1329 Eliane

1329 Eliane
Discovery [1]
Discovered by E. Delporte
Discovery site Uccle – Belgium
Discovery date 23 March 1933
Designations
MPC designation 1329 Eliane
Named after
 Éliane Bourgeois[2]
(Paul Bourgeois' daughter)
1933 FL · 1955 MP
1975 FT
main-belt · (middle) [3]
Orbital characteristics [1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 82.94 yr (30,293 days)  
Aphelion 3.0702 AU
Perihelion 2.1622 AU
2.6162 AU
Eccentricity 0.1735
4.23 yr (1,546 days)
144.7754°
0° 13m 58.44s / day
Inclination 14.4704°
132.0675°
164.9994°
Physical characteristics
Dimensions 20.94±0.25 km[4]
19.467±0.270 km[5]
22.64±0.47 km[6]
19.63 km (calculated)[3]
106±25 h[7]
72±2 h[8]
8.0±0.1 h (wrong)[9]
0.180±0.005[4]
0.1486±0.0119[5]
0.150±0.019[6]
0.20 (assumed)[3]
B–V = 0.873[1]
U–B = 0.443[1]
S (Tholen)[1]
S (SMASS)[1]
S [3][10]
10.90[1][3][4][5][6]
10.71±0.80[10]

    1329 Eliane, provisional designation 1933 FL, is a stony asteroid and slow rotator from the middle region of the asteroid belt, approximately 20 kilometers in diameter. It was discovered by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle, on 23 March 1933.[11]

    The S-type asteroid orbits the Sun at a distance of 2.2–3.1 AU once every 4 years and 3 months (1,546 days). Its orbit has an eccentricity of 0.17 and an inclination of 14° with respect to the ecliptic.[1]

    A rotational light-curve was reevaluated by American astronomer Brian Warner at the U.S. Palmer Divide Observatory, Colorado, in 2010. The photometric observations originally taken in April 2001, revealed a very long rotation period of 106±25 hours with a brightness amplitude of 0.30 in magnitude (U=2-).[7][lower-alpha 1] According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 19.5 and 22.6 kilometers in diameter and its surface has an albedo in the range of 0.15 to 0.18.[4][5][6] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20, and calculates a diameter of 19.6 kilometers.[3]

    The minor planet was named after Éliane Bourgeois, daughter of astronomer Paul Bourgeois, professor at the discovering Royal Observatory in Uccle, Belgium, and after whom the minor planet 1543 Bourgeois is named.[2] Naming citation was published before 1977 (H 121, no M.P.C. available).[12]

    References

    1. ↑ Note to Warner's Revised rotation period: "Updated results are given for six asteroids previously reported from the Palmer Divide Observatory. The original images were remeasured to obtain new data sets using the latest version of MPO Canopus photometry software, analysis tools, and revised techniques for linking multiple observing runs covering several days to several weeks. Results that were previously not reported or had significantly different periods and/or amplitudes were found for 1329 Eliane, 1582 Martir, 2023 Asaph, 8041 Masumoto, (26853) 1992 UQ2, and (52387) 1993 OM7. This is the second in a series of papers that examines results obtained during the initial years of the asteroid lightcurve program at PDO." Upon Further Review: II. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory
    1. 1 2 3 4 5 6 7 8 "JPL Small-Body Database Browser: 1329 Eliane (1933 FL)" (2016-02-29 last obs.). Jet Propulsion Laboratory. Retrieved May 2016.
    2. 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (1329) Eliane. Springer Berlin Heidelberg. p. 108. ISBN 978-3-540-00238-3. Retrieved May 2016.
    3. 1 2 3 4 5 6 "LCDB Data for (1329) Eliane". Asteroid Lightcurve Database (LCDB). Retrieved May 2016.
    4. 1 2 3 4 Usui, 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. Retrieved May 2016.
    5. 1 2 3 4 Mainzer, 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. Retrieved May 2016.
    6. 1 2 3 4 Masiero, 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. Retrieved May 2016.
    7. 1 2 Warner, Brian D. (October 2010). "Upon Further Review: II. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory". The Minor Planet Bulletin 37 (4): 150–151. Bibcode:2010MPBu...37..150W. ISSN 1052-8091. Retrieved May 2016.
    8. ↑ Behrend, Raoul. "Asteroids and comets rotation curves – (1329) Eliane". Geneva Observatory. Retrieved May 2016.
    9. ↑ Warner, B. D. (March 2002). "Asteroid Photometry at the Palmer Divide Observatory: Results for 573 Recha, 1329 Eliane, and 8041 Masumoto". The Minor Planet Bulletin 29: 14–15. Bibcode:2002MPBu...29...14W. Retrieved May 2016.
    10. 1 2 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. Retrieved May 2016.
    11. ↑ "1329 Eliane (1933 FL)". Minor Planet Center. Retrieved May 2016.
    12. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved May 2016.

    External links


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