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.
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+1⁄2 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]
^abcdP. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.Astronomy & Astrophysics 54, A56
^James Baer, Steven Chesley & Robert Matson (2011) "Astrometric masses of 26 asteroids and observations on asteroid porosity."The Astronomical Journal, Volume 141, Number 5
^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.
^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.
Sawyer, S. R. (1991).A High-Resolution CCD Spectroscopic Survey of Low-Albedo Main Belt Asteroids PhD thesis (Thesis). The University of Texas.Bibcode:1991PhDT.......105S.
Schmeer, P., and M. L. Hazen,CV Aquarii identified with (52) Europa, Journal of the American Association of Variable Star Observers, Vol. 28, p. 103 (2000).