155 Scylla

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155 Scylla
000155-asteroid shape model (155) Scylla.png
3D convex shape model of 155 Scylla
Discovery [1]
Discovered by J. Palisa
Discovery site Austrian Naval Obs.
Discovery date8 November 1875
Designations
(155) Scylla
Pronunciation /ˈsɪlə/ [2]
Named after
Scylla (Greek mythology) [3]
A875 VE; 1907 TJ;
1930 UN; 1930 XS;
1934 RU; 1939 TK;
1941 HL; 1950 FL;
1950 FN
main-belt [1] [4]  ·(middle)
background [5]
Symbol Scylla symbol (fixed width).svg
Orbital characteristics [4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc 142.38 yr (52,004 d)
Aphelion 3.5207 AU
Perihelion 1.9916 AU
2.7562 AU
Eccentricity 0.2774
4.58 yr (1,671 d)
2.9234°
0° 12m 55.44s / day
Inclination 11.388°
40.994°
45.838°
Physical characteristics
Mean diameter
32.90±12.33  km [6]
39.21±0.97 km [7]
39.605±0.198 km [8]
39.88±3.8 km [9]
41.38±11.37 km [10]
45.482±0.215 km [11]
7.955±0.005  h [12]
7.958±0.002 h [13]
7.95880±0.00005 h [14]
7.9597±0.0001 h [15]
7.960±0.001 h [16]
8.8±0.6 h [17]
0.0237±0.0022 [11]
0.027±0.003 [8]
0.03±0.01 [10]
0.0309±0.007 [9]
0.035±0.002 [7]
0.05±0.03 [6]
Tholen = XFC [4] [18]
B–V = 0.688 [4]
U–B = 0.234 [4]
11.23 [6]
11.39 [4] [18] [7] [10] [11]

    Scylla (minor planet designation: 155 Scylla) is a main belt asteroid. It was discovered by Austrian astronomer Johann Palisa at the Austrian Naval Observatory on 8 November 1875, and named after the monster Scylla in Greek mythology. Two weeks after its discovery this asteroid became lost and was not recovered for 95 years. It was finally found by Paul Wild of Berne, Switzerland with the aid of an ephemeris created in 1970 by Conrad M. Bardwell at Cincinnati Observatory. [19]

    Photometric observations of this asteroid during 2008 at the Organ Mesa Observatory in Las Cruces, New Mexico, gave an asymmetrical, bimodal light curve with a period of 7.9597 ± 0.0001 hours and a brightness variation of 0.46 ± 0.03 in magnitude. [15]

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    References

    1. 1 2 "155 Scylla". Minor Planet Center. Retrieved 29 May 2018.
    2. "Scylla" . Oxford English Dictionary (Online ed.). Oxford University Press.(Subscription or participating institution membership required.)
    3. Schmadel, Lutz D. (2007). "(155) Scylla". Dictionary of Minor Planet Names – (155) Scylla. Springer Berlin Heidelberg. p. 29. doi:10.1007/978-3-540-29925-7_156. ISBN   978-3-540-00238-3.
    4. 1 2 3 4 5 6 "JPL Small-Body Database Browser: 155 Scylla" (2018-03-28 last obs.). Jet Propulsion Laboratory . Retrieved 29 May 2018.
    5. "Asteroid 155 Scylla". Small Bodies Data Ferret. Retrieved 29 May 2018.
    6. 1 2 3 Nugent, 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 .
    7. 1 2 3 Usui, 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. 1 2 Masiero, 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. 1 2 Tedesco, 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 . Retrieved 22 October 2019.
    10. 1 2 3 Nugent, 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.
    11. 1 2 3 Mainzer, 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)
    12. Stephens, Robert D. (July 2014). "Asteroids Observed from CS3: 2014 January - March". The Minor Planet Bulletin. 41 (3): 171–175. Bibcode:2014MPBu...41..171S. ISSN   1052-8091.
    13. Addleman, Don; Covele, Brent; Duncan, Allison; Johnson, Jama; Kramb, Steve; Lecrone, Crystal; et al. (December 2005). "Rose-Hulman spring 2005 lightcurve results: 155 Scylla, 590 Tomyris, 1655 Comas Solá, 2058 Roka, 6379 Vrba, and (25934) 2001 DC74". The Minor Planet Bulletin. 32 (4): 76–78. Bibcode:2005MPBu...32...76A. ISSN   1052-8091.
    14. Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network". Astronomy and Astrophysics. 586: 24. arXiv: 1510.07422 . Bibcode:2016A&A...586A.108H. doi:10.1051/0004-6361/201527441. S2CID   119112278.
    15. 1 2 Pilcher, Frederick; Jardine, Don (April 2009). "Period Determinations for 31 Euphrosyne, 35 Leukothea 56 Melete, 137 Meliboea, 155 Scylla, and 264 Libussa". The Minor Planet Bulletin. 36 (2): 52–54. Bibcode:2009MPBu...36...52P. ISSN   1052-8091.
    16. Owings, Larry E. (April 2009). "Lightcurves for 155 Scylla and 2358 Bahner". The Minor Planet Bulletin. 36 (2): 51–52. Bibcode:2009MPBu...36...51O. ISSN   1052-8091.
    17. Behrend, Raoul. "Asteroids and comets rotation curves – (155) Scylla". Geneva Observatory. Retrieved 29 May 2018.
    18. 1 2 "LCDB Data for (155) Scylla". Asteroid Lightcurve Database (LCDB). Retrieved 29 May 2018.
    19. Hodgson, Richard G. (September 1976), "155 Scylla, 279 Thule, 944 Hidalgo, and 1620 Geographos: Four Challenges for Observation", The Minor Planet Bulletin, 4: 7, Bibcode:1976MPBu....4....7H.