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1054 Forsytia

From Wikipedia, the free encyclopedia
Dark background asteroid

1054 Forsytia
Shape model ofForsytia from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date20 November 1925
Designations
(1054) Forsytia
Pronunciation/fɔːrˈsɪtiə/[2]
Named after
Forsythia(flowering plant)[3]
1925 WD · 1962 DD
A907 EA
main-belt · (outer)[4]
background[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.32 yr (40,295 days)
Aphelion3.3198AU
Perihelion2.5284 AU
2.9241 AU
Eccentricity0.1353
5.00yr (1,826 days)
165.01°
0° 11m 49.56s / day
Inclination10.849°
85.888°
294.19°
Physical characteristics
Dimensions42.867±11.18 km[6]
45.42 km(derived)[4]
45.47±4.3 km[7]
46.40±13.38 km[8]
46.69±15.08 km[9]
47.780±3.344 km[10]
53.04±0.71 km[11]
7.650±0.001h[12]
0.035±0.013[10]
0.04±0.07[8]
0.048±0.002[11]
0.05±0.03[9]
0.0592(derived)[4]
0.0648±0.014[7]
0.0750±0.0441[6]
C(assumed)[4]
10.12[6] · 10.12±0.51[13] · 10.30[7][11] · 10.40[1][4][9] · 10.46[8] · 10.87[10]

1054 Forsytia/fɔːrˈsɪtiə/ is a darkbackground asteroid, approximately 46 kilometers in diameter, from the outer regions of theasteroid belt. It was discovered on 20 November 1925, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany and assigned provisional designation1925 WD.[14] It is named after the flowering plantforsythia, and marks the beginning of a sequence of 28 thematically named asteroids by the discoverer.[3]

Orbit and classification

[edit]

Forsytia is a non-family asteroid from the main belt'sbackground population.[5] It orbits the Sun in theouter asteroid belt at a distance of 2.5–3.3 AU once every 5.00 years (1,826 days;semi-major axis of 2.92 AU). Its orbit has aneccentricity of 0.14 and aninclination of 11° with respect to theecliptic.[1] The asteroid was first observed asA907 EA at Heidelberg in March 1907. The body'sobservation arc begins with its official discovery observation in November 1925.[14]

Naming

[edit]

Thisminor planet was named afterforsythia, a genus of flowering shrubs in the familyOleaceae. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 100).[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 with this asteroid, that were all named after plants, in particularflowering plants(also see list of minor planets named after animals and plants).[3]

Physical characteristics

[edit]

Forsytia is an assumed carbonaceousC-type asteroid.[4]

Rotation period

[edit]

In March 2002, a rotationallightcurve ofForsytia was obtained from photometric observations by American amateur astronomerJohn Gross at his Sonoran Skies Observatory (G94) in Arizona. Lightcurve analysis gave a well-definedrotation period of 7.650 hours with a brightness amplitude of 0.23magnitude (U=3).[12]

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,Forsytia measures between 42.867 and 53.04 kilometers in diameter and its surface has analbedo between 0.035 and 0.0750.[6][7][8][9][10][11] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0592 and a diameter of 45.42 kilometers based on anabsolute magnitude of 10.4.[4]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1054 Forsytia (1925 WD)" (2017-07-02 last obs.). Jet Propulsion Laboratory. Retrieved10 January 2018.
  2. ^Sunset Western Garden Book, 1995:606–607
  3. ^abcdSchmadel, 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.
  4. ^abcdefg"LCDB Data for (1054) Forsytia". Asteroid Lightcurve Database (LCDB). Retrieved10 January 2018.
  5. ^ab"Asteroid 1054 Forsytia – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  6. ^abcdMasiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos".The Astronomical Journal.154 (4): 10.arXiv:1708.09504.Bibcode:2017AJ....154..168M.doi:10.3847/1538-3881/aa89ec.
  7. ^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.
  8. ^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.
  9. ^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.
  10. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.
  11. ^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)
  12. ^abGross, John (September 2003). "Sonoran Skies Observatory lightcurve results for asteroids 1054, 1390, 1813 1838, 2988, 3167, 4448, and 5262".The Minor Planet Bulletin.30 (3):44–46.Bibcode:2003MPBu...30...44G.ISSN 1052-8091.
  13. ^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.S2CID 53493339.
  14. ^ab"1054 Forsytia (1925 WD)".Minor Planet Center. Retrieved10 January 2018.

External links

[edit]
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