Orbit diagram (top view, 1999 OX3 in blue)
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Discovery[1] and designation
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Discovered by | Mauna Kea |
Discovery date | July 21 1999 |
Designations
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MPC designation | (44594) 1999 OX3 |
Minor planet category |
TNO[2] centaur (DES)[3] |
Epoch 2008-11-30 (2454800.5) | |
Aphelion | 47.169 AU (Q) |
Perihelion | 17.644 AU (q) (near Uranus) |
Semi-major axis | 32.407 AU (a) (near Neptune) |
Eccentricity | 0.4555 |
Orbital period | 184.49 yr |
Mean anomaly | 330.47° (M) |
Inclination | 2.62° |
Longitude of ascending node | 259.13° |
Argument of perihelion | 143.92° |
Dimensions | 192 km[4] |
Geometric albedo | 0.09 (assumed) |
Absolute magnitude (H) | 6.7[2] |
(44594) 1999 OX3 is a Trans-Neptunian object with a centaur-like orbit.
Neptune has a semi-major axis of 30 AU and (44594) 1999 OX3 has a semi-major axis of 32 AU. The Minor Planet Center (MPC) does not classify this object as a centaur because the MPC defines centaurs as having a semi-major axis of less than 30.066 AU. (44594) 1999 OX3 crosses the orbits of both Neptune and Uranus and has an inclination of only 2.62°. The Deep Ecliptic Survey (DES) defines centaurs using a dynamical classification scheme, based on the behavior of orbital integrations over 10 million years. The DES defines centaurs as nonresonant objects whose osculating perihelia are less than the osculating semimajor axis of Neptune at any time during the integration. Using the dynamical definition of a centaur, (44594) 1999 OX3 is a centaur.[3]
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