2010 KZ39
| The true title of this article is "2010 KZ39". I change the indication of the title with "2010 KZ39" to break off the limitation of the article name. |
| 2010 KZ39 | |||||||
|---|---|---|---|---|---|---|---|
| Classification | The solar system circumference heavenly bodies [1] | ||||||
| Orbital kind | The separation heavenly bodies [2] キュビワノ group [3] | ||||||
| Discovery | |||||||
| Discovery day | 2010May 21[3] | ||||||
| Detector | RAS campaign eggplant astronomical observatory [3] | ||||||
| An orbital element and property Epoch: TDB 2456600.5 (November, 2013 4.0 days) [1] | |||||||
| Orbit semimajor axis (a) | 45.07 +-0.09 AU [1] | ||||||
| Perihelion distance (q) | 42.5 +-0.2 AU [1] | ||||||
| Aphelion distance (Q) | 47.63 +-0.09 AU [1] | ||||||
| Eccentricity (e) | 0.057 ± 0.004[1] | ||||||
| Revolution period (P) | 110,517+-321 days (302.6+-0.9 year) [1] | ||||||
| Orbit angle of inclination (i) | 26.124 +-0.08 degrees [1] | ||||||
| Perihelion argument (ω) | 321+-3 degrees [1] | ||||||
| Ascending node celestial longitude (Ω) | 53.204 +-0.005 degrees [1] | ||||||
| Mean anomaly (M) | 246+-3 degrees [1] | ||||||
| EMoid | 41.5471 AU [1] | ||||||
| The last time perihelion passage | JED 2,381,180+-1175 (about 1807) | ||||||
| The next time perihelion passage | JED 2,491,697+-872 (about 2109) [1] | ||||||
| Physical property | |||||||
| Diameter | 697km [4] | ||||||
| Mass | 3.55 *1,020 kg | ||||||
| Mean density | 2.0 g/cm3 (supposition) | ||||||
| Absolute magnitude (H) | 4.0 [1] [3] | ||||||
| Albedo (albedo) | 0.09 (supposition) [4] | ||||||
| Surface temperature |
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| The other name | |||||||
| The other name | |||||||
| ■Project ■ Template | |||||||
With 2010 KZ39 one of the separation heavenly bodies or the solar system circumference heavenly bodies belonging to a キュビワノ group [1] [2] [3].
Table of contents
Orbital property
Orbit semimajor axis is 45.0AU, but revolution orbit of 2010 KZ39 is the orbit which is extremely almost a circle where the orbit eccentricity has only 0.06. On the other hand, the orbit angle of inclination declines with 26.12 degrees. I revolve for approximately 303 years, but know the perihelion passage time only at all roughly together on the last time, the next time [1]. There is the document classifying in a キュビワノ group [3], but there is the document dividing into the classification called the separation heavenly bodies from the value of the big orbit angle of inclination [2]. In any case, it is thought that I do not do Neptune and the orbit resonance [2].
Physical property
The value of the absolute magnitude of 2010 KZ39 is 4.0, and this is a big value next to 3.8 of 2010 EK139 in the asteroid which an asteroid number is not given. The diameter becomes the huge heavenly bodies of 697km when I suppose albedo to be 0.09 [4]. This may become the resting hydraulic pressure equilibrium shape by mass of oneself and may meet the standard of the dwarf planet. By this thing, the candidate heavenly bodies of the dwarf planet include 2010 KZ39 [6]. A value of the absolute magnitude is secondly big next to Sedna while it is thought that I am classified in the separation heavenly bodies [7]. In addition, under a condition of the same albedo, it is thought that the surface temperature reaches it from -231 degrees Celsius to -234 degrees Celsius [5]. The mass becomes 3.55*1,020 kg when I suppose mean density to be 2.0 g/cm3 applied to the Pluto type heavenly bodies.
Source
- ^ a b c d e f g h i j k l m n o p (2010 KZ39) JPL Small-Body Database Browser
- ^ a b c d e Orbit Fit and Astrometric record for 10KZ39 Southwest Research Institute Planetary Science Directorate
- ^ a b c d e f g h 2010 KZ39 Minor Planet Center
- ^ a b c List of Known Trans-Neptunian Objects Johnston's Archive
- ^ a b c d Planet Equilibrium Temperature HEC: Calculators
- ^ How many dwarf planets are there in the outer solar system? (updates daily) California Institute of Technology
- ^ Diverse Albedos of Small Trans-Neptunian Objects arXiv
Allied item
This article is taken from the Japanese Wikipedia 2010 KZ39
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