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1112 Polonia

From Wikipedia, the free encyclopedia
Eoan asteroid
Not to be confused with142 Polana.

1112 Polonia
Discovery[1]
Discovered byP. Shajn
Discovery siteSimeiz Obs.
Discovery date15 August 1928
Designations
(1112) Polonia
Pronunciation/pˈlniə/[2]
Named after
Poland
(European country)[3]
1928 PE · 1933 PA
A908 XA
main-belt[1][4] · (outer)
Eos[5][6]
Orbital characteristics[4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc89.20yr (32,582 d)
Aphelion3.3423AU
Perihelion2.6963 AU
3.0193 AU
Eccentricity0.1070
5.25 yr (1,916 d)
326.70°
0° 11m 16.44s / day
Inclination8.9911°
302.86°
87.361°
Physical characteristics
35.76±1.6 km[7]
37.55±0.60 km[8]
39.661±0.334 km[9]
47.058±0.368 km[10]
82.5±0.5 h[11][a]
0.0763±0.0097[10]
0.097±0.023[9]
0.128±0.005[8]
0.1319±0.012[7]
S(Tholen)[4]
L(SDSS-MOC)[12]
B–V = 0.797[4]
U–B = 0.447[4]
10.05[4][6][7][8][10]

1112 Polonia (provisional designation1928 PE) is anEoan asteroid from the outer regions of theasteroid belt, approximately 38 kilometers (24 miles) in diameter. Discovered by Soviet astronomerPelageya Shajn atSimeiz in 1928,[1] it was the first asteroid discovery made by a woman.[3] TheL-type asteroid has a longrotation period of 82.5 hours,[6] and was named for the country ofPoland.[3]

Discovery

[edit]

Polonia was first observed asA908 XA at the GermanHeidelberg Observatory in December 1908. It was officially discovered on 15 August 1928, by Soviet astronomerPelageya Shajn at theSimeiz Observatory on the Crimean peninsula.[1] On the following night at Simeis, it was independently discovered by her collegeGrigory Neujmin.[3] TheMinor Planet Center only recognized the first discoverer.[1]

Polonia was Shajn's first discovery; and the first asteroid discovery made by a woman,[3] bringing a long-standing tradition – which began with the discovery of1 Ceres in 1801 – of more than athousand minor planet discoveries exclusively made bymale astronomers, to an end.

Orbit and classification

[edit]

Polonia is a core member of theEos family (606),[5][6] the largestasteroid family of theouter main belt consisting of nearly 10,000 asteroids.[13]

It orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,916 days;semi-major axis of 3.02 AU). Its orbit has aneccentricity of 0.11 and aninclination of 9° with respect to theecliptic.[4] The body'sobservation arc begins with its official discovery observation at Simeiz in 1928.[1]

Physical characteristics

[edit]

In theTholen classification, Polonia is a common, stonyS-type asteroid.[4] In the more refinedSDSS-based taxonomy, it is characterized as an uncommonL-type,[12] which is similar to aK-type, the overallspectral type of the Eoan asteroids.[13]: 23 

Rotation period

[edit]

In October 2007, a rotationallightcurve of Polonia was obtained fromphotometric observations by American astronomerBrian Warner at hisPalmer Divide Observatory in Colorado. Lightcurve analysis gave a longrotation period of 82.5 hours with a brightness amplitude of 0.20magnitude (U=2).[6][11][a] The asteroid's long period is close to that of aslow rotator.

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Polonia measures between 35.76 and 47.058 kilometers in diameter and its surface has analbedo between 0.0763 and 0.1319.[7][8][9][10] TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.1319 and a diameter of 35.76 kilometers based on anabsolute magnitude of 10.05.[6]

Naming

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Thisminor planet was named "Polonia", theLatin name for the European country ofPoland. It is the first minor planet discovery made by a woman. The naming was proposed by L. Matkiewicz, an astronomer of Polish origin, who calculated the body's orbit. The official citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 104).[3]

Notes

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  1. ^abLightcurve plot of 1(1112) Polonia, Palmer Divide Observatory,B. D. Warner (2007). Rotation period82.5±0.5 hours with a brightness amplitude of0.20±0.03 mag. Quality code is 2. Summary figures at theLCDB.

References

[edit]
  1. ^abcdef"1112 Polonia (1928 PE)".Minor Planet Center. Retrieved29 May 2018.
  2. ^"Polonia".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcdefSchmadel, Lutz D. (2007). "(1112) Polonia".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 94.doi:10.1007/978-3-540-29925-7_1113.ISBN 978-3-540-00238-3.
  4. ^abcdefgh"JPL Small-Body Database Browser: 1112 Polonia (1928 PE)" (2017-10-29 last obs.).Jet Propulsion Laboratory. Retrieved29 May 2018.
  5. ^ab"Asteroid 1112 Polonia".Small Bodies Data Ferret. Retrieved29 May 2018.
  6. ^abcdef"LCDB Data for (1112) Polonia". Asteroid Lightcurve Database (LCDB). Retrieved29 May 2018.
  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. ^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)
  9. ^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.
  10. ^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. (catalog)
  11. ^abWarner, Brian D. (June 2008). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: September-December 2007".The Minor Planet Bulletin.35 (2):67–71.Bibcode:2008MPBu...35...67W.ISSN 1052-8091.
  12. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  13. ^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.S2CID 119280014.

External links

[edit]
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Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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