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1152 Pawona

From Wikipedia, the free encyclopedia
Main-belt asteroid

1152 Pawona
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date8 January 1930
Designations
(1152) Pawona
Named after
Johann Palisa
andMax Wolf
(minor planet discoverers)[2]
1930 AD · 1926 AK
1942 GE1 · 1942 GY
1969 MD · A924 QA
main-belt · Vestian[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc92.61 yr (33,825 days)
Aphelion2.5288AU
Perihelion2.3256 AU
2.4272 AU
Eccentricity0.0419
3.78yr (1,381 days)
356.07°
0° 15m 38.16s / day
Inclination5.0797°
331.91°
218.56°
Physical characteristics
Dimensions15.69±1.0 km[4]
15.90 km(derived)[3]
16.35±0.31 km[5]
17.130±0.115 km[6]
18.826±0.090 km[7]
3.41500±0.00005h[8]
3.4151±0.0009 h[9]
3.4154±0.0001 h[8]
3.418±0.005 h[10][a]
3.425±0.001 h[11]
0.1529±0.0174[7]
0.203±0.004[6]
0.205±0.009[5]
0.2167±0.030[4]
0.2782(derived)[3]
SMASS =Sl[1] · S[3]
11.0[3] · 11.18±0.01[12] · 11.2[1] · 11.30[4][5][7]

1152 Pawona, provisional designation1930 AD, is a stony Vestianasteroid from the inner regions of theasteroid belt, approximately 16 kilometers in diameter. Discovered byKarl Reinmuth atHeidelberg Observatory in 1930, the asteroid was named in honor of astronomersJohann Palisa andMax Wolf.[13]

Discovery

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Pawona was discovered on 8 January 1930, by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[13] It was independently discovered by Italian astronomerLuigi Volta at theObservatory of Turin on 19 January 1930, and byGrigory Neujmin at theSimeiz Observatory on the Crimean peninsula on 21 January 1930.[2] TheMinor Planet Center, however, only acknowledges the first discoverer.[13]

The asteroid was first identified asA924 QA atVienna Observatory in August 1924. The body'sobservation arc begins with its identification as1926 AK at Heidelberg in January 1926, almost 4 years prior to its official discovery observation.[13]

Orbit and classification

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Pawona is a supposed member of the stonyVesta family (401), named after4 Vesta and the main belt's second-largestasteroid family by number.[3] It orbits the Sun in theinner main-belt at a distance of 2.3–2.5 AU once every 3 years and 9 months (1,381 days). Its orbit has aneccentricity of 0.04 and aninclination of 5° with respect to theecliptic.[1]

Physical characteristics

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In theSMASS classification,Pawona is an Sl-subtype, that transitions from the common stonyS-type to the rareL-type asteroids.[1]

Rotation period

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Several rotationallightcurves ofPawona have been obtained from photometric observations since 2002. Analysis of these lightcurves gave a well-definedrotation period between 3.415 and 3.425 hours with a brightness amplitude of 0.16 to 0.26magnitude (U=3/3/3/3/3).[8][9][10][11][a]

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,Pawona measures between 15.69 and 18.826 kilometers in diameter and its surface has analbedo between 0.1529 and 0.2167.[4][5][6][7]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2782 and a diameter of 15.90 kilometers based on anabsolute magnitude of 11.0.[3]

Naming

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Thisminor planet was named after astronomersJohann Palisa andMax Wolf, two prolificdiscoverers of minor planets, in recognition of their cooperation. The name was proposed by Swedish astronomer Bror Ansgar Asplind. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 107).[2]

Feminization of names

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Pawona is a combination of "Palisa" and "Wolf" (Pa, Wo) joined with a Latin feminine suffix. The custom of adding the female endings "a" or "ia" to male names had only faded out by World War II and was finally abolished in 1947, when theMinor Planet Center took over responsibility of numbering and naming asteroids.[14]

Notes

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  1. ^abLightcurve plot of (1152) Pawona, Robert Koff, Antelope Hills Observatory (H09). Summary figures atLCDB

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1152 Pawona (1930 AD)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved8 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1152) Pawona".Dictionary of Minor Planet Names – (1152) Pawona.Springer Berlin Heidelberg. p. 97.doi:10.1007/978-3-540-29925-7_1153.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1152) Pawona". Asteroid Lightcurve Database (LCDB). Retrieved8 September 2017.
  4. ^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.
  5. ^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)
  6. ^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. Retrieved8 September 2017.
  7. ^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 118700974.
  8. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1152) Pawona".Geneva Observatory. Retrieved8 September 2017.
  9. ^abSchmidt, Richard E. (July 2017)."Near-IR Minor Planet Photometry from Burleith Observatory".The Minor Planet Bulletin.44 (3):191–192.Bibcode:2017MPBu...44..191S.ISSN 1052-8091. Retrieved8 September 2017.
  10. ^abKoff, R. A.; Clark, M. (September 2002)."Lightcurve Photometry of 1152 Pawona".The Minor Planet Bulletin.29:49–50.Bibcode:2002MPBu...29...49K. Retrieved8 September 2017.
  11. ^abKlinglesmith, Daniel A. III; Hendrickx, Sebastian; Kimber, Cameron; Madden, Karl (July 2017)."CCD Asteroid Photometry from Etscorn Observatory".The Minor Planet Bulletin.44 (3):244–246.Bibcode:2017MPBu...44..244K.ISSN 1052-8091. Retrieved8 September 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.S2CID 53493339. Retrieved8 September 2017.
  13. ^abcd"1152 Pawona (1930 AD)".Minor Planet Center. Retrieved8 September 2017.
  14. ^Peebles, Curtis (2000)."The attack of the classicists".Asteroids: A History.Smithsonian Institution Press.ISBN 978-1-56098-982-0.

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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