7066 Nessus

7066 Nessus
Discovery and designation
Discovered by David L. Rabinowitz
Discovery date April 26, 1993
Designations
Named after Nessus
Alternate name(s) 1993 HA2
Minor planet
category
Centaur
Adjective Nessian
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 37.483 AU (Q)
5607.4 Gm
Perihelion 11.826 AU (q)
1769.1 Gm
Semi-major axis 24.655 AU (a)
3688.3 Gm
Eccentricity 0.520
Orbital period 44714.802 d
122.42 yr
Average orbital speed 5.57 km/s
Mean anomaly 43.762°
Inclination 15.647°
Longitude of ascending node 31.216°
Argument of perihelion 170.814°
Dimensions 60±16 km[2][3]
Mass ~1.6×1017 kg
Mean density 2.0? g/cm3
Equatorial surface gravity ~0.0148 m/s2
Equatorial escape velocity ~0.0280 km/s
Sidereal rotation
period
? d
Axial tilt
Pole ecliptic latitude ?
Pole ecliptic longitude ?
Geometric albedo 0.06[2]
Temperature ~56 K
Spectral type ?
Apparent magnitude ~23.4[4]
Absolute magnitude (H) 9.6[1]

7066 Nessus ( /ˈnɛsəs/; from Greek: Νέσσος) is a centaur (a type of icy planetoid) that was discovered by David L. Rabinowitz, working with Spacewatch, at Kitt Peak on 26 April 1993. It was the second centaur found by him (5145 Pholus being his previous find), and the third centaur discovery (2060 Chiron, discovered by Charles Kowal in 1977, was the first). Nessus was officially announced on May 13, 1993, in IAUC 5789 with designation 1993 HA2.

Contents

Orbit

7066 Nessus has an orbital period of 122.4 years, an eccentricity of 0.52 and an inclination to the ecliptic of 15.6 degrees. At perihelion, it moves much closer to the Sun than Uranus, while at aphelion it moves out well beyond the orbit of Neptune.

The orbits of centaurs are unstable due to perturbations by the giant planets. Nessus is a SE object since currently Saturn controls the perihelion and the Edgeworth–Kuiper belt controls the aphelion.[5] Nessus is estimated to have a relatively long orbital half-life of about 4.9 Myr.[5] Fifty clones of the orbit of Nessus suggest that Nessus will not pass within 1AU (150Gm) of a planet for at least twenty thousand years.[6]

Name

The naming of Nessus is an interesting break from tradition. Three astrologers were independently studying 1993 HA2 to see if it had any astrological significance. These were Zane B. Stein in the USA, and Dieter Koch and Robert Von Heeren in Germany. In separate letters to astronomers David L. Rabinowitz, Alan Stern, Jim Scotti and Dr. Brian Marsden, these astrologers suggested naming the body after the mythological centaur Nessus.

Dr. Marsden gave his support to the suggested name, and recommended it to the IAU. This name was approved, and 1993 HA2 was officially named 7066 Nessus on April 22, 1997. This naming was an unprecedented cooperation between astrologers and astronomers.

References

  1. ^ a b "JPL Small-Body Database Browser: 7066 Nessus (1993 HA2)". 2004-05-26 last obs. http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Nessus. Retrieved 2008-09-05. 
  2. ^ a b John Stansberry, Will Grundy, Mike Brown, Dale Cruikshank, John Spencer, David Trilling, Jean-Luc Margot (2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". arXiv:astro-ph/0702538 [astro-ph]. 
  3. ^ Wm. Robert Johnston (22 August 2008). "List of Known Trans-Neptunian Objects". Johnston's Archive. http://www.johnstonsarchive.net/astro/tnoslist.html. Retrieved 2008-09-05. 
  4. ^ "AstDys (7066) Nessus Ephemerides". Department of Mathematics, University of Pisa, Italy. http://hamilton.dm.unipi.it/astdys/index.php?pc=1.1.3.0&n=7066. Retrieved 2010-06-28. 
  5. ^ a b Horner, J.; Evans, N.W.; Bailey, M. E. (2004). "Simulations of the Population of Centaurs I: The Bulk Statistics". Monthly Notices of the Royal Astronomical Society 354 (3): 798–810. arXiv:astro-ph/0407400. Bibcode 2004MNRAS.354..798H. doi:10.1111/j.1365-2966.2004.08240.x. 
  6. ^ "Fifty clones of Centaur 7066 Nessus making passes within 150Gm". http://home.comcast.net/~kpheider/NessusClones.txt. Retrieved 2009-04-26.  (Solex 10)

External links