Attributes of the largest minor planets
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The largest minor planets (also known as planetoids) are smoothly rounded, like major planets, because their gravity overcomes material strength that keeps smaller bodies in non-spherical shapes. Before the discovery of 2060 Chiron and the trans-Neptunian objects, the term "minor planet" was a synonym for asteroid, but many people now prefer to restrict the use of "asteroid" to refer to rocky bodies of the inner solar system. Most trans-Neptunian objects are icy, like comets, although those we can detect at that distance are much larger than comets.
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Several asteroids, in the strict sense, are large enough to be spherical. The largest known trans-Neptunian objects are much larger than the large asteroids. (Natural satellites of major planets also range smoothly from small non-spherical objects to large spherical ones, and the largest are larger than 1 Ceres, the largest asteroid). the evolution of the kitchen
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All attributes below are measured relative to the Earth:
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| Minor
planet |
Equatorial diameter |
Mass |
Orbital
radius(AU) |
Orbital
period (years) |
Day(days) |
| 1 Ceres |
0.075 |
0.000
158 |
2.767 |
4.603 |
0.3781 |
| 90482
Orcus |
0.066 -
0.148 |
0.000
10 - 0.001 17 |
39.47 |
248
|
? |
| 28978
Ixion |
~0.083 |
0.000
10 - 0.000 21 |
39.49
|
248
|
? |
| (55636)
2002 TX300 |
0.0745
|
?
|
43.102
|
283 |
? |
| 20000
Varuna |
0.066 -
0.097 |
0.000
05 - 0.000 33 |
43.129 |
283 |
0.132
or 0.264 |
| 2003
EL61 |
~.0768 |
~0.000
67 |
43.339 |
285 |
? |
| 50000
Quaoar |
0.078 -
0.106 |
0.000
17 - 0.000 44 |
43.376 |
285 |
? |
| 2005
FY9 |
~0.14 |
? |
45.64 |
308 |
? |
| 2003
UB313 |
0.24 |
0.004? |
67.709 |
557 |
? |
| 90377
Sedna |
0.093 -
0.141 |
0.000
14 - 0.001 02 |
502.040 |
11500 |
20 |
 |