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2324 Janice

From Wikipedia, the free encyclopedia
Dark background asteroid from the outer regions of the asteroid belt

2324 Janice
Discovery[1]
Discovered byE. F. Helin
S. J. Bus
Discovery sitePalomar Obs.
Discovery date7 November 1978
Designations
(2324) Janice
Named after
Janice Cline [1]
(Supporter atCaltech)
1978 VS4 · 1929 WH
1934 VR · 1949 ME
1961 UP · 1971 OC1
1975 EM2 · 1977 RY4
A911 MC
main-belt[1][2] · (outer)
background[3] · Themis[4][5]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc83.28yr (30,418 d)
Aphelion3.6382AU
Perihelion2.5282 AU
3.0832 AU
Eccentricity0.1800
5.41 yr (1,977 d)
245.72°
0° 10m 55.56s / day
Inclination0.3995°
315.66°
305.63°
Physical characteristics
23.55 km(calculated)[4]
24.33±6.61 km[6]
24.44±1.22 km[7]
25.76±7.43 km[8]
28.463±0.354 km[9]
28.532±0.238 km[10]
28.9±15.91 km[11]
31.19±15.91 km[12]
23.2±0.1 h[11]
0.038±0.004[10]
0.050±0.040[12]
0.06±0.04[6]
0.0601±0.0049[9]
0.07±0.03[8]
0.08(assumed)[4]
0.093±0.010[7]
C(assumed)[4]
11.30[7] · 11.40[8][9][12]
11.46±0.36[13] · 11.5[2][4]
11.68[6]

2324 Janice, provisional designation1978 VS4, is a dark backgroundasteroid from the outer regions of theasteroid belt, approximately 25 kilometers (16 miles) in diameter. It was discovered on 7 November 1978, by American astronomersEleanor Helin andSchelte Bus at thePalomar Observatory in California.[1] The asteroid was named for Janice Cline atCaltech. The presumablyC-type asteroid has arotation period of 23.2 hours.[4]

Orbit and classification

[edit]

Based on osculating Keplerianorbital elements,Janice is located in the region of theThemis family (602), a very largefamily of carbonaceous asteroids, named after24 Themis.[4]

When applying thehierarchical clustering method to itsproper orbital elements, the object is both a non-family asteroid of the main belt'sbackground population (according to Nesvorný),[3] as well as a core member of the Themis family (according to Milani and Knežević).[5]

It orbits the Sun in theouter main-belt at a distance of 2.5–3.6 AU once every 5 years and 5 months (1,977 days;semi-major axis of 3.08 AU). Its orbit has aneccentricity of 0.18 and aninclination of 0° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation asA911 MC atLowell Observatory in June 1911, more than 67 years prior to its official discovery observation at Palomar.[1]

Physical characteristics

[edit]

Janice is a presumed carbonaceousC-type asteroid which is the overallspectral type of members of the Themis family (602).[4]

Rotation period

[edit]

In October 2010, a rotationallightcurve ofJanice was obtained from photometric observations by Gordon Gartrelle at theUniversity of North Dakota Observatory in Grand Forks (730). Lightcurve analysis gave a tentativerotation period of 23.2 hours with a brightness amplitude of 0.19magnitude (U=2-).[11] As of 2018, no secure period has been obtained.[4]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Janice measures between 24.33 and 31.19 kilometers in diameter and its surface has analbedo between 0.038 and 0.093.[6][7][8][9][10][12]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 23.55 kilometers based on anabsolute magnitude of 11.5.[4]

Naming

[edit]

Thisminor planet was named after Janice Cline, who for many years has encouragedastrometric studies of minor planets atCaltech.[1] The official naming citation was published by theMinor Planet Center on 1 March 1981 (M.P.C. 5850).[14]

References

[edit]
  1. ^abcdef"2324 Janice (1978 VS4)".Minor Planet Center. Retrieved26 March 2018.
  2. ^abcd"JPL Small-Body Database Browser: 2324 Janice (1978 VS4)" (2018-02-25 last obs.).Jet Propulsion Laboratory. Retrieved26 March 2018.
  3. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved26 March 2018.
  4. ^abcdefghij"LCDB Data for (2324) Janice". Asteroid Lightcurve Database (LCDB). Retrieved26 March 2018.
  5. ^ab"Asteroid 2324 Janice – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  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. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381.
  9. ^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.S2CID 35447010.
  10. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497.
  11. ^abcGartrelle, Gordon M. (April 2012). "Lightcurve Results for Eleven Asteroids".The Minor Planet Bulletin.39 (2):40–46.Bibcode:2012MPBu...39...40G.ISSN 1052-8091.
  12. ^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.S2CID 46350317.
  13. ^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.S2CID 53493339.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 March 2018.

External links

[edit]
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