Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1346 Gotha

From Wikipedia, the free encyclopedia
Main-belt asteroid

1346 Gotha
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date5 February 1929
Designations
(1346) Gotha
Named after
Gotha[2]
(German city inThuringia)
1929 CY · 1931 RC1
1948 PL1 · 1952 OC
main-belt · (middle)[3]
background[4] · Eunomia[5]
Orbital characteristics[6]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc90.53yr (33,065 d)
Aphelion3.0948AU
Perihelion2.1599 AU
2.6274 AU
Eccentricity0.1779
4.26 yr (1,556 d)
147.30°
0° 13m 53.04s / day
Inclination13.849°
166.12°
250.00°
Physical characteristics
13.731±0.120 km[7]
13.747±0.325 km[8]
2.64067±0.00002 h[3][9]
0.278±0.009[7]
0.2794±0.0411[8]
S(est.)[3][10]
B–V = 0.840[6]
11.25[6]
11.32[3][8][10]
11.4[1]

1346 Gotha, provisional designation1929 CY, is a stony backgroundasteroid from the central regions of theasteroid belt, approximately 14 kilometers (8.7 mi) in diameter. It was discovered on 5 February 1929, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[1] The presumedS-type asteroid has a shortrotation period of 2.6 hours.[3] It was named for the German city ofGotha, located inThuringia.[2]

Orbit and classification

[edit]

Based on thehierarchical clustering method,Gotha is a non-family asteroid of the main belt'sbackground population (Nesvorny),[4] but it has also been considered a core member of theEunomia family by Novakovic, Knezevic and Milani.[5] It orbits the Sun in thecentral main-belt at a distance of 2.2–3.1 AU once every 4 years and 3 months (1,556 days;semi-major axis of 2.63 AU). Its orbit has aneccentricity of 0.18 and aninclination of 14° with respect to theecliptic.[6] The body'sobservation arc begins with its official discovery observation at Heidelberg in 1929.[1]

Naming

[edit]

Thisminor planet was named after the city ofGotha, located nearErfurt capital of the Free State ofThuringia, Germany. The asteroids1254 Erfordia and934 Thüringia are also named after these places. The city is known for itsGotha Observatory and the work of astronomerFranz Xaver von Zach (1754–1832), who recovered the dwarf planetCeres and after whom999 Zachia was named. The officialnaming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 122).[2]

Physical characteristics

[edit]

Gotha has been estimated to be a stonyS-type asteroid.[3][10]

Rotation period

[edit]

Several rotationallightcurves ofGotha have been obtained from photometric observations since 1984.[3][9][10][11][12] Lightcurve analysis gave a consolidatedrotation period of 2.64067 hours with a brightness variation between 0.10 and 0.16magnitude (U=3-).[3]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Gotha measures between 13.731 and 13.747 kilometers in diameter and its surface has analbedo between 0.278 and 0.2794.[7][8] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 16.18 kilometers based on anabsolute magnitude of 11.32.[3]

References

[edit]
  1. ^abcd"1346 Gotha (1929 CY)".Minor Planet Center. Retrieved29 October 2019.
  2. ^abcSchmadel, Lutz D. (2007). "(1346) Gotha".Dictionary of Minor Planet Names – (1346) Gotha.Springer Berlin Heidelberg. p. 109.doi:10.1007/978-3-540-29925-7_1347.ISBN 978-3-540-00238-3.
  3. ^abcdefghi"LCDB Data for (1346) Gotha". Asteroid Lightcurve Database (LCDB). Retrieved16 November 2017.
  4. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved16 November 2017.
  5. ^ab"Asteroid 1346 Gotha – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^abcd"JPL Small-Body Database Browser: 1346 Gotha (1929 CY)" (2019-08-17 last obs.).Jet Propulsion Laboratory. Retrieved29 October 2019.
  7. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved16 November 2017.
  8. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1346) Gotha". Geneva Observatory. Retrieved16 November 2017.
  10. ^abcdBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved16 November 2017.
  11. ^Aznar Macias, Amadeo (January 2017)."Lightcurve Analysis from APT Observatory Group for Nine Mainbelt Asteroids: 2016 July-September. Rotation Period and Physical Parameters".The Minor Planet Bulletin.44 (1):60–63.Bibcode:2017MPBu...44...60A.ISSN 1052-8091. Retrieved16 November 2017.
  12. ^Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved16 November 2017.

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=1346_Gotha&oldid=1291783059"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp