Discovery | |
---|---|
Discovery date | 2003 |
Designations | |
2003 LA7 | |
1:4 resonance[1][2] | |
Orbital characteristics[3] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 3 | |
Observation arc | 1746 days (4.78 yr) |
Aphelion | 116.44 AU (17.419 Tm) (Q) |
Perihelion | 36.002 AU (5.3858 Tm) (q) |
76.220 AU (11.4023 Tm) (a) | |
Eccentricity | 0.52765 (e) |
665.45 yr (243054 d) | |
346.07° (M) | |
0° 0m 5.332s /day (n) | |
Inclination | 5.6369° (i) |
34.076° (Ω) | |
271.47° (ω) | |
Earth MOID | 34.9906 AU (5.23452 Tm) |
Jupiter MOID | 30.912 AU (4.6244 Tm) |
Physical characteristics | |
Dimensions | ~231 km (assumed)[4] |
0.09 (assumed) | |
~22.4[5] | |
6.5[3] | |
2003 LA7, also written as 2003 LA7, is a resonant trans-Neptunian object that goes around the Sun once for every four times that Neptune goes around. This means it is in a 1:4 orbital resonance with Neptune. Another example of such object in this resonance is 2011 UP411.
Orbit The orbit of "fourtino" 2003 LA7 compared to Pluto and Neptune. |
1:4 Libration Neptune is held stationary at 5 o'clock. |
2003 LA7 is in a 1:4 resonance with the planet Neptune.[1][2] For every one orbit that a it makes, Neptune orbits 4 times.
It is currently 43 AU from the Sun,[5] and will come to perihelion around 2041.[3]
Assuming a generic TNO albedo of 0.09, it is about 231 km in diameter.[4]
It has been observed 14 times over 4 oppositions.[3]