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52 Europa

From Wikipedia, the free encyclopedia
Large asteroid in the asteroid belt

52 Europa
Discovery
Discovered byH. Goldschmidt
Discovery date4 February 1858
Designations
(52) Europa
Pronunciation/jʊˈrpə/[1]
Named after
Europa
1948 LA
Main belt
AdjectivesEuropan, Europian
Orbital characteristics[2]
Epoch July 01, 2021
(JD 2459396.5, heliocentric)
Aphelion3.444AU (510 Gm)
Perihelion2.75 AU (420 Gm)
3.095 AU (460 Gm)
Eccentricity0.111
5.45yr (1989 d)
21°
Inclination7.48°
129°
343°
Physical characteristics
Dimensions(379±16)×(330±8)×(249±10) km[3]
319±4 km[4]
315±7 km[3]
Flattening0.33[a]
Mass(24±4)×1018 kg[4]
(22.6±1.6)×1018 kg[b][5]
1.41±0.23 g/cm3[4]
1.5±0.4 g/cm3[3]
5.6304 h[2]
0.057±0.007 geometric (0.679±0.017 BV,0.338±0.028 UB)[2]
Temperature~173K
max: 258K (−15 °C)[6]
C/CF[2]
6.66[2]

52 Europa is thesixth largestasteroid in theasteroid belt, having a diameter of over 300 km, though it is not correspondingly massive. It is not spherical but is shaped like an ellipsoid of approximately 380×330×250 km.[3] It was discovered on 4 February 1858, byHermann Goldschmidt from his balcony inParis. It is named afterEuropa, one ofZeus's conquests inGreek mythology, a name it shares withJupiter's moonEuropa.

Physical characteristics

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3D model ofEuropa based onlightcurve modeling

Europa is approximately the sixth largest asteroid by volume. Most likely it has a density of around 1.5 g/cm3, typical of C-type asteroids.[3] In 2007, James Baer and Steven R. Chesley estimated Europa to have a mass of(1.9±0.4)×1019 kg.[7] A more recent estimate by Baer suggests it has a mass of 3.27×1019 kg.[8]

Europa is a very dark carbonaceousC-type, and is the second largest of this group. Spectroscopic studies have found evidence ofolivines andpyroxenes on the surface,[9] and there is some indication that there may be compositional differences between different regions.[10] It orbits close to theHygiea asteroid family, but is not a member.

Lightcurve data for Europa have been particularly tricky to interpret, so much so that for a long time its period of rotation was in dispute (ranging from5+12 hours to 11 hours), despite numerous observations.[11] It has now been determined that Europa is aprograde rotator, but the exact direction in which its pole points remains ambiguous. The most detailed analysis indicates that it points either towards aboutecliptic coordinates (β, λ) = (70°, 55°) or (40°, 255°) with a 10° uncertainty.[12] This gives anaxial tilt of about 14° or 54°, respectively.

In 1988 a search for satellites or dust orbiting this asteroid was performed using theUH88 telescope at theMauna Kea Observatories, but the effort came up empty.[13]

Observations

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It has been found that the reputedcataclysmic variable star CV Aquarii, discovered in 1934, was actually a misidentification of 52 Europa.[14]

Animation of 52 Europa's orbit 2000–2020
   Sun   Earth ·    Mars ·   Jupiter ·    52 Europa

Notes

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  1. ^Flattening derived from the maximum aspect ratio (c/a):f=1ca{\displaystyle f=1-{\frac {c}{a}}}, where (c/a) =0.67±0.04.[4]
  2. ^(11.39 ± 0.79) × 10−12M

References

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  1. ^Noah Webster (1884)A Practical Dictionary of the English Language
  2. ^abcdeJPL data Retrieved 2021-09-29
  3. ^abcdeMerline, W.J. (2013). "The Resolved Asteroid Program – Size, shape, and pole of (52) Europa".Icarus.225 (1):794–805.arXiv:1301.5101.Bibcode:2013Icar..225..794M.doi:10.1016/j.icarus.2013.01.010.S2CID 119286695.
  4. ^abcdP. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.Astronomy & Astrophysics 54, A56
  5. ^James Baer, Steven Chesley & Robert Matson (2011) "Astrometric masses of 26 asteroids and observations on asteroid porosity."The Astronomical Journal, Volume 141, Number 5
  6. ^Dotto, E.; Müller, T. G.;Barucci, M. A.;Encrenaz, Th.; Knacke, R. F.; Lellouch, E.;Doressoundiram, A.;Crovisier, J.; Brucato, J. R.; Colangeli, L.; Mennella, V. (2000)."ISO results on bright Main Belt asteroids: PHT-S observations".Astronomy and Astrophysics.358: 1134.Bibcode:2000A&A...358.1133D. Retrieved23 February 2024.
  7. ^Baer, James;Steven R. Chesley (2007)."Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris".Celestial Mechanics and Dynamical Astronomy.100 (2008). Springer Science+Business Media B.V. 2007:27–42.Bibcode:2008CeMDA.100...27B.doi:10.1007/s10569-007-9103-8.
  8. ^Baer, James (2008)."Recent Asteroid Mass Determinations". Personal Website. Archived fromthe original on 2 July 2013. Retrieved29 November 2008.
  9. ^Dotto, E. (2000)."ISO results on bright Main Belt asteroids: PHT–S observations"(PDF).Astronomy & Astrophysics.358: 1133.Bibcode:2000A&A...358.1133D. Archived fromthe original(PDF) on 14 May 2005. Retrieved29 April 2006.
  10. ^Sawyer, Scott Raleigh (1 January 1991). "A High-Resolution CCD Spectroscopic Survey of Low-Albedo Main Belt Asteroids".PhD Thesis.Bibcode:1991PhDT.......105S – via NASA ADS.
  11. ^Zappalà, V.; di Martino, M.; Cacciatori, S (1983). "On the ambiguity of rotational periods of asteroids: The peculiar case of 52 Europa".Icarus.56 (2):319–324.Bibcode:1983Icar...56..319Z.doi:10.1016/0019-1035(83)90041-6.
  12. ^Michałowski, T (2004)."Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona"(PDF).Astronomy & Astrophysics.416:353–366.Bibcode:2004A&A...416..353M.doi:10.1051/0004-6361:20031706.
  13. ^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, vol. 19, pp. 405–406,Bibcode:1988LPI....19..405G.
  14. ^"CV Aquarii identified with (52) Europa"(PDF). Archived fromthe original(PDF) on 14 February 2006. Retrieved29 April 2006.

Bibliography

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External links

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Large asteroids (mean diameter greater than 200 km)
Mean diameter 900–1000 km
Mean diameter 500–600 km
Mean diameter 300–500 km
Mean diameter 200–300 km
Authority control databasesEdit this at Wikidata
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