Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

8661 Ratzinger

From Wikipedia, the free encyclopedia
Main-belt asteroid

8661 Ratzinger
Discovery[1]
Discovered byL. D. Schmadel
F. Börngen
Discovery siteKarl Schwarzschild Obs.
Discovery date14 October 1990
Designations
(8661) Ratzinger
Named after
Pope Benedict XVI
(Pope,chronology)[2]
1990 TA13 · 1969 US
1974 TM1 · 1992 CB1
main-belt · (outer)
Eos[3]
Orbital characteristics[1]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc49.86 yr (18,213 days)
Aphelion3.1158AU
Perihelion2.9001 AU
3.0080 AU
Eccentricity0.0359
5.22yr (1,906 days)
176.919°
0° 11m 20.04s / day
Inclination10.556°
38.061°
90.968°
Physical characteristics
Dimensions13.394±0.198[4]
4.301035±0.000002 h[5]
0.090±0.011[4]
S[6]
12.3[1]

8661 Ratzinger, provisional designation1990 TA13, is an Eoanasteroid from the outer region of theasteroid belt, approximately 13.4 kilometers in diameter. It was discovered on 14 October 1990, by German astronomersLutz Schmadel andFreimut Börngen at theKarl Schwarzschild Observatory in Tautenburg, eastern Germany.[7] The asteroid was named after Cardinal Joseph Ratzinger, who becamePope Benedict XVI.[2]

Orbit and classification

[edit]

Ratzinger is a member of theEos family (606),[3] the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids.[8]: 23  It orbits the Sun at a distance of 2.9–3.1 AU once every 5 years and 3 months (1,906 days). Its orbit has aneccentricity of 0.04 and aninclination of 11° with respect to theecliptic.[1]

In October 1969, it was first identified as1969 US atCrimea–Nauchnij. The body'sobservation arc begins atLeoncito in 1974, when it was identified as1974 TM1, 16 years prior to its official discovery observation at Tautenburg.[7]

Physical characteristics

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Ratzinger measures 13.4 kilometers in diameter and its surface has analbedo of 0.09.[4] In 2018,Josef Ďurechet al. measured its rotation period as4.301035±0.000002 hours and provided a partial shape model.[5]

As of 2020,Ratzinger's composition remains unknown.[1][6]

Naming

[edit]

Thisminor planet was named after GermanJoseph Ratzinger (born 1927), then Cardinal and professor of theology, for the role he played in supervising the opening of theVatican Secret Archives in 1998 to researchers investigating judicial errors against Galileo, after whom the minor planet697 Galilea is named, and other medieval scientists.[2]

Ratzinger was considered to be one of the most authoritative voices in the Vatican and becamePope Benedict XVI in 2005. The name was proposed by the asteroid's first discoverer,Lutz Schmadel.[2] The approved naming citation was published by theMinor Planet Center on 23 May 2000 (M.P.C. 40702).[9]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 8661 Ratzinger (1990 TA13)" (2019-08-28 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 25 December 2019. Retrieved17 April 2020.
  2. ^abcdSchmadel, Lutz D. (2007). "(8661) Ratzinger".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 659.doi:10.1007/978-3-540-29925-7_7136.ISBN 978-3-540-00238-3.
  3. ^ab"Asteroid 8661 Ratzinger – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  4. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved4 December 2016.
  5. ^abĎurech, J.; Hanuš, J.; Alí-Lagoa, V. (September 2018)."Asteroid models reconstructed from the Lowell PhotometricDatabase and WISE data".Astronomy & Astrophysics.617: A57.arXiv:1807.02083.doi:10.1051/0004-6361/201833437.S2CID 119388288. Retrieved17 April 2020.
  6. ^ab"LCDB Data for (8661) Ratzinger". Asteroid Lightcurve Database (LCDB). Retrieved17 April 2020.
  7. ^ab"8661 Ratzinger (1990 TA13)".Minor Planet Center. Retrieved4 July 2016.
  8. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.S2CID 119280014.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 July 2016.

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=8661_Ratzinger&oldid=1313216411"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp