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28978 Ixion

28978 Ixion
Ixion appears as a faint point because it is 41 AU, with an apparent magnitude of about 19.7 (AstDys)
Ixion imaged with the 2.2-meter MPG/ESO telescope at La Silla Observatory in 2001 at a distance of 41 AU
Discovery [1][2]
Discovered by Deep Ecliptic Survey
Cerro Tololo (807)
Discovery date 22 May 2001
Designations
MPC designation 28978 Ixion
Pronunciation [note 1]
2001 KX76
TNO (plutino)[3]
Adjectives Ixionian
Orbital characteristics[1]
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 49.269 AU (7370.503 Gm)
Perihelion 30.091 AU (4501.495 Gm)
39.680 AU (5935.999 Gm)
Eccentricity 0.242
249.95 yr (91295.847 d)
268.546°
Inclination 19.584°
71.028°
298.779°
Physical characteristics
Dimensions 617+19
−20
 km
[4]
Albedo 0.141±0.011[4]
Temperature ≈ 44 K
Spectral type
B−V = 1.03±0.03
V−R = 0.61±0.03[5]
19.6 (opposition)[6]
3.828±0.039[4]
0.022″

28978 Ixion is a plutino (an object that has a 2:3 orbital resonance with Neptune). It is very likely to be a dwarf planet,[7][8] although the IAU has not officially classified it as such. Light-curve-amplitude analysis shows only small deviations, which suggests that Ixion is a spheroid with small albedo spots and hence a dwarf planet.[9] It has a diameter of approximately 650 km, making it about the fifth-largest plutino. It is moderately red in visible light and has a surface made of a mixture of tholin and water ice.

It was discovered on May 22, 2001 by the Cerro Tololo Inter-American Observatory (807).[2] It is named after Ixion, a figure from Greek mythology.

Contents

  • Physical characteristics 1
  • Orbit and rotation 2
  • See also 3
  • Notes 4
  • References 5
  • External links 6

Physical characteristics

Different diameters for Ixion depending on its albedo

Other than Pluto, Ixion was the first trans-Neptunian object (TNO) discovered that was originally estimated to be larger than asteroid Ceres,[10] Even in 2002, a year after its discovery, Ixion was still believed to be more than 1000 km in diameter,[11] though the 2002 estimate was a result of a spurious detection at 250 GHz that was not confirmed by later observations.[12] More recent estimates suggest that Ixion has a high albedo[13] and is smaller than Ceres. Observations of Ixion by Herschel Space Telescope and Spitzer Space Telescope in the far-infrared part of the spectrum revealed that its size is about 620 km.[4]

Ixion is moderately red (slightly redder than

  • AstDys orbital elements
  • Orbital simulation from JPL (Java) / Ephemeris

External links

  1. ^ a b "JPL Small-Body Database Browser: 28978 Ixion (2001 KX76)".  
  2. ^ a b B. G. Mardsen (1 July 2001). "MPEC 2001-N01: 2001 FT185, 2001 KW76, 2001 KX76, 2001 KY76, 2001 KZ76, 2001 KA77". IAU Minor Planet Center. Retrieved 2010-01-06. 
  3. ^ M. W. Buie (12 July 2007). "Orbit Fit and Astrometric record for 28978". SwRI, Space Science Department. Retrieved 2008-09-29. 
  4. ^ a b c d Lellouch, E.; Santos-Sanz, P.; Lacerda, P.; Mommert, M.; Duffard, R.; Ortiz, J. L.; Müller, T. G.; Fornasier, S.; Stansberry, J.; Kiss, Cs.; Vilenius, E.; Mueller, M.; Peixinho, N.; Moreno, R.; Groussin, O.; Delsanti, A.; Harris, A. W. (September 2013). TNOs are Cool": A survey of the trans-Neptunian region. IX. Thermal properties of Kuiper belt objects and Centaurs from combined Herschel and Spitzer observations""" (PDF). Astronomy & Astrophysics 557: A60.  
  5. ^ Doressoundiram, A.; Peixinho, N.; Moullet, A.; Fornasier, S.; Barucci, M. A.; Beuzit, J. -L.; Veillet, C. (2007). "The Meudon Multicolor Survey (2MS) of Centaurs and Trans-Neptunian Objects: From Visible to Infrared Colors". The Astronomical Journal 134 (6): 2186.  
  6. ^ a b "AstDys (28978) Ixion Ephemerides".  
  7. ^  
  8. ^ Tancredi, G. (2010). "Physical and dynamical characteristics of icy "dwarf planets" (plutoids)". Icy Bodies of the Solar System: Proceedings IAU Symposium No. 263, 2009. 
  9. ^ Tancredi, G., & Favre, S. (2008) Which are the dwarfs in the Solar System?. Depto. Astronomía, Fac. Ciencias, Montevideo, Uruguay; Observatorio Astronómico Los Molinos, MEC, Uruguay. Retrieved 10-08-2011
  10. ^ R. Stenger (24 August 2001). "New object deemed largest minor planet".  
  11. ^ F. Bertoldi, W. Altenhoff, N. Junkes (7 October 2002). "Beyond Pluto: Max-Planck radioastronomers measure the sizes of distant minor planets". SpaceRef.com. Retrieved 2010-01-06. 
  12. ^ a b W. J. Altenhoff, F. Bertoldi, K. M. Menten (2004). "Size estimates of some optically bright KBOs".  
  13. ^ W. R. Johnston (17 September 2008). "TNO/Centaur diameters and albedos". Archived from the original on 29 August 2010. Retrieved 28 July 2010. 
  14. ^ a b S. Marchi, M. Lazzarin, S. Magrin, C. Barbieri (2003). "Visible spectroscopy of the two largest known trans–Neptunian objects: Ixion and Quaoar".  
  15. ^ J. Licandro, F. Ghinassi, L. Testi (2002). "Infrared spectroscopy of the largest known trans-Neptunian object 2001 KX76".  
  16. ^ a b H. Boehnhardt; et al. (2004). "Surface characterization of 28978 Ixion (2001 KX76)".  
  17. ^ O. Lorin, P. Rousselot (2007). "Search for cometary activity in three Centaurs (60558) Echeclus, 2000 FZ53 and 2000 GM137 and two trans-Neptunian objects (29981) 1999 TD10 and (28978) Ixion".  

References

  1. ^ Or as in Latin: Ixīōn, Ancient Greek: Ιξίων. Sometimes erroneously .

Notes

See also

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 below the ecliptic 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. Ixion does demonstrate some regular changes in brightness, which are thought to be caused by its rotation. As of 2010, however, the rotation period of Ixion remains undetermined.[16]

Orbit and position of Ixion (green), Pluto (red) and Neptune (grey) in 2006

Orbit and rotation

. perihelion and it is possible that Ixion could develop a coma or temporary atmosphere when it is closer to [6] Ixion is currently about 41 AU from the Sun,[17].coma (VLT) has checked Ixion for cometary activity, but did not detect a Very Large Telescope The [16]

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