2012 GX17

2012 GX17
Discovery
Discovered by Pan-STARRS 1
Discovery date April 14, 2012
Designations
MPC designation 2012 GX17
Centaur
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc 1066 days (2.92 yr)
Aphelion 58.496 AU (8.7509 Tm)
Perihelion 16.973 AU (2.5391 Tm)
37.734 AU (5.6449 Tm)
Eccentricity 0.55020
231.80 yr (84664.3 d)
41.574°
 0m 15.308s /day
Inclination 32.488°
209.24°
244.11°
Earth MOID 16.1167 AU (2.41102 Tm)
Jupiter MOID 12.652 AU (1.8927 Tm)
Physical characteristics
Dimensions 55-180 km
0.5-0.05 (assumed)
7.8

    2012 GX17, also written as 2012 GX17, is a minor body classified as centaur by the Minor Planet Center upon discovery. [2] The object is also a promising Neptune L5 trojan candidate.[3]

    Discovery

    2012 GX17 was discovered on April 14, 2012 by the Pan-STARRS 1 telescope, observing from Haleakala, Hawaii.[2]

    Orbit

    2012 GX17 follows a rather eccentric orbit (0.41) with a semi-major axis of 30.13 AU.[4] This object also has high orbital inclination (35.3º).[4] Unfortunately, its orbit is not well determined as it is currently (November 2012) based on 10 observations with a data-arc span of 4 days.[1]

    Physical properties

    2012 GX17 is a rather large minor body with an absolute magnitude of 7.8 which gives a characteristic diameter of 55–180 km for an assumed albedo in the range 0.5-0.05.[1]

    Neptune trojan candidate

    Based on its current heliocentric orbit, 2012 GX17 follows a tadpole orbit around Neptune's L5 point. Giving the fact that its orbit is, at present, poorly determined, the object is a promising Neptune trojan candidate.[3] Simulations suggest that it is dynamically unstable like Neptune L5 trojan 2004 KV18. If confirmed, this object could be the highest inclination Neptune trojan.

    References

    External links

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