Astronomy:192 Nausikaa

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192 Nausikaa
192Nausikaa (Lightcurve Inversion).png
A three-dimensional model of 192 Nausikaa based on its light curve.
Discovery
Discovered byJ. Palisa, 1879
Discovery date17 February 1879
Designations
(192) Nausikaa
Pronunciation/nɔːˈsɪki.ə/[1]
Named afterNausicaä
A879 DA; 1933 HH
Minor planet categoryMain belt
AdjectivesNausikaan[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc137.04 yr (50054 d)
|{{{apsis}}}|helion}}2.9934 astronomical unit|AU (447.81 Gm)
|{{{apsis}}}|helion}}1.8121 AU (271.09 Gm)
2.4028 AU (359.45 Gm)
Eccentricity0.24582
Orbital period3.72 yr (1360.4 d)
Mean anomaly94.342°
Mean motion0° 15m 52.632s / day
Inclination6.8137°
Longitude of ascending node343.25°
30.067°
Earth MOID0.814558 AU (121.8561 Gm)
Jupiter MOID2.48275 AU (371.414 Gm)
TJupiter3.474
Physical characteristics
Dimensions103.26±1.9 km[3]
90.18 ± 2.80 km[4]
Mass(1.79 ± 0.42) × 1018 kg[4]
Mean density4.64 ± 1.17 g/cm3[4]
Rotation period13.625 h (0.5677 d)
Geometric albedo0.2330±0.009
S
Apparent magnitude8.2
Absolute magnitude (H)7.13


Nausikaa[5] (minor planet designation: 192 Nausikaa) is a large main-belt S-type asteroid. It was discovered by Johann Palisa on February 17, 1879, at Pula, then in Austria, now in Croatia. The name derives from Nausicaä, a princess in Homer's Odyssey.

This is an S-type asteroid around 86 km with an elliptical ratio of 1.51. The sidereal rotation period is 13.6217 hours.[6]

Based on the lightcurve data obtained from Nausikaa, a possible satellite was reported in 1985. However, this has not been confirmed.[7] A shape model of Nausikaa has been constructed, also based on the lightcurve data. It indicates a roughly cut, but not very elongated body.[8] In 1998 an occultation of a star by the asteroid was observed from the United States.

In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty.[9]

Nausikaa's orbital period is 3.72 years, its distance from the Sun varying between 1.81 and 2.99 AU. The orbital eccentricity is 0.246. Nausikaa brightened to magnitude 8.3 at a quite favorable opposition on 2 September 2011, when it was 1.875 AU from the Sun and 0.866 AU from the Earth.

References

  1. "Nausicäa". Dictionary.com Unabridged. Random House. https://www.dictionary.com/browse/Nausic%C3%A4a. 
  2. Cf. James Joyce's Ulysses: critical essays (1974) Hart & Hayman
  3. 3.0 3.1 "192 Nausikaa". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=192;cad=1. 
  4. 4.0 4.1 4.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  5. Stressed on the 'i', /nɔːˈsɪkiə/.
  6. Marchis, F. et al. (November 2006), "Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey", Icarus 185 (1): pp. 39–63, doi:10.1016/j.icarus.2006.06.001, PMID 19081813, Bibcode2006Icar..185...39M. 
  7. Other reports of asteroid/TNO companions, Johnstonsarchive.net, http://www.johnstonsarchive.net/astro/asteroidmoonsq.html, retrieved 2012-09-01 
  8. "New worlds in our solar system". http://www.astro.helsinki.fi/~kaselain/asteroids.html. 
  9. Gradie, J.; Flynn, L. (March 1988), "A Search for Satellites and Dust Belts Around Asteroids: Negative Results", Abstracts of the Lunar and Planetary Science Conference 19: pp. 405–406, Bibcode1988LPI....19..405G. 

External links