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1628 Strobel

From Wikipedia, the free encyclopedia
Main-belt asteroid

1628 Strobel
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date11 September 1923
Designations
(1628) Strobel
Named after
Willi Strobel(astronomer)[2]
1923 OG · 1926 GY
1947 GC · 1949 QA2
1952 DV2 · 1957 CA
1960 WH
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc93.11 yr (34,007 days)
Aphelion3.2152AU
Perihelion2.8088 AU
3.0120 AU
Eccentricity0.0675
5.23yr (1,909 days)
244.38°
0° 11m 18.6s / day
Inclination19.387°
181.19°
289.14°
Physical characteristics
Dimensions51.15±14.91 km[4]
53.147±0.793 km[5]
54.26±16.39 km[6]
56.58±0.68 km[7]
57.06 km(derived)[3]
57.12±1.7 km(IRAS:12)[8]
59.345±0.484 km[9]
9.52±0.01h[10]
11.80 h[11]
0.047±0.010[9]
0.05±0.03[6]
0.0504(derived)[3]
0.0532±0.003(IRAS:12)[8]
0.055±0.002[7]
0.0581±0.0113[5]
0.06±0.04[4]
P[5] · X[12] · C[3]
B–V = 0.840[1]
U–B = 0.320[1]
10.02[1][6][7][8] · 10.08[3][5][11] · 10.31±0.20[12] · 10.32[4]

1628 Strobel (provisional designation1923 OG) is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 55 kilometers in diameter.

It was discovered on 11 September 1923, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany, and named afterARI-astronomerWilli Strobel.[2][13]

Classification and orbit

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Strobel orbits the Sun in theouter main-belt at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,909 days). Its orbit has aneccentricity of 0.07 and aninclination of 19° with respect to theecliptic.[1] Strobel'sobservation arc begins two nights after its official discovery observation at Heidelberg in 1923.[13]

Physical characteristics

[edit]

Strobel is a carbonaceousC-type asteroid. It is also classified as aP-type byWISE and as anX-type asteroid byPan-STARRS.[5][12]

Rotation period

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American astronomerRichard Binzel obtained the first rotationallightcurve of Strobel in May 1984. It gave arotation period of 11.80 hours with a brightness amplitude of 0.22magnitude (U=2).[11] In May 2005, photometric observations by French amateur astronomerLaurent Bernasconi gave a shorter period of 9.52 hours and a brightness change of 0.20 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's Wide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Strobel measures between 51.15 and 59.35 kilometers in diameter, and its surface has analbedo between 0.047 and 0.06.[4][5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0504 and a diameter of 57.06 kilometers with anabsolute magnitude of 10.08.[3]

Naming

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Thisminor planet was named in honor of Willi Strobel (1909–1988), staff member atAstronomisches Rechen-Institut (ARI) since 1938, and author of the 1963-edition ofIdentifizierungsnachweis der Kleinen Planeten (Minor planet identifications, published by ARI).[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3931).[14]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1628 Strobel (1923 OG)" (2016-10-19 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1628) Strobel".Dictionary of Minor Planet Names – (1628) Strobel.Springer Berlin Heidelberg. p. 129.doi:10.1007/978-3-540-29925-7_1629.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1628) Strobel". Asteroid Lightcurve Database (LCDB). Retrieved27 December 2016.
  4. ^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.
  5. ^abcdefMainzer, 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.
  6. ^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. Retrieved27 December 2016.
  7. ^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)
  8. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  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. Retrieved27 December 2016.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1628) Strobel".Geneva Observatory. Retrieved27 December 2016.
  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. Retrieved27 December 2016.
  12. ^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.S2CID 53493339. Retrieved27 December 2016.
  13. ^ab"1628 Strobel (1923 OG)".Minor Planet Center. Retrieved27 December 2016.
  14. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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