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C/2018 C2 (Lemmon)

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This is an old revision of this page, as edited by 66.76.2.61 (talk) at 02:44, 5 March 2018 (Correct mark for ʻOumuamua.). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

A/2018 C2
Discovery [1]
Discovered byMount Lemmon Survey (G96)
Discovery siteMount Lemmon Observatory
Discovery date5 February 2018
Designations
A/A/2018 C2
ZC82561
Hyperbolic asteroid,[2] Extended centaur, Damocloid
Orbital characteristics[3]
Epoch 15 February 2018 (JD 2458164.5)
Observation arc30 days
Perihelion1.9563±0.0007 AU
−1300±500 AU[n 1]
Eccentricity1.0015±0.0005
N/A
0° 0m 0.072s / day
Inclination34.452°
91.14°
134.15°
Earth MOID1.061 AU
Jupiter MOID1.405 AU
Physical characteristics
Dimensions1.7–7.6 km (assumed)
19.0 (March 2018)
15.1 ± 0.63

A/2018 C2 is a hyperbolic asteroid[2] discovered on 5 February 2018 by the Mount Lemmon Survey and announced on 4 March 2018 along with another such object, A/2017 U7.

Overview

Although A/2018 C2's orbit is not bound to the Solar System, unlike ʻOumuamua, it is probably not interstellar object. A barycentric orbit of A/2018 C2, shows that it is only a very distant Solar System object, approaching as far as 20,000 ± 80,000 AU from the Sun, around the distance of the Oort Cloud. It had an orbital period of roughly 1 million years until the current approach to the Solar System, where perturbations will shorten the orbit drastically to 2,900 ± 1,700 AU, with an orbital period of 55,000 years.

A/2018 C2 makes closest approach to the Sun on 2 June 2018 at a distance of 1.9 AU (outside the orbit of Mars).[3] If this object out gasses generating a cometary coma while near the inner solar system, it will be reclassified as a common hyperbolic comet.

Upon inclusion to the JPL Small-Body Database, it was incorrectly marked as "A/A/2018 C2" due to the automated database not knowing how to properly handle objects with A/ prefixes.

Notes

  1. ^ Objects on hyperbolic trajectories have negative semimajor axis, giving them a positive orbital energy.

References

  1. ^ "IAU Minor Planet Center - A/2017 U7". Minor Planet Center. International Astronomical Union. Retrieved 5 March 2018.
  2. ^ a b "JPL Small-Body Database Search Engine: orbital class Hyperbolic Asteroid (HYA)". Jet Propulsion Laboratory Solar System Dynamics. Retrieved 4 March 2018.
  3. ^ a b "JPL Small-Body Database Browser: (A/A/2018 C2)". Jet Propulsion Laboratory. Retrieved 4 March 2018.

External links