28978 Ixion
 | |
| Discovery | |
|---|---|
| Discovered by | Deep Ecliptic Survey |
| Discovery date | 22 May, 2001 |
| Designations | |
Designation | 28978 Ixion |
| 2001 KX76 | |
| TNO (plutino) | |
| Orbital characteristics | |
| Epoch December 31, 2006 (JD 2 454 100.5) | |
| Aphelion | 7 370.503 Gm (49.269 AU) |
| Perihelion | 4 501.495 Gm (30.091 AU) |
| 5 935.999 Gm (39.680 AU) | |
| Eccentricity | 0.242 |
| 91 295.847 d (249.95 a) | |
Average orbital speed | 4.66 km/s |
| 268.546° | |
| Inclination | 19.584° |
| 71.028° | |
| 298.779° | |
| Physical characteristics | |
| Dimensions | < 822 km diameter[1] |
| < 2.24×106 km² | |
| Volume | < 3.15×108 km³ |
| Mass | < 5.8×1020? kg |
Mean density | 2.0? g/cm³ |
| < 0.229 7? m/s² | |
| < 0.434 6? km/s | |
| ? d | |
| Albedo | 0.15-0.37[1] |
| Temperature | ~44 K |
Spectral type | (moderately red; B-V=1.03, V-R=0.61) |
| 19.6 (opposition) | |
| 3.244 | |
28978 Ixion (Template:PronEng, ik-SYE-ən, sometimes /ˈɪksiən/, IK-see-ən, from Latin: Ixīōn, [Ιξίων] Error: {{Lang-xx}}: text has italic markup (help)) is a Kuiper belt object discovered on May 22, 2001. Ixion is a plutino (an object that has a 2:3 orbital resonance with Neptune); its estimated diameter of 800 km makes it the third largest plutino. It is named after Ixion, a figure from Greek mythology; it previously had the provisional designation 2001 KX76.
Physical characteristics
Ixion is moderately red (slightly redder than 50000 Quaoar) and it has a higher albedo (0.15) than the mid-sized red cubewanos.
The latest spectroscopic results indicate that Ixion's surface is a mixture of dark carbon and tholin, which is a heteropolymer formed by irradiation of clathrates of water and organic compounds (see TNO spectra). Water ice absorption lines (1.5 and 2μm) were absent (Licandro et al. 2002). Unlike Varuna, Ixion does not show greater reflectivity for longer waves (the so-called red slope) in infrared.
Other than Pluto, Ixion was the first TNO discovered that was originally estimated to be larger than asteroid Ceres.[2] But more recent estimates suggest that Ixion has a high albedo[1] and is smaller than Ceres. It is more likely that 20000 Varuna or 50000 Quaoar may turn out to the first TNO discovered that is larger than Ceres.
Orbit
Ixion and Pluto follow similar but differently oriented orbits: Ixion’s perihelion is below the ecliptic whereas Pluto's is above it. Uncharacteristically for bodies locked in resonance with Neptune (such as Orcus), Ixion approaches Pluto with less than 20 degrees of angular separation. Ixion is currently crossing the ecliptic heading below, and will reach its perihelion in 2070. Pluto has passed its perihelion (1989) and is descending toward the ecliptic. Ixion's orbital period is almost 250 Earth years, about 0.5% larger than Pluto's.
See also
References
- ^ a b c Wm. Robert Johnston. "TNO/Centaur diameters and albedos".
- ^ Richard Stenger (2001-08-24). "New object deemed largest minor planet". CNN (space). Retrieved 2008-02-29.
- H. Boehnhardt, S. Bagnulo, K. Muinonen, M. A. Barucci, L. Kolokolova, E. Dotto and G. P. Tozzi (2003). "Surface characterization of 28978 Ixion (2001 KX76)". Astronomy & Astrophysics. 415: L17–L19.
{{cite journal}}: CS1 maint: multiple names: authors list (link) Pre-print about Ixion's surface from the Planetary Systems Research group of the University of Helsinki
- J. Licandro, F. Ghinassi, L. Testi (2002). "Infrared spectroscopy of the largest known trans-neptunian object 2001 KX76". Astronomy & Astrophysics. 388: L9. doi:10.1051/0004-6361:20020533.
{{cite journal}}: CS1 maint: multiple names: authors list (link) Pre-print on arXiv
- W. J. Altenhoff, F. Bertoldi and K. M. Menten (2004). "Size estimates of some optically bright KBOs". Astronomy & Astrophysics. 415.
External links
- AstDys orbital elements
- Orbital simulation from JPL (Java) / Ephemeris
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