2006 HH123, also written as 2006 HH123, was a misidentified nonexistent object that had a short 1 day observation arc. It was formerly thought to be a lost object with an assumed eccentricity of 0.46.[4] If it had been a scattered-disc object it would have had an absolute magnitude of 5.2,[4] and been a possible dwarf planet. The preliminary orbital elements (as displayed in the infobox to the right) were calculated using only three observations over a period of one day;[4] hence its orbit was very poorly known and it quickly became lost.
| Discovery[1][2] | |
|---|---|
| Discovered by | M. W. Buie R. L. Millis S. D. Kern |
| Discovery date | April 26, 2006 |
| Designations | |
MPC designation | 2006 HH123 |
Minor planet category | deleted[3] Lost TNO SDO |
| Orbital characteristics[4][5] | |
| Epoch April 15, 2006 (JD 2453840.5) | |
| Aphelion | 82 AU (Q) |
| Perihelion | 30 AU (q) |
Semi-major axis | 56 AU (a) |
| Eccentricity | 0.46 (assumed)[4] |
Orbital period (sidereal) | 416 yr |
Mean anomaly | 360° (M) |
| Inclination | 44° |
Longitude of ascending node | 240° |
Argument of perihelion | 0.4° |
| Physical characteristics | |
Absolute magnitude (H) | 5.2[4] |
Of the three discovery images, the first one is an unidentified object, the second one was identified as the main-belt asteroid (130902) 2000 VW33, and the third image shows nothing at the measured position.[6] The three observations of 2006 HH123 were deleted on 6 November 2014,[3] and the provisional designation 2006 HH123 is no longer listed in the Minor Planet Center database.
{{cite web}}: CS1 maint: bot: original URL status unknown (link)
Small Solar System bodies | |||||||
|---|---|---|---|---|---|---|---|
| Minor planets |
| ||||||
| Comets |
| ||||||
| Other |
| ||||||
This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it. |