Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

70 Panopaea

From Wikipedia, the free encyclopedia
Main-belt asteroid

70 Panopaea
A 3D model of 70 Panopaea made using Lightcurves.
Discovery[1]
Discovered byHermann Mayer Salomon Goldschmidt
Discovery siteParis Observatory
Discovery date5 May 1861
Designations
(70) Panopaea
Pronunciation/pænəˈpə/[2]
Named after
Panopea
main belt[3]
AdjectivesPanopaean
Orbital characteristics[4]
Epoch 30 November 2008
Aphelion3.0903AU
Perihelion2.1402 AU
2.61526 AU
Eccentricity0.181641
1544.79 days (4.23 years)
264.193°
Inclination11.584°
47.783°
256.016°
Physical characteristics
Dimensions122.17±2.3 km(mean)[5]
Mass(4.33 ± 1.09) × 1018 kg[6]
3.48 ± 1.05[6] g/cm3
15.87 ± 0.04 hours[7]
0.0675 ± 0.003[5]
C[8]
8.11[9]

70 Panopaea is a largemain beltasteroid. Its orbit is close to those of theEunomia asteroid family; however, Panopaea is a dark, primitivecarbonaceousC-type asteroid in contrast to theS-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 anamplitude of0.11±0.01 in magnitude. Previous studies that suggested the rotation period may be twice this amount were rejected based upon further observation.[11]

Panopaea was discovered byHermann Goldschmidt on 5 May 1861.[1] It was his fourteenth and last asteroid discovery. It is named afterPanopea, anymph inGreek mythology; the name was chosen byRobert Main, President of theRoyal Astronomical Society.[12] In 1862, Swedish astronomerNils Christoffer Dunér gave a doctoral thesis on theorbital elements of this asteroid.[13]

The orbit of 70 Panopaea places it in amean motion resonance with the planetsJupiter andSaturn. The computedLyapunov time for this asteroid is 24,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because ofgravitational perturbations of the planets.[14]

The asteroid frequently makes close approaches with16 Psyche, such as on 12 June 2040 when it will make a close approach of 0.00602 AU (2.34Lunar 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

[edit]
  1. ^ab"Discovery Circumstances: Numbered Minor Planets (1)-(5000)". IAU: Minor Planet Center.Archived from the original on 2 February 2009. Retrieved31 December 2008.
  2. ^'Panopea' in Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^ab"70 Panopaea".JPL Small-Body Database.Jet Propulsion Laboratory. Retrieved31 December 2008.
  4. ^"(70) Panopaea".AstDyS. Italy:University of Pisa. Retrieved31 December 2008.
  5. ^abTedesco; et al. (2004)."Supplemental IRAS Minor Planet Survey (SIMPS)".IRAS-A-FPA-3-RDR-IMPS-V6.0.Planetary Data System. Archived fromthe original on 17 August 2009. Retrieved31 December 2008.
  6. ^abCarry, 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 fromthe original on 5 August 2009. Retrieved27 December 2008.
  9. ^Tholen (2007)."Asteroid Absolute Magnitudes".EAR-A-5-DDR-ASTERMAG-V11.0.Planetary Data System. Archived fromthe original on 16 August 2009. Retrieved31 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.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=70_Panopaea&oldid=1318195276"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp