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1082 Pirola

From Wikipedia, the free encyclopedia
Asteroid

1082 Pirola
Modelled shape ofPirola from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date28 October 1927
Designations
(1082) Pirola
Pronunciation/ˈpɪrələ/[2]
Named after
Pyrola (wintergreen)
(herbaceous plant)[3]
1927 UC · 1931 JQ
1951 AH · 1952 DS
1971 YJ · A916 UP
main-belt[1][4] · (outer)
Themis[5][6][7]
Orbital characteristics[4]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc90.01 yr (32,875 days)
Aphelion3.6858AU
Perihelion2.5553 AU
3.1205 AU
Eccentricity0.1811
5.51yr (2,013 days)
130.74°
0° 10m 43.68s / day
Inclination1.8524°
148.01°
187.23°
Physical characteristics
37.363±1.036 km[8]
39.14±13.91 km[9]
41.47±12.07 km[10]
42.607±0.476 km[11]
42.61±0.48 km[11]
44.67±0.71 km[12]
15.85±0.01 h[13]
15.851±0.0140 h[14]
15.8525±0.0005 h[15]
15.8540±0.0001 h[16]
  • (123.0°, −42.0°) (λ11)[6]
  • (300.0°, −38.0°) (λ22)[6]
0.052±0.006[17]
0.06±0.05[9][10]
0.061±0.002[12]
0.067±0.008[11]
0.0867±0.0105[8]
10.4[1][4][8][9][11][12] · 10.450±0.002(R)[14] · 10.507±0.014[15] · 10.51[5] · 10.53[10]

1082 Pirola/ˈpɪrələ/ is a darkThemistian asteroid from the outer regions of theasteroid belt. It was discovered on 28 October 1927, by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in Germany, and assigned theprovisional designation1927 UC.[1] The carbonaceousC-type asteroid has arotation period of 15.9 hours and measures approximately 41 kilometers (25 miles) in diameter. It was named after the herbaceous plantPyrola (wintergreen).[3]

Orbit and classification

[edit]

When applying thehierarchical clustering method to itsproper orbital elements,Pirola is a Themistian asteroid that belongs to theThemis family (602),[18][6][7] a largefamily of nearly 6,000 known carbonaceous asteroids, named after24 Themis.[19]: 23  It orbits the Sun in theouter main belt at a distance of 2.6–3.7 AU once every 5 years and 6 months (2,013 days;semi-major axis of 3.12 AU). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[4] The asteroid was first identified asA916 UP atSimeiz Observatory in October 1916. The body'sobservation arc begins with its official discovery observation at Heidelberg in October 1927.[1]

Naming

[edit]

Thisminor planet was named afterPyrola, also known aswintergreen, a herbaceous plant (mostly evergreen), that belongs to theflowering herbs. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 102).[3]

Reinmuth's flowers

[edit]

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).[20](Unusually thePirola has lent its name to aCOVID-19 variant:BA.2.86.[21])

Physical characteristics

[edit]

In theTholen classification,Pirola is a carbonaceousC-type asteroid,[4][5] which matches the overallspectral type of the Themis family.[19]: 23 

Rotation period

[edit]

In 2010, three rotationallightcurves ofPirola were obtained from photometric observations. Lightcurve analysis gave arotation period of 15.85, 15.851 and 15.8525 hours with a brightness amplitude between 0.53 and 0.62magnitude (U=3-/2/3).[13][14][15]

A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database, gave a concurring period of 15.8540 hours, as well as twospin axis of (123.0°, −42.0°) and (300.0°, −38.0°) inecliptic coordinates (λ, β).[16]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Pirola measures between 37.363 and 44.67 kilometers in diameter and its surface has analbedo between 0.052 and 0.0867.[8][9][10][11][12][17] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0655 and a diameter of 41.06 kilometers based on anabsolute magnitude of 10.51.[5]

References

[edit]
  1. ^abcde"1082 Pirola (1927 UC)".Minor Planet Center. Retrieved28 November 2017.
  2. ^"pyrola, pirola".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1082) Pirola".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 92.doi:10.1007/978-3-540-29925-7_1083.ISBN 978-3-540-00238-3.
  4. ^abcdefgh"JPL Small-Body Database Browser: 1082 Pirola (1927 UC)" (2017-10-30 last obs.).Jet Propulsion Laboratory. Retrieved28 November 2017.
  5. ^abcde"LCDB Data for (1082) Pirola". Asteroid Lightcurve Database (LCDB). Retrieved28 November 2017.
  6. ^abcd"Asteroid 1082 Pirola – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  7. ^abZappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997)."Asteroid Dynamical Families".NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. Retrieved4 March 2020. (PDS main page)
  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. ^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.
  10. ^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.
  11. ^abcdeMasiero, 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.
  12. ^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)
  13. ^abGartrelle, Gordon M. (April 2012). "Lightcurve Results for Eleven Asteroids".The Minor Planet Bulletin.39 (2): 40%–46.Bibcode:2012MPBu...39...40G.ISSN 1052-8091.
  14. ^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.
  15. ^abcBaker, Ronald E.; Pilcher, Frederick; Benishek, Vladimir (April 2011). "Photometric Observations and Analysis of 1082 Pirola".The Minor Planet Bulletin.38 (2):111–114.Bibcode:2011MPBu...38..111B.ISSN 1052-8091.
  16. ^abDurech, 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.
  17. ^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.
  18. ^"Asteroid 1082 Pirola – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved13 March 2020.
  19. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  20. ^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.
  21. ^"What we know about the new COVID strain nicknamed after an asteroid". 19 August 2023 – via www.abc.net.au.

External links

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