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1251 Hedera

From Wikipedia, the free encyclopedia

1251 Hedera
Modelled shape ofHedera from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date25 January 1933
Designations
(1251) Hedera
Pronunciation/ˈhɛdərə/[2]
Named after
Hedera(a.k.a. "Ivy")[3]
1933 BE · 1929 CD1
1931 TJ2 · 1975 NW1
A907 GD · A915 CA
main-belt[1][4] · (middle)
background[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc102.80 yr (37,548 days)
Aphelion3.1452AU
Perihelion2.2884 AU
2.7168 AU
Eccentricity0.1577
4.48yr (1,636 days)
55.862°
0° 13m 12.36s / day
Inclination6.0489°
140.65°
217.52°
Physical characteristics
13.239±0.150 km[6][7]
44.22 km(calculated)[4]
15.015±0.010 h[8]
19.9000±0.0002 h[9]
19.9020±0.0001 h[10]
19.9020±0.0002 h[11]
19.915±0.005 h[12]
19.915±0.007 h[12]
19.985±0.002 h[13]
0.057(assumed)[4]
0.636±0.050[6][7]
Tholen =E[1]
SMASS =X[1]
E[7][14] · C(SDSS-MFB)[4]
B–V = 0.689[1]
U–B = 0.233[1]
10.5[1][4][7] · 10.67±0.28[15]

1251 Hedera (prov. designation:1933 BE) is abackground asteroid from the central regions of theasteroid belt, approximately 13 kilometers (8 miles) in diameter. It was discovered on 25 January 1933, by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[16] The asteroid was named for the climbing plantHedera, commonly known as "ivy".[3]

Orbit and classification

[edit]

Hedera is a non-family asteroid from the main belt'sbackground population.[5] It orbits the Sun in thecentral asteroid belt at a distance of 2.3–3.1 AU once every 4 years and 6 months (1,636 days;semi-major axis of 2.72 AU). Its orbit has aneccentricity of 0.16 and aninclination of 6° with respect to theecliptic.[1] The asteroid was first observed asA907 GD at Heidelberg in April 1907. The body'sobservation arc begins at Heidelberg, the night after its official discovery observation.[16]

Naming

[edit]

Thisminor planet was named after the evergreen woody plantHedera ("ivy") a genus of climbing or ground-creeping woody plants in thearalia family (ivy family). Thenaming was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 115).[3]

Reinmuth's flowers

[edit]

Due to his many discoveries,Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between(1009) and(1200). This list also contained a sequence of 28 asteroids, starting with1054 Forsytia, that were all named after plants, in particularflowering plants(also see list of minor planets named after animals and plants).[17]

Physical characteristics

[edit]

Hedera is anE-type andX-type asteroid in theTholen andSMASS classification, respectively.[1]

Rotation period

[edit]

Several rotationallightcurves ofHedera have been obtained from photometric observations since 2007.[8][9][12][13] Best-rated lightcurve byJulian Oey at Kingsgrove and Leura observatories, Australia, gave arotation period of 19.9000 hours with a consolidated brightness amplitude between 0.41 and 0.61magnitude (U=3-).[4][9]

Spin axis

[edit]

Modeled photometric data from the Lowell Photometric Database (LPD) and the robotic BlueEye600 Observatory, gave a concurring period of 19.9020 hours,[10][11] Both studies determined twospin axes of (124.0°, −70.0°) and (266.0°, −62.0°), as well as (271.0°, −53.0°) and (115.0°, −62.0°) inecliptic coordinates (λ, β).[10][11]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Hedera measures 13.239 kilometers in diameter and its surface has analbedo of 0.636.[6][7]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and consequently calculates a larger diameter of 44.22 kilometers based on anabsolute magnitude of 10.50.[4]

References

[edit]
  1. ^abcdefghij"JPL Small-Body Database Browser: 1251 Hedera (1933 BE)" (2017-11-24 last obs.).Jet Propulsion Laboratory. Retrieved31 December 2017.
  2. ^"hederal".Oxford English Dictionary (Online ed.).Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2003). "(1251) Hedera".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 104.doi:10.1007/978-3-540-29925-7_1252.ISBN 978-3-540-00238-3.
  4. ^abcdefg"LCDB Data for (1251) Hedera". Asteroid Lightcurve Database (LCDB). Retrieved31 December 2017.
  5. ^ab"Asteroid 1251 Hedera – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^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.
  7. ^abcdeMainzer, 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.
  8. ^abShevchenko, V. G.; Krugly, Yu. N.; Chiorny, V. G.; Belskaya, I. N.; Gaftonyuk, N. M. (August 2003). "Rotation and photometric properties of E-type asteroids".Planetary and Space Science.51 (9–10):525–532.Bibcode:2003P&SS...51..525S.doi:10.1016/S0032-0633(03)00076-X.
  9. ^abcOey, Julian (September 2008)."Lightcurve Analysis of Asteroids from the Kingsgrove and Leura Observatories in the 2nd Half of 2007"(PDF).Minor Planet Bulletin.35 (3):132–135.Bibcode:2008MPBu...35..132O.ISSN 1052-8091.
  10. ^abcDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573.
  11. ^abcDurech, Josef; Hanus, Josef; Broz, Miroslav; Lehky, Martin; Behrend, Raoul; Antonini, Pierre; et al. (July 2017). "Shape models of asteroids based on lightcurve observations with BlueEye600 robotic observatory".Icarus.304:101–109.arXiv:1707.03637.Bibcode:2018Icar..304..101D.doi:10.1016/j.icarus.2017.07.005.
  12. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1251) Hedera". Geneva Observatory. Retrieved31 December 2017.
  13. ^abChiorny, V. G.; Shevchenko, V. G.; Krugly, Yu. N.; Velichko, F. P.; Gaftonyuk, N. M. (May 2007)."Photometry of asteroids: Lightcurves of 24 asteroids obtained in 1993 2005".Planetary and Space Science.55 (7–8):986–997.Bibcode:2007P&SS...55..986C.doi:10.1016/j.pss.2007.01.001.
  14. ^Belskaya, I. N.; Fornasier, S.; Tozzi, G. P.; Gil-Hutton, R.; Cellino, A.; Antonyuk, K.; et al. (March 2017). "Refining the asteroid taxonomy by polarimetric observations".Icarus.284:30–42.Bibcode:2017Icar..284...30B.doi:10.1016/j.icarus.2016.11.003.hdl:11336/63617.
  15. ^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.
  16. ^ab"1251 Hedera (1933 BE)".Minor Planet Center. Retrieved31 December 2017.
  17. ^Schmadel, Lutz D. (2007). "(1054) Forsytia".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 90.doi:10.1007/978-3-540-29925-7_1055.ISBN 978-3-540-00238-3.

External links

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