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100 Hekate

From Wikipedia, the free encyclopedia

100 Hekate
3D convex shape model of Hekate
Discovery[1]
Discovered byJ. C. Watson
Discovery date11 July 1868
Designations
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
5.433 yr (1984.4 d)
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
Mean density
~2.7 g/cm3 (estimate)[5]
Equatorial surface gravity
~0.033 m/s2
Equatorial escape 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~154 K
max: 238K (−35 °C)
S-type asteroid
7.67

100 Hekate is a large main-belt asteroid.

About

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Orbit of Hekate

Hekate is a stony S-type asteroid with a diameter of 87+5
−4
 km
and a sidereal rotation period of 27.07 h.[7] It orbits in the same region of space as the Hygiea asteroid family, though it is actually an unrelated interloper. Its geometric albedo of 0.22±0.03[7] is too high, and it is of the wrong spectral class to be part of the dark carbonaceous Hygiea family. It is listed as a member of the Hecuba group of asteroids that orbit near the 2:1 mean-motion resonance with Jupiter.[8]

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

An occultation of a star by Hekate was observed on July 14, 2003, from New Zealand.

See also

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References

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  1. "100 Hekate". Minor Planet Center. Retrieved 23 October 2025.
  2. 1 2 "Hecate". Oxford English Dictionary (online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  3. 1 2 3 4 "100 Hekate". JPL Small-Body Database. Jet Propulsion Laboratory. SPK-ID: 2000100. Retrieved 23 October 2025.
  4. 1 2 "IRAS Minor Planet Survey".{{cite web}}: CS1 maint: deprecated archival service (link)
  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. 1 2 Marciniak, 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. Retrieved 7 April 2013.
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