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1132 Hollandia

From Wikipedia, the free encyclopedia
Asteroid

1132 Hollandia
1132 Hollandia
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
(Leiden Southern Station)
Discovery date13 September 1929
Designations
(1132) Hollandia
Pronunciation/hɒˈlændiə/
Named after
Holland(part of TheNetherlands)[2]
1929 RB1 · 1942 NC
1946 JA · 1951 WA
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc86.74 yr (31,680 days)
Aphelion3.4238AU
Perihelion1.9498 AU
2.6868 AU
Eccentricity0.2743
4.40yr (1,609 days)
335.62°
0° 13m 25.68s / day
Inclination7.2217°
29.624°
270.51°
Physical characteristics
Dimensions20.48±5.58 km[4]
25.32 km(calculated)[3]
27.235±0.116 km[5]
27.36±0.66 km[6]
27.59±0.78 km[7]
27.727±0.313 km[8]
5.326±0.015 h[9]
5.360±0.001h[10]
5.568±0.005 h[11]
0.086±0.013[6]
0.10(assumed)[3]
0.12±0.06[4]
0.1328±0.0221[8]
0.135±0.008[7]
S[3]
10.60[7][8] · 11.1[1][3][4][6] · 11.12±0.50[12]

1132 Hollandia, provisional designation1929 RB1, is a stonyasteroid from the middle region of theasteroid belt, approximately 27 kilometers in diameter. It was discovered on 13 September 1929, by Dutch astronomerHendrik van Gent at Leiden Southern Station, annex to theJohannesburg Observatory in South Africa.[13] It was named for the regionHolland in the Netherlands.[2]

Classification and orbit

[edit]

Hollandia is an assumed stonyS-type asteroid. It orbits the Sun at a distance of 1.9–3.4 AU once every 4 years and 5 months (1,609 days). Its orbit has aneccentricity of 0.278 and aninclination of 7° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation as noprecoveries were taken and no prior identifications were made.[13]

Physical characteristics

[edit]

Between 2003 and 2014, three rotationallightcurves ofHollandia were obtained from photometric observations taken by French amateur astronomerRené Roy, Jason Sauppe atOakley Observatory and Maurice Clark atTTU's Preston Gott Observatory. Lightcurve analysis gave arotation period between 5.360 and 5.568 hours with a brightness variation of 0.15–0.35magnitude (U=2+/2+/2+).[9][10][11]

According to the surveys carried out by the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Hollandia measures between 20.48 and 27.727 kilometers in diameter, and its surface has analbedo between 0.086 and 0.135.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 – a compromise value that lies in between the albedos forcarbonaceous (0.057) and forstony (0.20) asteroids – and calculates a diameter of 25.32 kilometers using anabsolute magnitude of 11.1.[3]

Naming

[edit]

Thisasteroid was named after the Latin name forThe Netherlands, a region in theEuropean Union.[2] Naming citation was first published byPaul Herget inThe Names of the Minor Planets in 1955 (H 106).[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1132 Hollandia (1929 RB1)" (2016-06-08 last obs.).Jet Propulsion Laboratory. Retrieved1 February 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1132) Hollandia".Dictionary of Minor Planet Names – (1132) Hollandia.Springer Berlin Heidelberg. p. 96.doi:10.1007/978-3-540-29925-7_1133.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1132) Hollandia". Asteroid Lightcurve Database (LCDB). Retrieved1 February 2017.
  4. ^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. Retrieved1 February 2017.
  5. ^abMasiero, 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. Retrieved1 February 2017.
  6. ^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. Retrieved1 February 2017.
  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. ^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. ^abSauppe, Jason; Torno, Steven; Lemke-Oliver, Robert; Ditteon, Richard (December 2007)."Asteroid Lightcurve Analysis at the Oakley Observatory - March/April 2007".The Minor Planet Bulletin.34 (4):119–122.Bibcode:2007MPBu...34..119S.ISSN 1052-8091. Retrieved1 February 2017.
  10. ^abClark, Maurice (January 2015)."Asteroid Photometry from the Preston Gott Observatory".The Minor Planet Bulletin.42 (1):15–20.Bibcode:2015MPBu...42...15C.ISSN 1052-8091. Retrieved1 February 2017.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1132) Hollandia".Geneva Observatory. Retrieved1 February 2017.
  12. ^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. Retrieved1 February 2017.
  13. ^ab"1132 Hollandia (1929 RB1)".Minor Planet Center. Retrieved1 February 2017.

External links

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