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201 Penelope

From Wikipedia, the free encyclopedia
Main-belt asteroid

201 Penelope
A three-dimensional model of 201 Penelope based on its light curve.
Discovery
Discovered byJohann Palisa
Discovery date7 August 1879
Designations
(201) Penelope
Pronunciation/pɪˈnɛləp/[1]
Named after
Penelópē
A879 PA; 1869 GA
Main belt
AdjectivesPenelopean/pɪˈnɛlˈpən/[1]
Orbital characteristics[2]
Epoch 21 January 2022 (JD 2457600.5)
Uncertainty parameter 0
Observation arc142.58 yr (52,077 d)[3]
Aphelion3.160 AU (472.710 Gm)[3]
Perihelion2.199 AU (329.009 Gm)[4][3]
2.680 AU (400.859 Gm)[4][3]
Eccentricity0.17924[4][3]
4.39 yr (1,602.14 d)[3]
18.19 km/s
169.01173°[4]
0° 13m 28.917s / day[4]
Inclination5.75625°[4][3]
156.91554°[4]
180.90559°[4]
Jupiter MOID2.23013 AU (333.623 Gm)[3]
TJupiter3.347[3]
Physical characteristics
Dimensions68.39±3.5 km[2]
87.72 km[5]
3.7474 h (0.15614 d)[3]
0.1604±0.018[2]
0.0881±0.0187[5]

201 Penelope is a largemain beltasteroid that was discovered by Austrian astronomerJohann Palisa on August 7, 1879, inPola. The asteroid is named afterPenelope, the wife ofOdysseus inHomer'sThe Odyssey. It is orbiting theSun at a distance of2.68 AU with aneccentricity (ovalness) of 0.18 and aperiod of 4.381 years. Theorbital plane is tilted at an angle of 5.8° to theplane of the ecliptic.[2]

Based upon the spectra of this object, it is classified as aM-type asteroid, indicating it may be metallic in composition.[5] It may be the remnant of the core of a larger, differentiated asteroid. Near infrared absorption features indicate the presence of variable amounts of low-iron, low-calciumorthopyroxenes on the surface. Trace amounts of water is detected with amass fraction of about 0.13–0.15 wt%.[6] It has an estimated size of around 88 km.[5] With a rotation period of 3.74 hours, it is the fastest rotating asteroid larger than 50 km in diameter.[2]

References

[edit]
  1. ^ab"Penelope".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  2. ^abcdef"JPL Small-Body Database Search Engine: diameter > 50 (km) and rot_per > 0 (h)".JPL Solar System Dynamics. Retrieved12 May 2016.
  3. ^abcdefghijklmn"Small-Body Database Lookup".ssd.jpl.nasa.gov. Retrieved12 April 2022.
  4. ^abcdefghi"IAU Minor Planet Center".minorplanetcenter.net. Retrieved12 April 2022.
  5. ^abcdefPravec, P.; et al. (May 2012), "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations",Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16–20, 2012 in Niigata, Japan, no. 1667,Bibcode:2012LPICo1667.6089P. See Table 4.
  6. ^Hardersen, Paul S.; Gaffey, Michael J.; Abell, Paul A. (January 1983), "Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids",Icarus, vol. 175, no. 1, pp. 141–158,Bibcode:2005Icar..175..141H,doi:10.1016/j.icarus.2004.10.017.

External links

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