194 Prokne

Main-belt asteroid From Wikipedia, the free encyclopedia

194 Prokne

194 Prokne is a main-belt asteroid that was discovered by German-American astronomer C. H. F. Peters on March 21, 1879, in Clinton, New York, and named after Procne, the sister of Philomela in Greek mythology. Stellar occultations by Prokne have been observed twice, in 1984 from Italy and again in 1999 from Iowa (United States).

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194 Prokne
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Orbital diagram
Discovery
Discovered byC. H. F. Peters, 1879
Discovery date21 March 1879
Designations
(194) Prokne
Pronunciation/ˈprɒkn/[1]
Named after
Procne
A879 FA
Main belt
AdjectivesProknean /prɒkˈnən/[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc136.76 yr (49950 d)
Aphelion3.2386 AU (484.49 Gm)
Perihelion1.9930 AU (298.15 Gm)
2.6158 AU (391.32 Gm)
Eccentricity0.23810
4.23 yr (1545.3 d)
42.282°
0° 13m 58.692s / day
Inclination18.509°
159.32°
163.24°
Earth MOID0.986917 AU (147.6407 Gm)
Jupiter MOID2.15988 AU (323.113 Gm)
TJupiter3.295
Physical characteristics
Dimensions168.42±4.1 km[3]
170.33±6.92 km[4]
Mass(2.68±0.29)×1018 kg[4]
Mean density
1.03±0.16 g/cm3[4]
15.679 h (0.6533 d)[3][5]
0.0528±0.003
C
7.68
    Close

    Observations from the W. M. Keck Observatory show the asteroid to be around 151 km across, with a size ratio of 1.13±0.06 between the major and minor axes. For comparison, observations by the IRAS observatory gave a diameter of 164 km.[6] The spectrum matches a classification of a C-type asteroid, indicating it has a primitive carbonaceous composition. Judging from radar data, the near surface solid density of the asteroid is 3.6+1.1
    0.9
    g cm−3.[7]

    Based upon a light curve that was generated from photometric observations of this asteroid at Pulkovo Observatory, it has a rotation period of 15.679±0.001 hours and varies in brightness by 0.16±0.02 in magnitude.[5]

    References

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