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100 Hekate

From Wikipedia, the free encyclopedia
Main-belt asteroid

100 Hekate
3D convex shape model of Hekate
Discovery[1]
Discovered byJ. C. Watson
Discovery date11 July 1868
Designations
(100) Hekate
Pronunciation/ˈhɛkət/[2]
Named after
Hecate
1955 QA
Main belt
AdjectivesHekatean (Hecatæan)/hɛkəˈtən/[2]
Orbital characteristics[3]
Epoch 2025 Nov 21 (JD 2461000.5)
Uncertainty parameter 0
Observation arc154.56 yr (56452 d)
Aphelion3.60957 AU (539.984 Gm)
Perihelion2.57132 AU (384.664 Gm)
3.09045 AU (462.325 Gm)
Eccentricity0.16798
5.433yr (1984.4d)
323.244°
0° 10m 53.093s / day
Inclination6.43092°
127.156°
183.552°
Earth MOID1.55453 AU (232.554 Gm)
Jupiter MOID1.66378 AU (248.898 Gm)
TJupiter3.194
Physical characteristics
Dimensions88.734±1.961 km[3]
89 km[4]
Mass~1.0×1018 kg
~2.7 g/cm3(estimate)[5]
~0.033 m/s2
Equatorialescape velocity
~0.054 km/s
27.066 h (1.1278 d)[3]
0.5555 d[6]
0.205±0.01[3]
0.192[4]
Temperature~154K
max: 238K (−35 °C)
S-type asteroid
7.67

100 Hekate is a largemain-beltasteroid.

About

[edit]
Orbit of Hekate

Hekate is a stonyS-type asteroid with a diameter of87+5
−4
 km
and a siderealrotation period of27.07 h.[7] It orbits in the same region of space as theHygiea asteroid family, though it is actually an unrelated interloper. However, its geometricalbedo of0.22±0.03[7] is too high, and it is of the wrong spectral class to be part of the darkcarbonaceous Hygiea family. It is listed as a member of theHecuba group of asteroids that orbit near the 2:1mean-motion resonance withJupiter.[8]

Hekate was the 100th asteroid to be discovered, by Canadian-American astronomerJ. C. Watson (his fourth discovery) on July 11, 1868.[9] It is named afterHecate, the goddess ofwitchcraft inGreek mythology, but its name also commemorates it as the hundredth asteroid, as ἑκατόν (hekaton) is Greek for 'hundred'.

Anoccultation of a star by Hekate was observed on July 14, 2003, fromNew Zealand.

See also

[edit]

References

[edit]
  1. ^"100 Hekate".Minor Planet Center. Retrieved23 October 2025.
  2. ^ab"Hecate".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcd"100 Hekate".JPL Small-Body Database.Jet Propulsion Laboratory. SPK-ID: 2000100. Retrieved23 October 2025.
  4. ^ab"IRAS Minor Planet Survey". Archived fromthe original on 11 December 2005.
  5. ^Krasinsky, G. A. (2002). "Hidden Mass in the Asteroid Belt".Icarus.158 (1): 98.Bibcode:2002Icar..158...98K.doi:10.1006/icar.2002.6837.
  6. ^"Asteroid Lightcurve Parameters".
  7. ^abMarciniak, A.; et al. (May 2019). "Thermal properties of slowly rotating asteroids: results from a targeted survey".Astronomy & Astrophysics.625: 40.arXiv:1905.06056.Bibcode:2019A&A...625A.139M.doi:10.1051/0004-6361/201935129.S2CID 146059739. A139.
  8. ^McDonald, S. L. (1948)."General perturbations and mean elements, with representations of 35 minor planets of the Hecuba group".The Astronomical Journal.53: 199.Bibcode:1948AJ.....53..199M.doi:10.1086/106097.
  9. ^"Discovery Circumstances: Numbered Minor Planets 1–5000".IAU Minor Planet Center. Retrieved7 April 2013.

External links

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