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2839 Annette

From Wikipedia, the free encyclopedia
Flora family asteroid

2839 Annette
Shape model ofAnnette from itslightcurve
Discovery[1]
Discovered byC. W. Tombaugh
Discovery siteLowell Obs.
Discovery date5 October 1929
Designations
(2839) Annette
Named after
Annette Tombaugh
(discoverer's daughter)[2]
1929 TP · 1937 AB1
1939 UL · 1962 TE
1970 BB · 1972 XF1
1982 VP
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.67 yr (32,023 days)
Aphelion2.5493AU
Perihelion1.8838 AU
2.2166 AU
Eccentricity0.1501
3.30yr (1,205 days)
200.55°
0° 17m 55.32s / day
Inclination4.8085°
44.569°
6.8264°
Physical characteristics
5.41±0.86 km[4]
7.313±0.150 km[5]
7.562±0.122 km[6]
10.457±0.003 h[7]
10.4595±0.0001 h[8]
0.0563±0.0118[6]
0.060±0.005[5]
0.24(assumed)[3]
0.47±0.22[4]
S[3]
12.9[1] · 12.92[4] · 14.35[3][6][8]

2839 Annette (prov. designation:1929 TP) is a brightFlora asteroid from the inner regions of theasteroid belt. It was discovered on 5 October 1929, by American astronomerClyde Tombaugh atLowell Observatory during his search forPluto.[9] The presumedS-type asteroid has arotation period of 10.5 hours and measures approximately five kilometers (three miles) in diameter. It was named after the discoverer's daughter.[2]

Orbit and classification

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Annette is aS-type asteroid and member of theFlora family, one of the largest families of stony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.9–2.5 AU once every 3 years and 4 months (1,205 days). Its orbit has aneccentricity of 0.15 and aninclination of 5° with respect to theecliptic.[1] Due to aprecovery taken at Lowell Observatory, the body'sobservation arc was extended by 4 days prior to its official discovery observation.[9]

Naming

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Thisminor planet was named after Clyde Tombaugh's daughter, Annette.[2] The approved naming citation was published by theMinor Planet Center on 22 June 1986 (M.P.C. 10845).[10]

Physical characteristics

[edit]

Rotation period

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Lightcurve-based 3D-model ofAnnette

The first rotationallightcurve ofAnnette was obtained by American astronomerBrian Warner at his Palmer Divide Observatory, Colorado, in December 2005. It gave arotation period of 10.457 hours with a brightness variation of 0.92magnitude (U=3-).[7] In November 2006, a second lightcurve by astronomer Robert Buchheim at Altimira Observatory in southern California gave a concurring period of 10.4595 hours and an amplitude of 0.64 magnitude (U=3). He also noted a significantly fainterabsolute magnitude of 14.35 than previously reported.[8]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Annette measures between 5.41 and 7.562 kilometers in diameter and its surface has analbedo between 0.056 and 0.47,[4][5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its family – and calculates a diameter of 3.66 kilometers using Robert Buchheim's fainterabsolute magnitude of 14.35.[3]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2839 Annette (1929 TP)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Retrieved14 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2839) Annette".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 232.doi:10.1007/978-3-540-29925-7_2840.ISBN 978-3540002383.
  3. ^abcde"LCDB Data for (2839) Annette". Asteroid Lightcurve Database (LCDB). Retrieved9 March 2017.
  4. ^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.
  5. ^abcMasiero, 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. Retrieved9 March 2017.
  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.S2CID 35447010.
  7. ^abWarner, Brian D. (September 2006)."Asteroid lightcurve analysis at the Palmer Divide Observatory – late 2005 and early 2006"(PDF).Minor Planet Bulletin.33 (3):58–62.Bibcode:2006MPBu...33...58W.ISSN 1052-8091. Archived fromthe original(PDF) on 19 March 2020. Retrieved18 March 2020.
  8. ^abcBuchheim, Robert K. (September 2007)."Lightcurves of 25 Phocaea, 468 Lina, 482 Petrina 551 Ortrud, 741 Botolphia, 834 Burnhamia, 2839 Annette, and 3411 Debetencourt"(PDF).Minor Planet Bulletin.34 (3):68–71.Bibcode:2007MPBu...34...68B.ISSN 1052-8091. Retrieved18 March 2020.
  9. ^ab"2839 Annette (1929 TP)".Minor Planet Center. Retrieved9 March 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved9 March 2017.

External links

[edit]
Minor planets
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Distant minor planet
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Authority control databasesEdit this at Wikidata
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