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1165 Imprinetta

From Wikipedia, the free encyclopedia
Carbonaceous Meliboean asteroid

1165 Imprinetta
Shape model ofImprinetta from itslightcurve
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
(Leiden Southern Station)
Discovery date24 April 1930
Designations
(1165) Imprinetta
Pronunciation/ˌɪmprɪˈnɛtə/
Named after
Imprinetta Gent
(wife of the discoverer)[2]
1930 HM · A909 TA
main-belt · (outer)[3]
Meliboea[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc107.47 yr (39,253 days)
Aphelion3.7891AU
Perihelion2.4589 AU
3.1240 AU
Eccentricity0.2129
5.52yr (2,017 days)
221.92°
0° 10m 42.6s / day
Inclination12.812°
203.79°
96.959°
Physical characteristics
Dimensions47.14±15.99 km[5]
48.65 km(derived)[3]
48.82±1.9 km[6]
50.30±14.80 km[7]
53.187±0.325 km[8]
53.40±1.62 km[9]
56.44±0.87 km[10]
59.378±0.290 km[11]
7.9374±0.0016h[12]
8.107±0.010 h[13]
0.029±0.005[10]
0.0380±0.0055[11]
0.0392(derived)[3]
0.04±0.02[5]
0.04±0.03[7]
0.047±0.003[9]
0.048±0.002[8]
0.0562±0.005[6]
C[3][14]
10.30[6][9][11] · 10.69±0.38[14] · 10.70[1][3][5][7][10]

1165 Imprinetta, provisional designation1930 HM, is a carbonaceous Meliboeanasteroid from the outer regions of theasteroid belt, approximately 49 kilometers (30 mi) in diameter. It was discovered on 24 April 1930 by Dutch astronomerHendrik van Gent at theUnion Observatory in Johannesburg, South Africa.[15] The asteroid was named after Imprinetta Gent, wife of the discoverer.[2]

Orbit and classification

[edit]

Imprinetta is a member of theMeliboea family, a smallerasteroid family of carbonaceous outer-belt asteroids with a few hundred members, named after137 Meliboea.[4][16]: 23 

This asteroid orbits the Sun in theouter main-belt at a distance of 2.5–3.8 AU once every 5 years and 6 months (2,017 days). Its orbit has aneccentricity of 0.21 and aninclination of 13° with respect to theecliptic.[1]

The body'sobservation arc begins with its first identification asA909 TA atHeidelberg Observatory in October 1909, more than 20 years prior to its official discovery observation at Johannesburg.[15]

Physical characteristics

[edit]

Imprinetta has been characterized as a carbonaceousC-type asteroid byPanSTARRS photometric survey,[3][14] which corresponds with the overallspectral type of the Meliboea family.[16]: 23 

Rotation period

[edit]

In October 2003, a rotationallightcurve ofImprinetta was obtained from photometric observations by American John Menke at his observatory in Barnesville, Maryland. Lightcurve analysis gave a well-definedrotation period of 8.107 hours with a brightness variation of 0.20magnitude (U=3).[13] An alternative observation gave a lightcurve with period of 7.9374 hours and an amplitude of 0.20 magnitude (U=2).[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,Imprinetta measures between 47.14 and 59.378 kilometers (29.291 and 36.896 mi) in diameter and its surface has analbedo between 0.029 and 0.0562.[5][6][7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0392 and a diameter of 48.65 kilometers (30.23 mi) based on anabsolute magnitude of 10.7.[3]

Naming

[edit]

Thisminor planet was named after Imprinetta Gent, wife of the discoverer. The naming was proposed by the discoverer and byGerrit Pels, who computed its orbit. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 108).[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1165 Imprinetta (1930 HM)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved6 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1165) Imprinetta".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 98.doi:10.1007/978-3-540-29925-7_1166.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1165) Imprinetta". Asteroid Lightcurve Database (LCDB). Retrieved6 September 2017.
  4. ^ab"Asteroid 1165 Imprinetta – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved31 October 2019.
  5. ^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. Retrieved6 September 2017.
  6. ^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.
  7. ^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.
  8. ^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. Retrieved6 September 2017.
  9. ^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)
  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. Retrieved6 September 2017.
  11. ^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.
  12. ^abMonson, Andy; Kipp, Steven (December 2004)."Corrigendum: Rotational periods of asteroids 1165 Imprinetta, 1299 Mertona 1645 Waterfield, 1833 Shmakova, 2313 Aruna, and (13856) 1999 XZ105".The Minor Planet Bulletin.31 (4): 97.Bibcode:2004MPBu...31...97M.ISSN 1052-8091. Retrieved6 September 2017.
  13. ^abMenke, John L. (September 2005)."Lightcurves and periods for asteroids 471 Papagena, 675 Ludmilla, 1016 Anitra, 1127 Mimi, 1165 Imprinetta, 1171 Rustahawelia, and 2283 Bunke".The Minor Planet Bulletin.32 (3):64–66.Bibcode:2005MPBu...32...64M.ISSN 1052-8091. Retrieved6 September 2017.
  14. ^abcVeres, 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. Retrieved6 September 2017.
  15. ^ab"1165 Imprinetta (1930 HM)".Minor Planet Center. Retrieved6 September 2017.
  16. ^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.

External links

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