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1250 Galanthus

From Wikipedia, the free encyclopedia
Main-belt asteroid

1250 Galanthus
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date25 January 1933
Designations
(1250) Galanthus
Pronunciation/ɡəˈlænθəs/[2]
Named after
Galanthus (snowdrop)
(herbaceous plants)[3]
1933 BD · 1971 OQ
main-belt · (middle)
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc84.84 yr (30,987 days)
Aphelion3.2465AU
Perihelion1.8560 AU
2.5513 AU
Eccentricity0.2725
4.08yr (1,488 days)
249.60°
0° 14m 30.84s / day
Inclination15.169°
292.02°
217.17°
Physical characteristics
Dimensions17.18±5.39 km[5]
19.394±0.152 km[6]
19.54±0.36 km[7]
20.062±0.112 km[8]
20.33±4.93 km[9]
21.00±2.9 km[10]
3.918±0.0009h[11]
3.92 h[12]
0.04±0.02[9]
0.0443±0.0069[6]
0.0500±0.017[10]
0.055±0.011[8]
0.058±0.002[7]
0.06±0.04[5]
C(assumed)[13]
12.233±0.001(R)[11] · 12.26[1][5][6][7][10][13] · 12.52[9]

1250 Galanthus, provisional designation1933 BD, is a dark backgroundasteroid from the central regions of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 25 January 1933, by German astronomerKarl Reinmuth at theHeidelberg Observatory.[14] The asteroid was named for the herbaceous plantGalanthus, also known as "snowdrop".[3]

Orbit and classification

[edit]

Galanthus is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in thecentral main-belt at a distance of 1.9–3.2 AU once every 4 years and 1 month (1,488 days;semi-major axis of 2.55 AU). Its orbit has aneccentricity of 0.27 and aninclination of 15° with respect to theecliptic.[1] The body'sobservation arc begins at Heidelberg the night after its official discovery observation.[14]

Physical characteristics

[edit]

Galanthus is an assumed carbonaceousC-type asteroid.[13]

Rotation period

[edit]

In the early 1980s, a rotationallightcurve ofGalanthus was obtained during a survey conducted byRichard P. Binzel at theMcDonald Observatory, Texas. Lightcurve analysis gave a well-definedrotation period of 3.92 hours with a brightness variation of 0.28magnitude (U=3).[12] The period was confirmed from photometric observations by astronomers at thePalomar Transient Factory in October 2015, which gave a similar period of 3.918 hours and an amplitude of 0.22 magnitude (U=2).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Galanthus measures between 17.18 and 21.00 kilometers in diameter and its surface has analbedo between 0.04 and 0.06.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0500 and a diameter of 21.0 kilometers based on anabsolute magnitude of 12.26.[13]

Naming

[edit]

Thisminor planet was named after the herbaceous plantGalanthus, also known as "snowdrop".[3] The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 115).[3]

Reinmuth's flowers

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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).[15]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1250 Galanthus (1933 BD)" (2017-11-27 last obs.). Jet Propulsion Laboratory. Retrieved31 December 2017.
  2. ^"Galanthus".Merriam-Webster.com Dictionary. Merriam-Webster.
  3. ^abcdSchmadel, Lutz D. (2003). "(1250) Galanthus".Dictionary of Minor Planet Names – (1250) Galanthus. Springer Berlin Heidelberg. p. 102.doi:10.1007/978-3-540-29925-7_1251.ISBN 978-3-540-00238-3.
  4. ^ab"Asteroid 1250 Galanthus – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved31 December 2017.
  6. ^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.S2CID 35447010.
  7. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  8. ^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.S2CID 119293330.
  9. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  10. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  11. ^abcWaszczak, 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.S2CID 8342929. Retrieved31 December 2017.
  12. ^abBinzel, R. P.; Mulholland, J. D. (December 1983)."A photoelectric lightcurve survey of small main belt asteroids".Icarus.56 (3):519–533.Bibcode:1983Icar...56..519B.doi:10.1016/0019-1035(83)90170-7.ISSN 0019-1035. Retrieved31 December 2017.
  13. ^abcd"LCDB Data for (1250) Galanthus". Asteroid Lightcurve Database (LCDB). Retrieved31 December 2017.
  14. ^ab"1250 Galanthus (1933 BD)".Minor Planet Center. Retrieved31 December 2017.
  15. ^Schmadel, Lutz D. (2007). "(1054) Forsytia".Dictionary of Minor Planet Names – (1054) Forsytia. Springer Berlin Heidelberg. p. 90.doi:10.1007/978-3-540-29925-7_1055.ISBN 978-3-540-00238-3.

External links

[edit]
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