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7066 Nessus

From Wikipedia, the free encyclopedia
Very red centaur on an eccentric orbit beyond Saturn in the outer Solar System
Not to be confused withNeso (moon).

7066 Nessus
Hubble Space Telescope image of Nessus taken in 2009
Discovery[1]
Discovered bySpacewatch
(D. Rabinowitz uncredited)[2]
Discovery siteKitt Peak National Obs.
Discovery date26 April 1993
Designations
(7066) Nessus
Pronunciation/ˈnɛsəs/[3]
Named after
ΝέσσοςNessos(Greek mythology)[1]
1993 HA2
centaur[4][5][6] · distant[1]
AdjectivesNessian/ˈnɛsiən/[7]
Symbol (astrological)
Orbital characteristics[4]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 3
Observation arc11.08yr (4,048 d)
Aphelion37.423AU
Perihelion11.854 AU
24.639 AU
Eccentricity0.5189
122.30 yr (44,670 d)
80.046°
0° 0m 29.16s / day
Inclination15.663°
31.183°
170.96°
Jupiter MOID6.400 AU
TJupiter3.793
Physical characteristics
57±17 km[8]
60±16 km[5][9]
0.065[5][9]
0.086[8]
RR(very red)[10]
B–V =1.090±0.010[10]
V–R =0.790±0.010[10]
V–I =1.470±0.030[10]
B–R =1.847[11]
24.31[12]
9.55[13][14]
9.6[1][4]
Uranus
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7066 Nessus/ˈnɛsəs/ is a very redcentaur on an eccentric orbit, located beyondSaturn in theouter Solar System. It was discovered on 26 April 1993, by astronomers of theSpacewatch program at theKitt Peak National Observatory inTucson, Arizona.[1] The dark and reddishminor planet is likely elongated and measures approximately 60 kilometers (37 miles) in diameter.[5][13] It was named afterNessus from Greek mythology.[1]

Orbit and classification

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Nessus is acentaur, a dynamically unstable population ofminor planets between the classicalasteroids and thetrans-Neptunian objects. It orbits the Sun at a distance of 11.9–37.4 AU once every 122 years and 4 months (44,670 days;semi-major axis of 24.64 AU). Its orbit has aneccentricity of 0.52 and aninclination of 16° with respect to theecliptic. At itsperihelion (11.9 AU), it moves much closer to theSun thanUranus (19.2 AU) but not as close as Saturn (9.6 AU), while at itsaphelion (37.4 AU), it moves out well beyond the orbit ofNeptune (30.1 AU).[4]

The orbits of centaurs are unstable due toperturbations by thegiant planets. Nessus is an "SE object" because currently Saturn controls its perihelion and its aphelion is within theKuiper belt. It is estimated to have a relatively long orbital half-life of about 4.9 million years.[15] Fifty clones of the orbit of Nessus suggest that it will not pass within 1 AU (or 150 million kilometers) of any planet for at least 20,000 years.[16]

Discovery and naming

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Nessus was discovered byDavid Rabinowitz (not officially credited), working with theSpacewatch program, atKitt Peak National Observatory on 26 April 1993.[1][2] The discovery was announced on 13 May 1993 in anIAU Circular (IAUC 5789) of theCentral Bureau for Astronomical Telegrams.[2] It was the third discovery of a centaur after2060 Chiron and5145 Pholus, discovered byCharles Kowal and David Rabinowitz in 1977 and 1992, respectively.[17] The body'sobservation arc begins with its official discovery observation atKitt Peak in April 1993.[1]

Thisminor planet was named afterNessus, acentaur fromGreek mythology, who poisoned and was killed by the divine heroHeracles.[1] The officialnaming citation was published by theMinor Planet Center on 22 April 1997 (M.P.C. 29671).[18]

A symbol derived from that for2060 Chiron,U+2BDC NESSUS (), was devised in the late 1990s by German astrologer Robert von Heeren. It replaces Chiron's K with an N for Nessus.[19]

Physical characteristics

[edit]

Nessus has a very red color (RR),[10] with aB–R magnitude of 1.847 and 1.88, respectively.[5][11]Color indices were also determined by Bauer (2003) and Hainaut (2002, 2012).[6][20][21][22]

Rotation period

[edit]

As of 2018, no rotationallightcurve of Nessus has been obtained fromphotometric observations. However, a brightness variation of 0.5magnitude was measured in the 1990s, indicating that the body has a non-spherical, elongated shape.[14] The body'srotation period andpole remain unknown.[4][13]

Diameter and albedo

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According to theHerschel Space Observatory with itsPACS instrument, Nessus measures 57 kilometers in diameter and its surface has analbedo of 0.086,[8] while infrared observations with theSpitzer Space Telescope gave a diameter of 60 kilometers with an albedo of 0.065.[9] TheCollaborative Asteroid Lightcurve Link assumes acarbonaceous standard albedo of 0.057 and derives a diameter of 68.48 kilometers based on anabsolute magnitude of 9.55.[13]

