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756 Lilliana

From Wikipedia, the free encyclopedia
Main-belt asteroid

756 Lilliana
Discovery[1]
Discovered byJoel Hastings Metcalf
Discovery siteTaunton, Massachusetts
Discovery date26 April 1908
Designations
(756) Lilliana
1908 DC[2]
main belt
Orbital characteristics[2][3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc101.86 yr (37203 d)
Aphelion3.66990 AU (549.009 Gm)
Perihelion2.71910 AU (406.772 Gm)
3.19450 AU (477.890 Gm)
Eccentricity0.148819
5.71 yr (2085.5 d)
281.138°
0° 10m 21.446s / day
Inclination20.3578°
208.088°
5.26073°
Physical characteristics
  • 35.75±0.7km[2]
  • 35.75 ± 0.7 km (22.21 ± 0.43 mi)[4]
  • 9.361±0.002 h[5]
  • 7.834 h (0.3264 d)[2]
0.0500±0.002[4]

756 Lilliana is aminor planet orbiting theSun that was discovered by American astronomerJoel Hastings Metcalf on 26 April 1908 fromTaunton, Massachusetts. It rotates around itsaxis of rotation every 9.36 hours.[5][clarification needed]

Photometric observations of this asteroid atPalmer Divide Observatory inColorado Springs, Colorado, during 2007 gave alight curve with a period of9.262±0.001 hours and a brightness variation of0.83±0.03 inmagnitude.[7] A 2012 study based upon observations at the Organ Mesa Observatory inLas Cruces, New Mexico, during 2012 produced a conflicting period of7.834±0.001 hours and a brightness variation of0.17±0.02 inmagnitude. Further study will be needed to resolve the discrepancies in period and amplitude.[8]

References

[edit]
  1. ^"Numbered Minor Planets 1–5000",Discovery Circumstances, IAU Minor Planet center, retrieved7 April 2013.
  2. ^abcdeYeomans, Donald K.,"756 Lilliana",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved5 May 2016.
  3. ^"(756) Lilliana".AstDyS. Italy:University of Pisa. Archived fromthe original on 26 May 2011. Retrieved12 December 2008.
  4. ^abTedesco; et al. (2004)."Supplemental IRAS Minor Planet Survey (SIMPS)".IRAS-A-FPA-3-RDR-IMPS-V6.0.Planetary Data System. Retrieved7 January 2009.{{cite web}}:|archive-url= is malformed: timestamp (help)CS1 maint: url-status (link)
  5. ^abSzékely; Kiss, L; Szabo, G; Sarneczky, K; Csak, B; Varadi, M; Meszaros, S; et al. (2005). "CCD photometry of 23 minor planets".Planetary and Space Science.53 (9):925–936.arXiv:astro-ph/0504462.Bibcode:2005P&SS...53..925S.doi:10.1016/j.pss.2005.04.006.S2CID 119361591.web preprint
  6. ^Tholen (2007)."Asteroid Absolute Magnitudes".EAR-A-5-DDR-ASTERMAG-V11.0.Planetary Data System. Retrieved7 January 2009.{{cite web}}:|archive-url= is malformed: timestamp (help)CS1 maint: url-status (link)
  7. ^Warner, Brian D. (June 2008), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory – June–October 2007",The Minor Planet Bulletin,35 (2):56–60,Bibcode:2008MPBu...35...56W.
  8. ^Pilcher, Frederick (October 2012), "Rotation Period Determinations for 47 Aglaja, 252 Clementina, 611 Valeria, 627 Charis, and 756 Lilliana",Minor Planet Bulletin,39 (4):220–222,Bibcode:2012MPBu...39..220P.

External links

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