Jump to content

86 Semele

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by 2600:6c58:4b7f:ffdf:f9c2:84e1:1304:9702 (talk) at 20:48, 9 April 2020 (Altered pronunciation). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

86 Semele
Discovery
Discovered byFriedrich Tietjen
Discovery dateJanuary 4, 1866
Designations
(86) Semele
Pronunciation/ˈsɛmɪlə/[1]
Named after
Semele
Main belt
AdjectivesSemelean /sɛmɪˈlən/[2]
Orbital characteristics[3]
Epoch December 31, 2006 (JD 2454100.5)
Aphelion562.652 Gm (3.761 AU)
Perihelion369.116 Gm (2.467 AU)
465.884 Gm (3.114 AU)
Eccentricity0.208
2,007.366 d (5.50 a)
16.69 km/s
264.875°
Inclination4.822°
86.452°
307.886°
Physical characteristics
Dimensions120.6 km
Mass1.8×1018 kg
Equatorial surface gravity
0.0337 m/s²
Equatorial escape velocity
0.0638 km/s
0.047 [4]
C
8.54

Semele (minor planet designation: 86 Semele) is a large and very dark main-belt asteroid. It is probably composed of carbonates. Semele was discovered by German astronomer Friedrich Tietjen on January 4, 1866.[5] It was his first and only asteroid discovery. It is named after Semele, the mother of Dionysus in Greek mythology.

The orbit of 86 Semele places it in a 13:6 mean motion resonance with the planet Jupiter. The computed Lyapunov time for this asteroid is only 6,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because of gravitational perturbations of the planets. This Lyapunov time is the second lowest among the first 100 named minor planets.[6]

References

  1. ^ "Semele". Lexico UK English Dictionary. Oxford University Press. n.d.
  2. ^ Robert Calverley Trevelyan (1898) Mallow and Asphadel, p. 4.
  3. ^ Yeomans, Donald K., "86 Semele", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 7 April 2013.
  4. ^ Asteroid Data Sets Archived 2009-12-17 at the Wayback Machine
  5. ^ "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
  6. ^ 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.