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258 Tyche

Main belt asteroid


Main belt asteroid

FieldValue
minorplanetyes
name258 Tyche
background#D6D6D6
image258Tyche (Lightcurve Inversion).png
caption
discovery_ref
discovered4 May 1886
discovererR. Luther
discovery_siteDüsseldorf-Bilk Obs.
mpc_name(258) Tyche
pronounced
alt_namesA886 JA
named_afterTyche
mp_categoryEunomiamain-belt
orbit_ref
epoch31 July 2016 (JD 2457600.5)
uncertainty0
observation_arc129.95 yr (47465 d)
aphelion3.1512 AU
perihelion2.0838 AU
semimajor2.6175 AU
eccentricity0.20390
period4.23 yr (1546.8 d)
mean_anomaly157.95°
inclination14.305°
asc_node207.59°
arg_peri155.01°
moid1.09016 AU
avg_speed18.42 km/s
mass~ 4×1017 kg *(estimate)*
dimensions
65 km
density~ 2.7 g/cm3
rotation10.041 h
albedo
0.168
spectral_typeB–V = 0.876
U–B = 0.459
S (Tholen), S (SMASS)
abs_magnitude8.50
single_temperature~ 169 K
*max:* 268 K
mean_motion/ day
jupiter_moid2.34517 AU
tisserand3.334
Note

the asteroid

65 km 0.168 U–B = 0.459 S (Tholen), S (SMASS) max: 268 K

258 Tyche is a relatively large main belt asteroid discovered by Robert Luther at Düsseldorf-Bilk Observatory on 4 May 1886. The stony S-type asteroid measures about 65 kilometers in diameter and has a perihelion of 2.1 AU.

Tyche orbits very close to the Eunomia family of asteroids, and could be a member based on composition. However, it is larger than all family members apart from 15 Eunomia while lying at the very edge of the family group. Hence, there is a good chance that it is an unrelated interloper.

There is some uncertainty regarding Tyche's rotation period. Various authors give values from 9.983 to 10.041 hours.

It was named after the Greek goddess of fortune, Tyche, which is also the name of one of the Oceanids. Tyche's Roman equivalent is Fortuna, after which the asteroid 19 Fortuna is named.

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. [http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab Supplemental IRAS Minor Planet Survey] {{webarchive. link. (June 23, 2006)
  3. [http://www.psi.edu/pds/archive/lc.html PDS lightcurve data] {{webarchive. link. (June 14, 2006)
  4. (2001). "Rotational periods of asteroids II". Planetary and Space Science.
  5. (2002). "Hidden Mass in the Asteroid Belt". Icarus.
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