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1068 Nofretete

From Wikipedia, the free encyclopedia
Main-belt asteroid
Not to be confused with3199 Nefertiti.

1068 Nofretete
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date13 September 1926
Designations
(1068) Nofretete
Pronunciation/nɒfrəˈttə/[a]
Named after
Nefertiti[2]
(Ancient Egyptian Queen)
1926 RK · 1929 CV
main-belt · (outer)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.73 yr (32,409 days)
Aphelion3.1868AU
Perihelion2.6274 AU
2.9071 AU
Eccentricity0.0962
4.96yr (1,810 days)
250.26°
0° 11m 55.68s / day
Inclination5.4840°
318.69°
267.47°
Physical characteristics
Dimensions21.346±0.106 km[5]
22.03 km(derived)[3]
23.186±0.116 km[6]
23.92±0.74 km[7]
26.73±0.45 km[8]
6.15h[9]
0.104±0.007[7]
0.142±0.025[8]
0.1832±0.0400[6]
0.20(assumed)[3]
S[3][9]
B–V = 0.850[1]
U–B = 0.420[1]
10.60[8] · 10.65[3][6][9] · 10.7[1] · 10.84±0.47[10] · 11.20[7]

1068 Nofretete (/nɒfrəˈttə/[a]), provisional designation1926 RK, is a stonyasteroid from thebackground population in the outerasteroid belt, approximately 23 kilometers in diameter. It was discovered on 13 September 1926, by Belgian astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle.[11] The asteroid was named after the Ancient Egyptian QueenNefertiti by its German name "Nofretete".[2] The near-Earth asteroid3199 Nefertiti is also named after her.

Orbit and classification

[edit]

Nofretete is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in theouter asteroid belt at a distance of 2.6–3.2 AU once every 4 years and 12 months (1,810 days;semi-major axis of 2.91 AU). Its orbit has aneccentricity of 0.10 and aninclination of 5° with respect to theecliptic.[1] The body'sobservation arc begins at Uccle in September 1926, three nights after its official discovery observation.[11]

Physical characteristics

[edit]

Nofretete has been characterized as a stonyS-type asteroid by American astronomerRichard Binzel.[9]

Rotation period

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In May 1984, a rotationallightcurve ofNofretete was obtained from photometric observations by Richard Binzel which gave arotation period of 6.15 hours with a low brightness amplitude of 0.04magnitude, indicative for a nearly spheroidal shape (U=2).[9]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Nofretete measures between 21.346 and 26.73 kilometers in diameter and its surface has analbedo between 0.104 and 0.1832.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 22.03 kilometers based on anabsolute magnitude of 10.65.[3]

Naming

[edit]

Thisminor planet was named by German astronomerGustav Stracke after the Ancient Egyptian QueenNefertiti (c.1370 – c.1330 BC) by its common German name "Nofretete".[a] She was the wife of pharaohAkhenaten (a.k.a. Echnaton or Amenhotep IV), after whom the asteroid4847 Amenhotep is named. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 101). The near-Earth asteroid3199 Nefertiti, discovered by American astronomersCarolyn andEugene Shoemaker at Palomar, was also named after her.[2]

Notes

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  1. ^abcPronunciation of "Nofretete" fromCollins English Dictionary. The original naming in German is pronounced asnɔfʁəˈteːtə.

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1068 Nofretete (1926 RK)" (2017-10-30 last obs.).Jet Propulsion Laboratory. Retrieved7 December 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1068) Nofretete".Dictionary of Minor Planet Names – (1068) Nofretete.Springer Berlin Heidelberg. p. 91.doi:10.1007/978-3-540-29925-7_1069.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1068) Nofretete". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2017.
  4. ^ab"Asteroid 1068 Nofretete – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  5. ^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.
  6. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  7. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  8. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved7 December 2017.
  9. ^abcdeBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved7 December 2017.
  10. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved7 December 2017.
  11. ^ab"1068 Nofretete (1926 RK)".Minor Planet Center. Retrieved7 December 2017.

External links

[edit]
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