Possible observations



While working with the Adeona and Gefion asteroid families we were interested in finding objects with D > 15 km and apparent ejection velocities larger than 100 m/s.   We were looking for relatively "large" asteroids because those bodies could not be moved on time-scales comparable with the ages of these families (~500 Myr) by the Yarkovsky force, and we wanted to find objects with an apparent ejection velocity larger than 100 m/s because this seems to be the largest possible velocity produced for such bodies by hydrocode simulations (Michel et al. 2001).   To compute the ejection velocities we computed the center of the family as the center of mass of the family in a, e, and i for all objects with H < 12.5 (which roughly corresponds to D = 10 km), to avoid taking into account objects displaced by the Yarkovsky force.

We found 16 such bodies in the Adeona family and 14 in the Gefion family.  Of these, only 3 had a known spectral type in the Adeona family (Ch), and 11 in the Gefion family (S).   Since these objects cannot have been moved by the Yarkovsky force, the 14 objects with compatible spectral types are possible candidates to have experienced past close encounters with (1) Ceres or other massive asteroids.    We still do not know if the remaining 16 objects are actual members or possible interlopers.   We believe it would be interesting to check their spectral type, in the following table we report their numbers, effective diameteres,
the computed ejection velocities, and the spectral type, when available.
 
 
 
ADEONA FAMILY
GEFION FAMILY
       
Asteroid number
Diameter
Ejection Velocity
Spectral type
 
[km]
[m/s]
 
       
2333
20
125
 
4157
20
105
Ch
3445
19
110
 
46644
19
145
 
997
18
135
Ch
1994
18
165
 
19133
17
350
 
5270
17
105
 
5831
17
320
 
17284
17
110
 
22053
16
210
 
13856
16
250
 
36648
16
110
 
4523
15
125
Ch
15445
15
125
 
     
       
Asteroid number
Diameter
Ejection Velocity
Spectral type
 
[km]
[m/s]
 
       
3724
22
180
 
2386
20
110
S
2521
20
140
S
2053
19
145
S
2905
19
115
S
1433
17
200
S
3860
17
185
S
2157
17
105
S
3910
17
100
S
2595
17
185
 
4417
17
305
S
10064
16
355
 
1839
16
155
S
2875
15
185
S
       
       

The following figures display the locations in the e-a and i-a planes of the centers of the families (black cross), the family members (blue dots) and the asteroids with a possible past history of close encounters (red crosses).
 
Adeona family
Gefion family