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1178 Irmela

From Wikipedia, the free encyclopedia
Stony asteroid

1178 Irmela
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date13 March 1931
Designations
(1178) Irmela
Named after
Irmela Ruska
(wife ofErnst Ruska)[2]
1931 EC · 1940 GC
1962 JD · 1988 CK6
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc85.83 yr (31,351 days)
Aphelion3.1700AU
Perihelion2.1916 AU
2.6808 AU
Eccentricity0.1825
4.39yr (1,603 days)
209.87°
0° 13m 28.56s / day
Inclination6.9511°
170.11°
357.21°
Physical characteristics
Dimensions17.00±3.43 km[4]
17.50±4.91 km[5]
17.90±0.57 km[6]
19.05 km(derived)[3]
19.09±0.8 km(IRAS:15)[7]
19.663±0.049 km[8]
20.683±0.181 km[9]
11.989±0.001 h[10]
19.17h[11]
0.0503±0.0031[9]
0.070±0.006[8]
0.08±0.03[4]
0.08±0.07[5]
0.0838(derived)[3]
0.0916±0.008(IRAS:15)[7]
0.105±0.007[6]
S[3]
11.81[1][4][6][7] · 11.87±0.35[12] · 11.91[3][9][11] · 12.14[5]

1178 Irmela, provisional designation1931 EC, is a stonyasteroid from the middle regions of theasteroid belt, approximately 19 kilometers in diameter.

It was discovered on 13 March 1931, by German astronomerMax Wolf atHeidelberg Observatory in southwest Germany.[13] The asteroid was named after Irmela Ruska, wife ofErnst Ruska.[2]

Orbit and classification

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Irmela orbits the Sun in thecentral main-belt at a distance of 2.2–3.2 AU once every 4 years and 5 months (1,603 days). Its orbit has aneccentricity of 0.18 and aninclination of 7° with respect to theecliptic.[1]A firstprecovery was taken atLowell Observatory in February 1931, extending the body'sobservation arc by 3 weeks prior to its official discovery observation at Heidelberg.[13]

Physical characteristics

[edit]

Lightcurves

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In May 1984, a first rotationallightcurve ofIrmela was obtained from photometric observations by American astronomerRichard Binzel. Lightcurve analysis gave arotation period of 19.17 hours with a brightness variation of 0.34magnitude (U=2).[11]

In March 2010, astronomerRobert Stephens obtained another lightcurve at the Center for Solar System Studies, that gave a divergent period of 11.989 hours with an amplitude of 0.40 magnitude (U=2).[10]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Irmela measures between 17.00 and 20.683 kilometers in diameter and its surface has analbedo between 0.0503 and 0.105.[4][5][6][7][8][9]

10μm radiometric data collected fromKitt Peak National Observatory in 1975, gave a diameter estimate of 19 kilometers.[14]

TheCollaborative Asteroid Lightcurve Link characterizesIrmela as a commonS-type asteroid, derives an albedo of 0.0838 and calculates a diameter of 19.05 kilometers with anabsolute magnitude of 11.91.[3]

Naming

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Thisminor planet was named after Irmela Ruska, wife of the inventor of the electron microscope and 1986 Nobelist, the German physicistErnst Ruska (1906–1988), who shared the Nobel prize withGerd Binnig andHeinrich Rohrer. The naming was granted by Max Wolf to his colleagueAugust Kopff, himself a prolificdiscoverer of minor planets. The citation was published byPaul Herget inThe Names of the Minor Planets (H 109).[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1178 Irmela (1931 EC)" (2016-12-22 last obs.).Jet Propulsion Laboratory. Retrieved2 May 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1178) Irmela".Dictionary of Minor Planet Names – (1178) Irmela.Springer Berlin Heidelberg. p. 99.doi:10.1007/978-3-540-29925-7_1179.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1178) Irmela". Asteroid Lightcurve Database (LCDB). Retrieved2 May 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.S2CID 9341381.
  5. ^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.
  6. ^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)
  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. ^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.
  9. ^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.
  10. ^abStephens, Robert D. (April 2012). "Asteroids Observed from GMARS and Santana Observatories: 2011 October- December".The Minor Planet Bulletin.39 (2):80–82.Bibcode:2012MPBu...39...80S.ISSN 1052-8091.
  11. ^abcBinzel, R. P. (October 1987). "A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035.
  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.
  13. ^ab"1178 Irmela (1931 EC)".Minor Planet Center. Retrieved2 May 2017.
  14. ^Morrison, D.; Chapman, C. R. (March 1976), "Radiometric diameters for an additional 22 asteroids",Astrophysical Journal,204:934–939,Bibcode:1976ApJ...204..934M,doi:10.1086/154242

External links

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