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128 Nemesis

From Wikipedia, the free encyclopedia
Main-belt asteroid

128 Nemesis
Discovery[1]
Discovered byJames Craig Watson
Discovery date25 November 1872
Designations
(128) Nemesis
Pronunciation/ˈnɛmɪsɪs/[2]
Named after
Nemesis
A872 WA;1952 HW1
main-belt[1][3] · Nemesis
AdjectivesNemesian/nəˈmʒ(i)ən/[4][5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc144.93yr (52,934 d)
Aphelion3.10 AU (463.69 Gm)
Perihelion2.40 AU (359.00 Gm)
2.75 AU (411.35 Gm)
Eccentricity0.1272
4.56 years (1,665 d)
345.49°
0° 12m 58.32s / day
Inclination6.2453°
76.243°
303.82°
Physical characteristics
163±5 km[6]
162.5±1.3 km[7]
184.2±5.2 km[8]
Flattening0.17[a]
Mass(3.4±1.7)×1018 kg[6]
(6.0±2.6)×1018 kg[8]
1.5±0.8 g/cm3[6]
1.82±0.79 g/cm3[8]
77.81 h (3.242 d)[9]
38.9325 h (1.62219 d)[3]
0.067 (calculated)[6]
0.067±0.005[3]
Tholen =C[3]
SMASS =C[3]
7.70[3]

128 Nemesis is a large 180 kmmain-beltasteroid, ofcarbonaceous composition. It rotates rather slowly, taking about 78 hours to complete one rotation.[3][9] Nemesis is the largest member of the Nemesian asteroid family bearing its name. It was discovered byJ. C. Watson on 25 November 1872,[3] and named afterNemesis, the goddess of retribution inGreek mythology.

Diagram of Nemesis's orbit

This object is orbiting theSun with aperiod of 4.56 years and aneccentricity (ovalness) of 0.13. Theorbital plane isinclined by 6.2° to theplane of the ecliptic. It is categorized as aC-type asteroid,[10] indicating a primitivecarbonaceous composition. Based onIRAS data Nemesis is about 188 km in diameter and is around the 33rd largestmain-belt asteroid,[11] whileWISE measurements yield a size of ~163 km.[7] The 77.81‑hour[12]rotation period is the second longest for an asteroid more than 150 km in diameter.[13]

Between 2005 and 2021, Nemesis has been observed tooccult eight stars.

Notes

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  1. ^Flattening derived from the maximum aspect ratio (c/a):f=1ca{\displaystyle f=1-{\frac {c}{a}}}, where (c/a) =0.83±0.04.[6]

References

[edit]
  1. ^ab"128 Nemesis".Minor Planet Center. Retrieved14 September 2018.
  2. ^"Nemesis".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcdefghi"JPL Small-Body Database Browser: 128 Nemesis" (2017-10-31 last obs.).Jet Propulsion Laboratory. Retrieved14 September 2018.
  4. ^Hornum (1993)Nemesis, the Roman state and the games
  5. ^Peery (1963)Studies in the Renaissance, vol. 10
  6. ^abcdeP. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.Astronomy & Astrophysics 54, A56
  7. ^abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.S2CID 119293330.
  8. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science,73 (1):98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009,S2CID 119226456. See Table 1.
  9. ^abScaltriti, F.; Zappala, V.; Schober, H. J. (January 1979), "The rotations of 128 Nemesis and 393 Lampetia - The longest known periods to date",Icarus,37 (1):133–141,Bibcode:1979Icar...37..133S,doi:10.1016/0019-1035(79)90121-0.
  10. ^DeMeo, Francesca E.; et al. (July 2009),"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.2009.02.005, archived fromthe original(PDF) on 17 March 2014, retrieved8 April 2013. See appendix A.
  11. ^"JPL Small-Body Database Search Engine: asteroids and orbital class (IMB or MBA or OMB) and diameter > 188.1 (km)". JPL's Solar System Dynamics Group. Retrieved17 April 2012.
  12. ^Pilcher, Frederick (July 2015), "New Photometric Observations of 128 Nemisis [sic], 249 Ilse, and 279 Thule",The Minor Planet Bulletin,42 (3): 190−192,Bibcode:2015MPBu...42..190P.
  13. ^"JPL Small-Body Database Search Engine: diameter > 150 (km) and rot_per > 24 (h)".JPL Solar System Dynamics. Retrieved6 June 2015.

External links

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