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58534 Logos

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(Redirected from Zoe (moon)) Minor planet in the Kuiper belt

58534 Logos
Logos and its companion Zoe imaged by the Hubble Space Telescope in 2004
Discovery
Discovered byMauna Kea Obs. (team disc.)
Discovery siteMauna Kea Obs.
Discovery date4 February 1997
Designations
MPC designation(58534) Logos
Pronunciation/ˈloʊɡɒs/ or /ˈlɒɡɒs/
Named afterLogos
(Aeon in Ptolemy Gnostics)
Alternative designations1997 CQ29
Minor planet categoryTNO  · cubewano
cold
AdjectivesLogian /ˈlɒdʒiən/
Orbital characteristics
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc5582 days (15.28 yr)
Aphelion51.153 AU (7.6524 Tm)
Perihelion39.945 AU (5.9757 Tm)
Semi-major axis45.549 AU (6.8140 Tm)
Eccentricity0.12304
Orbital period (sidereal)307.42 yr (112284 d)
Mean anomaly56.495°
Mean motion0° 0 11.542 / day
Inclination2.8946°
Longitude of ascending node132.491°
Argument of perihelion339.21°
Known satellitesZoe (est. D: 66 km)
Physical characteristics
Mean diameter77±18 km
Mass2.7×10 kg
Mean density1.0 g/cm
Geometric albedo0.39 ± 0.17
Absolute magnitude (H)6.6

58534 Logos, or as a binary system (58534) Logos-Zoe, is a trans-Neptunian object and binary system from the classical Kuiper belt, approximately 77 kilometers (48 miles) in diameter. The bright cubewano belongs to the cold population and has a 66-kilometer (41 miles) sized companion named Zoe. The system mass is (4.58±0.07)×10 kg.

In the Gnostic tradition, Logos and Zoe are a paired emanation of the deity, and part of its creation myth.

Zoe

Zoe
Two bodies with similar mass orbiting around a common barycenter (red cross) with elliptic orbits. The interaction of Logos and Zoe is similar to this.
Discovery
Discovered byKeith S. Noll et al.
Discovery date17 November 2001
Designations
Pronunciation/ˈzoʊ.iː/
Named afterZoe (Ζωή)
Alternative designations(58534) Logos I Zoe
AdjectivesZoean /zoʊˈiːən/)
Orbital characteristics
Semi-major axis8217 km
Eccentricity0.546
Orbital period (sidereal)309.9 d
Satellite ofLogos
Physical characteristics
Dimensions66 km
Mass(1.5±0.2)×10 kg

Logos is a binary with the components of comparable size orbiting the barycentre on a moderately elliptical orbit.

Logos was discovered on 4 February 1997, and its companion, Zoe, was discovered on 17 November 2001 from Hubble Space Telescope observations by K. S. Noll, D. C. Stephens, W. M. Grundy, J. Spencer, Robert Millis, Marc Buie, Dale Cruikshank, S. C. Tegler, and W. Romanishin and announced on 11 February 2002.

After the discovery, it received the provisional designation S/2001 (58534) 1. Once confirmed it was officially named (58534) Logos I Zoe. It orbits Logos with a semi-major axis of 8217 km in 309.9 days with an eccentricity of 0.546. Its estimated diameter is 66 km, and mass (0.15 ± 0.02)×10 kg.

Orbit

A 10-million-year integration of the orbit shows that it is a Classical Kuiper belt object that does not get closer to the Sun than 38.8 AU (5.80 billion km) or further than 52.1 AU.

Orbit of Logos (grey object) compared with Pluto (orange) and Neptune (blue)

References

  1. ^ "58534 Logos (1997 CQ29)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 April 2016.
  2. ^ Marc W. Buie (31 May 2003). "Orbit Fit and Astrometric record for 58534". SwRI (Space Science Department).
  3. Brown, Mike. "How many dwarf planets are there in the Solar System". Retrieved 17 February 2018.
  4. "Logian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  5. ^ Wm. Robert Johnston (4 March 2007). "(58534) Logos and Zoe". Johnston's Archive.
  6. ^ Grundy, W. M; Noll, K. S.; Stephens, D. C. (2005). "Diverse albedos of small trans-neptunian objects". Icarus. 176 (1): 184–191. arXiv:astro-ph/0502229. Bibcode:2005Icar..176..184G. doi:10.1016/j.icarus.2005.01.007. S2CID 118866288.
  7. ^ Grundy, W. M.; Noll, K. S.; Nimmo, F.; Roe, H. G.; Buie, M. W.; Porter, S. B.; Benecchi, S. D.; Stephens, D. C.; Levison, H. F.; Stansberry, J. A. (2011). "Five new and three improved mutual orbits of transneptunian binaries" (PDF). Icarus. 213 (2): 678. arXiv:1103.2751. Bibcode:2011Icar..213..678G. doi:10.1016/j.icarus.2011.03.012. S2CID 9571163.

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