(55565) 2002 AW197

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The correct title of this article is (55565) 2002 AW197. It features superscript or subscript characters that are substituted or omitted because of technical limitations.
(55565) 2002 AW197
Discovery
Discovered by Michael E. Brown,
Eleanor F. Helin,
Michael Hicks,
Kenneth Lawrence,
Steven H. Pravdo,
Chad Trujillo
Discovery date January 10, 2002
Designations
MPC designation (55565) 2002 AW197
Alternative names none
Minor planet
category
TNO (cubewano)
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 8003.964 Gm (53.503 AU)
Perihelion 6143.329 Gm (41.066 AU)
Semi-major axis 7073.647 Gm (47.284 AU)
Eccentricity 0.132
Orbital period 118761.410 d (325.15 a)
Average orbital speed 4.31 km/s
Mean anomaly 281.945°
Inclination 24.410°
Longitude of ascending node 297.513°
Argument of perihelion 295.307°
Physical characteristics
Dimensions 940 km
Mass 5.2×1020? kg
Mean density 2.0? g/cm³
Equatorial surface gravity 0.2216? m/s²
Escape velocity 0.4192? km/s
Sidereal rotation
period
? d
Albedo 0.17±0.03
Temperature ~39–40 K
Spectral type ?
Absolute magnitude 3.27

(55565) 2002 AW197 is a trans-Neptunian object (TNO). It was discovered in 2002 by Michael E. Brown et al. It is classified as a cubewano.

Contents

[edit] Size

Observations of thermal emissions by Spitzer give a diameter of about 940 km[1] and a higher than expected albedo of 0.17±0.03.

[edit] Surface

ESO analysis of spectra reveals a strong red slope and no presence of water ice (in contrast to Quaoar, also red) suggesting organic material (see comparison of colours and typical composition inferred from spectra of the TNOs).

[edit] External links

[edit] References

  • Cruikshank, D., et al. High Albedo KBO (55565)2002 AW197, The Astronomical Journal Letters, 624,53 (May 2004). Abstract
  • Doressoundiram, A.; Barucci, M. A.; Tozzi, G. P.; Poulet, F.; Boehnhardt, H.; de Bergh, C.; Peixinho, N. Spectral characteristics and modeling of the trans-neptunian object (55565) 2002 AW197 and the Centaurs (55576) 2002 GB10 and (83982) 2002 GO9: ESO Large Program on TNOs and Centaurs. Planetary and Space Science, 53, Issue 14-15, p. 1501-1509 (2005). Abstract