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Contents

   



(Top)
 


1 Discovery  





2 Physical characteristics  





3 Satellite system  



3.1  Petit-Prince  





3.2  S/2004 (45) 1  







4 Notes  





5 See also  





6 References  





7 External links  














45 Eugenia






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From Wikipedia, the free encyclopedia
 

(Redirected from S/2004 (45) 1)

45 Eugenia
Discovery[1]
Discovered byH. Goldschmidt
Discovery date27 June 1857
Designations

MPC designation

(45) Eugenia
Pronunciation/jˈniə/[2]

Named after

Empress Eugénie

Alternative designations

1941 BN

Minor planet category

Main belt
AdjectivesEugenian
Orbital characteristics[3]
Epoch 26 November 2005 (JD 2453701.5)
Aphelion440.305 Gm (2.943 AU)
Perihelion373.488 Gm (2.497 AU)

Semi-major axis

406.897 Gm (2.720 AU)
Eccentricity0.082

Orbital period (sidereal)

1638.462 d (4.49 a)

Mean anomaly

45.254°
Inclination6.610°

Longitude of ascending node

147.939°

Argument of perihelion

85.137°
Known satellitesPetit-Prince
S/2004 (45) 1
Physical characteristics
Dimensions232 × 193 × 161 km[4]
305 × 220 × 145 km[5][6]

Mean radius

94±km[7]
107.3±2.1 km[5]
Mass(5.8±0.1)×1018 kg[7]
(5.69±0.1)×1018 kg[4]
(5.8±0.2)×1018 kg[8][9][a]

Mean density

1.66±0.07 g/cm3[7]
1.1±0.1 g/cm3[4]
1.1±0.3 g/cm3[9]

Equatorial surface gravity

0.017 m/s²[b]

Equatorial escape velocity

0.071 km/s[b]

Sidereal rotation period

0.2375 d (5.699 h)[10]

Axial tilt

117±10°

Pole ecliptic latitude

−30±10°[6]

Pole ecliptic longitude

124±10°

Geometric albedo

0.065 (calculated)[7]
0.040±0.002[5]

Spectral type

F[11]

Absolute magnitude (H)

7.46[5]

Eugenia (minor planet designation: 45 Eugenia) is a large asteroid of the asteroid belt. It is famed as one of the first asteroids to be found to have a moon orbiting it. It was also the second triple asteroid to be discovered, after 87 Sylvia.

Discovery

[edit]

Eugenia was discovered on 27 June 1857 by the Franco-German amateur astronomer Hermann Goldschmidt.[12] His instrument of discovery was a 4-inch aperture telescope located in his sixth floor apartment in the 6th ArrondissementofParis.[13] It was the forty-fifth minor planet to be discovered. The preliminary orbital elements were computed by Wilhelm Forster in Berlin, based on three observations in July, 1857.[14]

The asteroid was named by its discoverer after Empress Eugenia di Montijo, the wife of Napoleon III.[12] It was the first asteroid to be definitely named after a real person, rather than a figure from classical legend.[15]

Physical characteristics

[edit]

Eugenia is a large asteroid, with a diameter of 214 km. It is an F-type asteroid, which means that it is very dark in colouring (darker than soot) with a carbonaceous composition. Like Mathilde, its density appears to be unusually low, indicating that it may be a loosely packed rubble pile, not a monolithic object. Eugenia appears to be almost anhydrous.[16] Lightcurve analysis indicates that Eugenia's pole most likely points towards ecliptic coordinates (β, λ) = (-30°, 124°) with a 10° uncertainty,[6] which gives it an axial tilt of 117°. Eugenia's rotation is then retrograde, rotating backward to its orbital plane.

Satellite system

[edit]

Petit-Prince

[edit]

In November 1998, astronomers at the Canada-France-Hawaii TelescopeonMauna Kea, Hawaii, discovered a small moon orbiting Eugenia. This was the first time an asteroid moon had been discovered by a ground-based telescope. The moon is much smaller than Eugenia, about 13 km in diameter, and takes five days to complete an orbit around it.

