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88 Thisbe

From Wikipedia, the free encyclopedia
Main-belt asteroid

88 Thisbe
Discovery
Discovered byChristian Heinrich Friedrich Peters
Discovery date15 June 1866
Designations
(88) Thisbe
Pronunciation/ˈθɪzb/[1]
Named after
Thisbē
Main belt
AdjectivesThisbean/θɪzˈbən/,/ˈθɪzbiən/
Orbital characteristics[2]
Epoch 31 December 2006 (JD 2454100.5)
Aphelion482.242 Gm (3.224 AU)
Perihelion345.809 Gm (2.312 AU)
414.025 Gm (2.768 AU)
Eccentricity0.165
1,681.709 d (4.60 yr)
165.454°
Inclination5.219°
276.765°
36.591°
Physical characteristics
Dimensions(255×232×193)±12 km[3]
218±3 km[4]
225 km[3]
232 km (Dunham)[2]
Flattening0.19[a]
Mass(11.6±2.2)×1018 kg[4]
18.3×1018 kg[3]
1.5×1019 kg[5][b]
2.14±0.42 g/cm3[4]
3.06±0.52 g/cm3[3]
6.04[6] h
0.057[4]
0.067[7]
B[2]
7.04[2]

88 Thisbe is the13th largestmain-beltasteroid.C. H. F. Peters discovered it on 15 June 1866, named afterThisbe, heroine of aRomanfable. This asteroid orbits the Sun at a distance of 2.768 AU over aperiod of 4.60 years and anorbital eccentricity (ovalness) of 0.165. Theorbital plane is inclined at an angle of 5.219° to theecliptic.

On 7 October 1981, asteroid 88 Thisbe was observed tooccult the 9th-magnitude star SAO 187124 from 12 sites. The timing of the different chords across the asteroid provided a diameter estimate of232±12 km. This is 10% larger than the diameter estimate based on radiometric techniques.[8][9][10] During 2000, 88 Thisbe was observed by radar from theArecibo Observatory. The return signal matched an effective diameter of 207 ± 22 km. This is consistent with the asteroid dimensions computed through other means.[11]

Photometric observations of this asteroid during 1977 gave alight curve with a period of 6.0422 ± 0.006 hours and a brightness variation of 0.19 inmagnitude.[6]

Perturbation

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Asteroid7 Iris hasperturbed Thisbe; in 2001, Michalak estimated it to have a mass of 15×1018 kg.[5][b] But Iris is strongly perturbed by many minor planets such as10 Hygiea and15 Eunomia.[5]

In 2008, Baer estimated Thisbe to have a mass of 10.5×1018 kg.[3] In 2011, Baer revised this to 18.3×1018 kg with an uncertainty of 1.1×1018 kg.[3]

Notes

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  1. ^Flattening derived from the maximum aspect ratio (c/a):f=1ca{\displaystyle f=1-{\frac {c}{a}}}, where (c/a) =0.81±0.07.[4]
  2. ^ab(7.4 ± 1.3)×10−12M = 1.47×1019 kg

References

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  1. ^Noah Webster (1884).A Practical Dictionary of the English Language.
  2. ^abcdYeomans, Donald K.,"88 Thisbe",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved25 March 2013.
  3. ^abcdefJim Baer (2011)."Recent Asteroid Mass Determinations". Personal Website. Archived fromthe original on 2 July 2013. Retrieved12 April 2012.
  4. ^abcdeP. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.Astronomy & Astrophysics 54, A56
  5. ^abcMichalak, G. (2001)."Determination of asteroid masses".Astronomy & Astrophysics.374 (2):703–711.Bibcode:2001A&A...374..703M.doi:10.1051/0004-6361:20010731. Retrieved6 November 2008.
  6. ^abSchober, H. J.; et al. (April 1979), "Photoelectric photometry and rotation periods of three large and dark asteroids - 49 Pales, 88 Thisbe and 92 Undina",Astronomy and Astrophysics Supplement Series, vol. 36, pp. 1–8,Bibcode:1979A&AS...36....1S.
  7. ^Asteroid Data SetsArchived 2009-12-17 at theWayback Machine
  8. ^Millis, R. L.; et al. (February 1983), "The diameter of 88 THISBE from its occultation of SAO 187124",Astronomical Journal,88:229–235,Bibcode:1983AJ.....88..229M,doi:10.1086/113310,hdl:2060/19820025413.
  9. ^Taylor, G. E., "Progress in accurate determinations of diameters of minor planets",Asteroids, comets, meteors; Proceedings of the Meeting, Uppsala, Sweden, 20-22 June 1983, pp. 107–109,Bibcode:1983acm..proc..107T.
  10. ^Observed minor planet occultation events, version of 2005 July 26
  11. ^Magri, Christopher; et al. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999–2003",Icarus,186 (1):126–151,Bibcode:2007Icar..186..126M,doi:10.1016/j.icarus.2006.08.018

External links

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Large asteroids (mean diameter greater than 200 km)
Mean diameter 900–1000 km
Mean diameter 500–600 km
Mean diameter 300–500 km
Mean diameter 200–300 km
Minor planets
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