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101 Helena

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Main-belt asteroid
Not to be confused with Helene (moon).

101 Helena
Orbital diagram
Discovery
Discoveredby James Craig Watson
Discoverydate15 August 1868
Designations
Pronunciation/ˈhɛlənə/ [1]
Named after
Helen of Troy
A868 PA
Main belt
Orbital characteristics [2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 145.07 yr (52986 d)
Aphelion 2.94606AU (440.724Gm)
Perihelion 2.22353AU (332.635Gm)
2.58480AU (386.681Gm)
Eccentricity 0.13977
4.16 yr (1517.9 d)
Average orbital speed
18.44 km/s
236.265°
0° 14m 13.823s / day
Inclination 10.1976°
343.419°
348.030°
EarthMOID 1.21369AU (181.565Gm)
JupiterMOID 2.4117AU (360.79Gm)
TJupiter 3.387
Physical characteristics
Dimensions 65.84±1.3km [2]
Mass 3.0×ばつ1017 kg
Mean density
2.0 g/cm3
Equatorial surfacegravity
0.0184 m/s2
Equatorial escape velocity
0.0348 km/s
23.080h (0.9617d)[2]
0.1898±0.008[2]
Temperature ~173 K
S [3]
8.33

101 Helena is a large, rocky main-belt asteroid. It was discovered by Canadian-American astronomer J. C. Watson on August 15, 1868,[4] and was named after Helen of Troy in Greek mythology.

This object is orbiting the Sun with a period of 4.16 years and an eccentricity of 0.14. Its orbital plane is inclined by 10.2° to the plane of the ecliptic. Radar observations were made of this object on Oct 7 and 19, 2001 from the Arecibo Observatory. Analysis of the data gave an estimated ellipsoidal diameter of ×ばつ63 ± 16% km. The mean diameter estimated from IRAS infrared measurements is 66 km, in agreement with the radar findings. It is classified as an S-type asteroid in the Tholen system,[3] [5] suggesting a predominantly silicate composition. 101 Helena is spinning on its axis with a period of 23 hours.[2]

References

[edit ]
  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. 1 2 3 4 5 Yeomans, Donald K., "101 Helena", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, archived from the original on 24 September 2014, retrieved 12 May 2016.
  3. 1 2 DeMeo, Francesca E.; et al. (2011), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus, 202 (1): 160–180, Bibcode:2009Icar..202..160D, doi:10.1016/j.icarus.200902005, archived from the original (PDF) on 17 March 2014, retrieved 22 March 2013. See appendix A.
  4. "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
  5. Magri, Christopher; Nolan, Michael C.; Ostro, Steven J.; Giorgini, Jon D. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999 2003", Icarus, 186 (1): 126–151, Bibcode:2007Icar..186..126M, doi:10.1016/j.icarus.2006年08月01日8.
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