In popular culture

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Nessus is a playable destination in the 2017 video gameDestiny 2, after previously being referenced in the series' 2014 debut entryDestiny. Known simply as "Nessus," it is described as a planetoid that has beenterraformed by acybernetic species known as the Vex into a "machine world".[23]

See also

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References

[edit]
  1. ^abcdefghi"7066 Nessus (1993 HA2)".Minor Planet Center. Retrieved26 November 2018.
  2. ^abc"IAUC 5789: 1993 HA2".Central Bureau for Astronomical Telegrams. 13 May 1993. Retrieved26 November 2018.
  3. ^"Nessus".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  4. ^abcde"JPL Small-Body Database Browser: 7066 Nessus (1993 HA2)" (2004-05-26 last obs.).Jet Propulsion Laboratory. Retrieved26 November 2018.
  5. ^abcdeJohnston, Wm. Robert (7 October 2018)."List of Known Trans-Neptunian Objects".Johnston's Archive. Retrieved26 November 2018.
  6. ^ab"Asteroid 7066 Nessus".Small Bodies Data Ferret. Retrieved26 November 2018.
  7. ^Lamb (1836)Elia
  8. ^abcDuffard, R.; Pinilla-Alonso, N.; Santos-Sanz, P.; Vilenius, E.; Ortiz, J. L.; Mueller, T.; et al. (April 2014). ""TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs".Astronomy and Astrophysics.564: 17.arXiv:1309.0946.Bibcode:2014A&A...564A..92D.doi:10.1051/0004-6361/201322377.S2CID 119177446.
  9. ^abcJohn 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.Bibcode:2008ssbn.book..161S.
  10. ^abcdeBelskaya, Irina N.; Barucci, Maria A.; Fulchignoni, Marcello; Dovgopol, Anatolij N. (April 2015). "Updated taxonomy of trans-neptunian objects and centaurs: Influence of albedo".Icarus.250:482–491.Bibcode:2015Icar..250..482B.doi:10.1016/j.icarus.2014.12.004.
  11. ^abPeixinho, N.; Delsanti, A.; Guilbert-Lepoutre, A.; Gafeira, R.; Lacerda, P. (October 2012). "The bimodal colors of Centaurs and small Kuiper belt objects".Astronomy and Astrophysics.546: 12.arXiv:1206.3153.Bibcode:2012A&A...546A..86P.doi:10.1051/0004-6361/201219057.S2CID 55876118.
  12. ^"Asteroid (7066) Nessus" (Ephemeris at epoch 58447 MJD). AstDyS-2, Asteroids – Dynamic Site; Department of Mathematics, University of Pisa, Italy. Retrieved26 November 2018.
  13. ^abcd"LCDB Data for (7066) Nessus". Asteroid Lightcurve Database (LCDB). Retrieved26 November 2018.
  14. ^abDavies, John K.; McBride, Neil; Ellison, Sara L.; Green, Simon F.; Ballantyne, David R. (August 1998). "Visible and Infrared Photometry of Six Centaurs".Icarus.134 (2):213–227.Bibcode:1998Icar..134..213D.doi:10.1006/icar.1998.5931.
  15. ^Horner, J.; Evans, N. W.; Bailey, M. E. (November 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.S2CID 16002759.
  16. ^"Fifty clones of Centaur 7066 Nessus making passes within 150Gm". Archived fromthe original on 22 February 2013. Retrieved26 April 2009.
    "The SOLEX page". Archived fromthe original on 29 April 2009.
  17. ^"The third Centaur Nessus".The Centaur Research Project. Retrieved26 November 2018.
  18. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 November 2018.
  19. ^Miller, Kirk; Stein, Zane (26 August 2021)."Comment on U+26B7 CHIRON"(PDF). L2/21-225.
  20. ^Bauer, James M.; Meech, Karen J.; Fernández, Yanga R.; Pittichova, Jana; Hainaut, Olivier R.; Boehnhardt, Hermann; et al. (November 2003). "Physical survey of 24 Centaurs with visible photometry".Icarus.166 (1):195–211.Bibcode:2003Icar..166..195B.doi:10.1016/j.icarus.2003.07.004.
  21. ^Hainaut, O. R.; Delsanti, A. C. (July 2002)."Colors of Minor Bodies in the Outer Solar System. A statistical analysis".Astronomy and Astrophysics.389:641–664.Bibcode:2002A&A...389..641H.doi:10.1051/0004-6361:20020431.
  22. ^Hainaut, O. R.; Boehnhardt, H.; Protopapa, S. (October 2012). "Colours of minor bodies in the outer solar system. II. A statistical analysis revisited".Astronomy and Astrophysics.546: 20.arXiv:1209.1896.Bibcode:2012A&A...546A.115H.doi:10.1051/0004-6361/201219566.S2CID 54776793.
  23. ^"Destiny 2's new planet Nessus is on a visiting orbit with a "limited window" (and it's real)".GamesRadar.com. 18 May 2017. Retrieved27 October 2020.

External links

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