The discoverers chose the name "Petit-Prince" (formally "(45) Eugenia I Petit-Prince"). This name refers to Empress Eugenia's son, the Prince Imperial. However, the discoverers also intended an allusion to the children's novella The Little PrincebyAntoine de Saint-Exupéry, which is about a young prince who lives on an asteroid.[17]

S/2004 (45) 1

[edit]

A second, smaller (estimated diameter of 6 km) satellite that orbits closer to Eugenia than Petit-Prince has since been discovered and provisionally named S/2004 (45) 1.[18] It was discovered by analyses of three images acquired in February 2004 from the 8.2 m VLT "Yepun" at the European Southern Observatory (ESO) Cerro Paranal, in Chile.[19] The discovery was announced in IAUC 8817, on 7 March 2007 by Franck Marchis and his IMCCE collaborators. It orbits the asteroid at about ~700 km, with an orbital period of 4.7 days.[18]

Notes

[edit]
  1. ^ Uncertainty calculated from uncertainties in the orbit of Petit-Prince.
  • ^ a b On the extremities of the long axis.
  • See also

    [edit]

    References

    [edit]
    1. ^ "Discovery Circumstances: Numbered Minor Planets". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. 9 February 2010. Archived from the original on 10 May 2008. Retrieved 12 August 2010.
  • ^ "Eugenia". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  • ^ "ASTORB". Orbital elements database. Lowell Observatory.
  • ^ a b c Baer, Jim (2008). "Recent Asteroid Mass Determinations". Personal Website. Archived from the original on 2 July 2013. Retrieved 7 December 2008.
  • ^ a b c d "Supplemental IRAS minor planet survey". Planetary Science Institute. Archived from the original on 17 August 2009.
  • ^ a b c Kaasalainen, M.; et al. (2002). "Models of Twenty Asteroids from Photometric Data" (PDF). Icarus. 159 (2): 369–395. Bibcode:2002Icar..159..369K. doi:10.1006/icar.2002.6907.
  • ^ a b c d P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
  • ^ Marchis, F. "synthesis of several observations". Berkeley. Archived from the original on 13 September 2006.
  • ^ a b Marchis, F.; et al. (2004). "Fine Analysis of 121 Hermione, 45 Eugenia, and 90 Antiope Binary Asteroid Systems With AO Observations". Bulletin of the American Astronomical Society. 36: 1180. Bibcode:2004DPS....36.4602M.
  • ^ "PDS lightcurve data". Planetary Science Institute. Archived from the original on 9 April 2009.
  • ^ "PDS node taxonomy database". Planetary Science Institute. Archived from the original on 5 August 2009.
  • ^ a b Schmadel, Lutz D. (2003). Dictionary of minor planet names. Physics and astronomy online library (5th ed.). Springer. p. 19. ISBN 3-540-00238-3.
  • ^ J. C. (1867). "Obituary: Herman Goldschmidt". Memoirs of the Royal Astronomical Society. 36: 114–117. Retrieved 13 August 2010.
  • ^ Goldschmidt, H. (July 1857). "New Planet (45)". Monthly Notices of the Royal Astronomical Society. 17: 263–264. Bibcode:1857MNRAS..17..263G. doi:10.1093/mnras/17.9.263b.
  • ^ Tobin, William (2003). The life and science of Léon Foucault: the man who proved the earth rotates. Cambridge University Press. p. 301. ISBN 0-521-80855-3.
  • ^ A. S. Rivkin (2002). "Calculated Water Concentrations on C Class Asteroids" (PDF). Lunar and Planetary Institute. Retrieved 22 May 2008.
  • ^ William J. Merlin et al., "On a Permanent Name for Asteroid S/1998(45)1". 26 May 2000.
  • ^ a b Marchis, F.; Baek, M.; Descamps, P.; Berthier, J.; Hestroffer, D.; Vachier, F. (2007). "S/2004 (45) 1". IAU Circular. 8817: 1. Bibcode:2007IAUC.8817....1M.
  • ^ "IMCCÉ Breaking News". Archived from the original on 27 September 2007. Retrieved 30 April 2019.
  • [edit]
    Retrieved from "https://en.wikipedia.org/w/index.php?title=45_Eugenia&oldid=1236132153#S/2004_(45)_1"

    Categories: 
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