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35 Leukothea

From Wikipedia, the free encyclopedia
Main-belt asteroid

35 Leukothea
Three-dimensional model of 35 Leukothea created based on light-curve
Discovery
Discovered byR. Luther
Discovery dateApril 19, 1855
Designations
Designation
(35) Leukothea
Pronunciation/ljˈkɒθiə/[1]
Named after
ΛευκοθέαLeykothea
1948 DC;1950 RS1; 1976 WH
Main belt
AdjectivesLeukothean/ljˈkɒθiən/
Symbol (historical)
Orbital characteristics[2]
Epoch December 31, 2006 (JD 2454100.5)
Aphelion549.374 Gm (3.672AU)
Perihelion345.074 Gm (2.307 AU)
447.224 Gm (2.990 AU)
Eccentricity0.228
1,887.983 d (5.17 a)
17.00 km/s
77.469°
Inclination7.938°
353.817°
213.962°
Physical characteristics
103.05 ± 1.2 km[3]
Mass(1.014 ± 0.491/0.321)×1018 kg[3]
1.769 ± 0.857/0.56 g/cm3[3]
~0.0513 km/s
31.900[4] h
Albedo0.066[5]
Temperature~162K
Spectral type
C
8.5

35 Leukothea is a large, darkasteroid from theasteroid belt. It was discovered by German astronomerKarl Theodor Robert Luther on April 19, 1855,[6] and named afterLeukothea, a sea goddess inGreek mythology. Its historical symbol was apharos (ancient lighthouse); it was encoded inUnicode 17.0 as U+1CED0 𜻐 ().[7][8]

Leukothea is a C-type asteroid in theTholen classification system,[2] suggesting acarbonaceous composition. It is orbiting theSun with a period of 5.17 years and has a cross-sectional size of 103.1 km.

Photometric observations of this asteroid from the Organ Mesa Observatory inLas Cruces, New Mexico during 2010 gave alight curve with a rotation period of31.900±0.001 hours and a brightness variability of0.42±0.04 inmagnitude. This is consistent with previous studies in 1990 and 2008.[4]

The computedLyapunov time for this asteroid is 20,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because ofgravitational perturbations of the planets.[9]

References

[edit]
  1. ^"Leukothea".Dictionary.com Unabridged (Online). n.d.
  2. ^abYeomans, Donald K.,"35 Leukothea",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved7 April 2013.
  3. ^abcFienga, A.; Avdellidou, C.; Hanuš, J. (February 2020)."Asteroid masses obtained with INPOP planetary ephemerides".Monthly Notices of the Royal Astronomical Society.492 (1).doi:10.1093/mnras/stz3407.
  4. ^abPilcher, Frederick (July 2010), "Period Determinations for 11 Parthenope, 35 Leukothea, 38 Leda, 111 Ate, 194 Prokne, 262 Valda, 728 Leonisis, and 747 Winchester",The Minor Planet Bulletin, vol. 37, no. 3, pp. 119–122,Bibcode:2010MPBu...37..119P.
  5. ^Asteroid Data Archive, Planetary Science Institute, archived fromthe original on 23 May 2006, retrieved3 November 2008.
  6. ^"Numbered Minor Planets 1–5000",Discovery Circumstances, IAU Minor Planet center, retrieved7 April 2013.
  7. ^Bala, Gavin Jared; Miller, Kirk (18 September 2023)."Unicode request for historical asteroid symbols"(PDF).unicode.org. Unicode. Retrieved26 September 2023.
  8. ^"Miscellaneous Symbols Supplement"(PDF).unicode.org. The Unicode Consortium. 2025. Retrieved9 September 2025.{{cite web}}: CS1 maint: url-status (link)
  9. ^Šidlichovský, M. (1999), Svoren, J.; Pittich, E. M.; Rickman, H. (eds.), "Resonances and chaos in the asteroid belt",Evolution and source regions of asteroids and comets : proceedings of the 173rd colloquium of the International Astronomical Union, held in Tatranska Lomnica, Slovak Republic, August 24–28, 1998, pp. 297–308,Bibcode:1999esra.conf..297S.

External links

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