Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

2037 Tripaxeptalis

From Wikipedia, the free encyclopedia
Main-belt asteroid

2037 Tripaxeptalis
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date25 October 1973
Designations
(2037) Tripaxeptalis
Named after
Tripaxeptalis(fantasy name)
(3 ×679 Pax = 7 ×291 Alice)[2]
1973 UB · A917 SN
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc43.52 yr (15,894 days)
Aphelion2.6046AU
Perihelion1.9996 AU
2.3021 AU
Eccentricity0.1314
3.49yr (1,276 days)
235.93°
0° 16m 55.92s / day
Inclination4.2509°
9.5018°
346.18°
Physical characteristics
Dimensions5.956±0.213 km[4][5]
6.21 km(calculated)[3]
2.33±0.01h[6]
0.198±0.032[4][5]
0.24(assumed)[3]
S[3]
13.2[1][3] · 13.44±0.12[7] · 13.5[4]

2037 Tripaxeptalis, provisional designation1973 UB, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 6 kilometers in diameter.

It was discovered on 25 October 1973, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland.[8] The asteroid's constructed name "Tripaxeptalis" derives from a numbers game with the asteroids679 Pax and291 Alice.[2]

Orbit and classification

[edit]

Tripaxeptalis is a member of theFlora family, one of the largest collisional populations ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 2.0–2.6 AU once every 3 years and 6 months (1,276 days). Its orbit has aneccentricity of 0.13 and aninclination of 4° with respect to theecliptic.[1]

In September 1917, the asteroid was first identified asA917 SN atSimeiz Observatory on the Crimean peninsula. The body'sobservation arc begins with its official discovery observation at Zimmerwald.[8]

Physical characteristics

[edit]

Rotation period

[edit]

In January 2006, a rotationallightcurve ofTripaxeptalis was obtained from photometric observations by astronomerAdrián Galád atModra Observatory in Slovakia. Lightcurve analysis gave arotation period of 2.33 hours with a brightness variation of 0.10magnitude (U=2). The ambiguous lightcurve gave an alternative period solution of 2.23 hours and an amplitude of 0.10.[6]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Tripaxeptalis measures 5.956 kilometers in diameter and its surface has analbedo of 0.198.[4][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its family – and calculates a diameter of 6.21 kilometers based on anabsolute magnitude of 13.2.[3]

Naming

[edit]

Thisminor planet's constructed name "Tripaxeptalis" (tri–Pax–hepta–Alice) refers to the fact that its number, 2037, matches 3 ×679 Pax as well as 7 ×291 Alice.[2] The approved naming citation was published by theMinor Planet Center on 1 June 1980 (M.P.C. 5359).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2037 Tripaxeptalis (1973 UB)" (2017-05-01 last obs.).Jet Propulsion Laboratory. Retrieved28 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2037) Tripaxeptalis".Dictionary of Minor Planet Names – (2037) Tripaxeptalis.Springer Berlin Heidelberg. p. 165.doi:10.1007/978-3-540-29925-7_2038.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2037) Tripaxeptalis". Asteroid Lightcurve Database (LCDB). Retrieved28 June 2017.
  4. ^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.
  5. ^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. Retrieved28 June 2017.
  6. ^abGalad, Adrian (March 2008)."Several Byproduct Targets of Photometric Observations at Modra".The Minor Planet Bulletin.35 (1):17–21.Bibcode:2008MPBu...35...17G.ISSN 1052-8091. Retrieved28 June 2017.
  7. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved28 June 2017.
  8. ^ab"2037 Tripaxeptalis (1973 UB)".Minor Planet Center. Retrieved28 June 2017.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved28 June 2017.


Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=2037_Tripaxeptalis&oldid=1313183453"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp