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Panopaea (minor planet designation: 70 Panopaea) is a large main belt asteroid. Its orbit is close to those of the Eunomia asteroid family; however, Panopaea is a dark, primitive carbonaceous C-type asteroid in contrast to the S-type asteroids of the Eunomian asteroids. The spectra of the asteroid displays evidence of aqueous alteration.[10] Photometric studies give a rotation period of 15.797 hours and an amplitude of 0.11±0.01 in magnitude. Previous studies that suggested the rotation period may be twice this amount were rejected based upon further observation.[11]

70 Panopaea
Discovery[1]
Discovered byHermann Mayer Salomon Goldschmidt
Discovery siteParis Observatory
Discovery date5 May 1861
Designations
MPC designation
(70) Panopaea
Pronunciation/pænəˈpiːə/[2]
Named after
Panopea
Minor planet category
main belt[3]
AdjectivesPanopaean
Orbital characteristics[4]
Epoch 30 November 2008
Aphelion3.0903 AU
Perihelion2.1402 AU
Semi-major axis
2.61526 AU
Eccentricity0.181641
Orbital period (sidereal)
1544.79 days (4.23 years)
Mean anomaly
264.193°
Inclination11.584°
Longitude of ascending node
47.783°
Argument of perihelion
256.016°
Physical characteristics
Dimensions122.17±2.3 km (mean)[5]
Mass(4.33 ± 1.09) × 1018 kg[6]
Mean density
3.48 ± 1.05[6] g/cm3
Synodic rotation period
15.87 ± 0.04 hours[7]
Geometric albedo
0.0675 ± 0.003[5]
Spectral type
C[8]
Absolute magnitude (H)
8.11[9]

    Panopaea was discovered by Hermann Goldschmidt on 5 May 1861.[1] It was his fourteenth and last asteroid discovery. It is named after Panopea, a nymph in Greek mythology; the name was chosen by Robert Main, President of the Royal Astronomical Society.[12] In 1862, Swedish astronomer Nils Christoffer Dunér gave a doctoral thesis on the orbital elements of this asteroid.[13]

    The orbit of 70 Panopaea places it in a mean motion resonance with the planets Jupiter and Saturn. The computed Lyapunov time for this asteroid is 24,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because of gravitational perturbations of the planets.[14]

    The asteroid frequently makes close approaches with 16 Psyche, such as on 12 June 2040 when it will make a close approach of 0.00602 AU (2.34 Lunar distances, or approx. 770,000 km, 478,455 mi) to the asteroid, and on 2 June 2095 when it will come only 0.003372 AU (1.31 LD) to the asteroid.[3]


    References


    1. "Discovery Circumstances: Numbered Minor Planets (1)-(5000)". IAU: Minor Planet Center. Archived from the original on 2 February 2009. Retrieved 31 December 2008.
    2. 'Panopea' in Noah Webster (1884) A Practical Dictionary of the English Language
    3. "70 Panopaea". JPL Small-Body Database. Jet Propulsion Laboratory. Retrieved 31 December 2008.
    4. "(70) Panopaea". AstDyS. Italy: University of Pisa. Retrieved 31 December 2008.
    5. Tedesco; et al. (2004). "Supplemental IRAS Minor Planet Survey (SIMPS)". IRAS-A-FPA-3-RDR-IMPS-V6.0. Planetary Data System. Archived from the original on 17 August 2009. Retrieved 31 December 2008.
    6. Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
    7. Schroll & Schober (1983). "Lightcurves and rotation periods for the asteroids 70 Panopaea and 235 Carolina". Astronomy and Astrophysics Supplement Series. 53: 77–79. Bibcode:1983A&AS...53...77S.
    8. Neese (2005). "Asteroid Taxonomy". EAR-A-5-DDR-TAXONOMY-V5.0. Planetary Data System. Archived from the original on 5 August 2009. Retrieved 27 December 2008.
    9. Tholen (2007). "Asteroid Absolute Magnitudes". EAR-A-5-DDR-ASTERMAG-V11.0. Planetary Data System. Archived from the original on 16 August 2009. Retrieved 31 December 2008.
    10. Fornasier, S.; et al. (February 1999), "Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites", Astronomy and Astrophysics Supplement, 135: 65−73, Bibcode:1999A&AS..135...65F, doi:10.1051/aas:1999161.
    11. Marciniak, Anna; et al. (June 2016), "Difficult cases in photometric studies of asteroids", 37th Meeting of the Polish Astronomical Society, held 7-10 September, 2015 at Adam Mickiewicz University in Poznań, Poland. Proceedings of the Polish Astronomical Society, vol. 3, pp. 84−87, Bibcode:2016pas..conf...84M.
    12. Schmadel, Lutz (2003). Dictionary of minor planet names (fifth ed.). Germany: Springer. p. 22. ISBN 3-540-00238-3.
    13. Plicht, Christof A. (24 December 2016), "Dunér, Nils Christoffer", Biographical Encyclopedia of Astronomers, doi:10.1007/978-1-4419-9917-7_388.
    14. Šidlichovský, M. (1999), Svoren, J.; Pittich, E. M.; Rickman, H. (eds.), "Resonances and chaos in the asteroid belt", Evolution and source regions of asteroids and comets : proceedings of the 173rd colloquium of the International Astronomical Union, held in Tatranska Lomnica, Slovak Republic, August 24–28, 1998, pp. 297–308, Bibcode:1999esra.conf..297S.



    На других языках

    [de] (70) Panopaea

    (70) Panopaea ist ein Asteroid des Hauptgürtels, der am 5. Mai 1864 durch den deutsch-französischen Astronomen Hermann Mayer Salomon Goldschmidt entdeckt wurde.
    - [en] 70 Panopaea

    [es] (70) Panopaea

    (70) Panopaea es un asteroide perteneciente al cinturón de asteroides descubierto el 5 de mayo de 1861 por Hermann Mayer Salomon Goldschmidt desde París, Francia. Está nombrado por Panopea, un personaje de la mitología griega.[2]

    [ru] (70) Панопея

    (70) Панопея (лат. Panopaea) — астероид главного пояса, который принадлежит к тёмному спектральному классу C и входит в состав семейства Эвномии. Он был открыт 5 мая 1861 года немецким астрономом Германом Гольдшмидтом с помощью 4-дюймового телескопа, расположенного на шестом этаже его квартиры в Латинском квартале Парижа, и назван в честь Панопеи, дочери Нерея в древнегреческой мифологии. Имя было предложено британским астрономом Робертом Мэном — президентом Британского королевского астрономического общества[6].


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