Astronomy:1017 Jacqueline

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1017 Jacqueline
001017-asteroid shape model (1017) Jacqueline.png
Shape model of Jacqueline from its lightcurve
Discovery[1]
Discovered byB. Jekhovsky
Discovery siteAlgiers Obs.
Discovery date4 February 1924
Designations
(1017) Jacqueline
Named afterJacqueline Zadoc-Kahn Eisenmann[2]
(discoverer's pupil)
1924 QL · 1929 LG
1953 AC · A924 ED
A924 CH
Minor planet category
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc92.01 yr (33,607 d)
|{{{apsis}}}|helion}}2.8098 AU
|{{{apsis}}}|helion}}2.4017 AU
2.6058 AU
Eccentricity0.0783
Orbital period4.21 yr (1,536 d)
Mean anomaly292.84°
Mean motion0° 14m 3.48s / day
Inclination7.9280°
Longitude of ascending node118.94°
68.145°
Physical characteristics
Mean diameter
  • 37.65±3.4 km[6]
  • 38.87±0.51 km[7]
  • 40.152±0.199 km[8]
Rotation period7.87±0.01 h[9]
Pole ecliptic latitude
  • (7.0°, 55.0°) (λ1/β1)[5]
  • (170.0°, 65.0°) (λ2/β2)[5]
Geometric albedo
  • 0.051±0.002[7]
  • 0.052±0.005[8]
  • 0.0544±0.011[6]
SMASS = C[3]
Absolute magnitude (H)11.1[1][3]


1017 Jacqueline (prov. designation: A924 CH or 1924 QL) is a dark background asteroid from the central regions of the asteroid belt. It was discovered on 4 February 1924, by Russian-French astronomer Benjamin Jekhowsky at the Algiers Observatory, Algeria, in North Africa.[1] The carbonaceous C-type asteroid has a rotation period of 7.87 hours with a high brightness amplitude of 0.6 magnitude and measures approximately 39 kilometers (24 miles) in diameter.[10] It was named after the French physicist and long-time pupil of the discoverer, Jacqueline Zadoc-Kahn Eisenmann (1904–1998).[2]

Orbit and classification

Jacqueline is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the intermediate asteroid belt at a distance of 2.4–2.8 AU once every 4 years and 3 months (1,536 days; semi-major axis of 2.61 AU). Its orbit has an eccentricity of 0.08 and an inclination of 8° with respect to the ecliptic.[3] The asteroid's earliest preserved observation dates back to 7 March 1924 at Heidelberg Observatory, where the body's observation arc begins in February 1928, nearly four years after its official discovery observation at Algiers–Bouzaréah.[1]

Naming

This minor planet was named after Jacqueline Zadoc-Kahn Eisenmann (1904–1998),[11] a French physicist and long-time student of Jekhowsky's. The naming was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 97).[2]

Physical characteristics

In the Bus–Binzel SMASS classification, Jacqueline is a common, carbonaceous C-type asteroid.[3][10]

Rotation period

In May 2000, a rotational lightcurve of Jacqueline was obtained from photometric observations by American photometrist Robert Stephens at the Santana Observatory (646) in California. Analysis of the classically shaped bimodal lightcurve gave a well-defined rotation period of 7.87±0.01 hours and a brightness variation of 0.6±0.02 magnitude, indicative of a non-spheroidal shape ({{{1}}}).[9] Other measurements by Eric Barbotin and by astronomers at the Palomar Transient Factory gave a similar period of 7.873 and 7.875 hours with an amplitude of 0.72 and 0.43 magnitude, respectively ({{{1}}}).[12][13]

In 2016, a lightcurve was published using modeled photometric data from the Lowell Photometric Database. It gave a concurring sidereal period of 7.87149 hours, as well as two spin axes of (7.0°, 55.0°) and (170.0°, 65.0°) in ecliptic coordinates (λ, β).[14]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Jacqueline measures (37.65±3.4), (38.87±0.51) and (40.152±0.199) kilometers in diameter and its surface has an albedo of (0.0544±0.011), (0.051±0.002) and (0.052±0.005), respectively.[6][7][8] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0497 and a diameter of 37.61 kilometers based on an absolute magnitude of 11.0.[10]

Alternative mean-diameter measurements published by the WISE team include (29.523±10.14 km), (30.09±11.84 km), (31.991±0.454 km), (32.631±9.058 km) and (45.056±0.325 km) with corresponding albedos of (0.0670±0.0538), (0.07±0.06), (0.069±0.012), (0.06±0.02) and (0.0380±0.0053).[5][10]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 "1017 Jacqueline (A924 CH)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1017. Retrieved 12 March 2020. 
  2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(1017) Jacqueline". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 88. doi:10.1007/978-3-540-29925-7_1018. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "JPL Small-Body Database Browser: 1017 Jacqueline (A924 CH)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001017. Retrieved 12 March 2020. 
  4. ↑ 4.0 4.1 "Asteroid 1017 Jacqueline – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1017. 
  5. ↑ 5.0 5.1 5.2 5.3 5.4 "Asteroid 1017 Jacqueline – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1017+Jacqueline. Retrieved 24 October 2019. 
  6. ↑ 6.0 6.1 6.2 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 12 March 2020. 
  7. ↑ 7.0 7.1 7.2 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  8. ↑ 8.0 8.1 8.2 Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R. et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. Bibcode: 2016PDSS..247.....M. https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab. Retrieved 12 March 2020. 
  9. ↑ 9.0 9.1 Stephens, R. D. (December 2000). "Rotational Periods and Lightcurves of 891 Gunhild and 1017 Jacqueline". Minor Planet Bulletin 27 (1): 54–55. Bibcode: 2000MPBu...27...54S. http://www.minorplanet.info/MPB/issues/MPB_27-1.pdf. 
  10. ↑ 10.0 10.1 10.2 10.3 "LCDB Data for (1017) Jacqueline". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1017%7CJacqueline. Retrieved 8 March 2018. 
  11. ↑ "Jacqueline Eisenmann (Zadoc-Kahn)". www.geni.com. https://www.geni.com/people/Jacqueline-Eisenmann/6000000025241158880. Retrieved 8 March 2018. 
  12. ↑ Behrend, Raoul. "Asteroids and comets rotation curves – (1017) Jacqueline". Geneva Observatory. http://obswww.unige.ch/~behrend/page3cou.html#001017. Retrieved 8 March 2018. 
  13. ↑ Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal 150 (3): 35. doi:10.1088/0004-6256/150/3/75. Bibcode: 2015AJ....150...75W. 
  14. ↑ Durech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database". Astronomy and Astrophysics 587: 6. doi:10.1051/0004-6361/201527573. Bibcode: 2016A&A...587A..48D. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016A&A...587A..48D. Retrieved 8 March 2018. 

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