Tholen and SMASSII classes Bus & Binzel (2002), while the third corresponds to the SDSS-based classification (Carvano et al. 2010). Ellipses are used to indicate that the given classification was not found.
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