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1018 Arnolda
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Main-belt asteroid
October 2019
yes
1018 Arnolda
#D6D6D6
K. Reinmuth
Heidelberg Obs.
3 March 1924
(1018) Arnolda
1924 QM1926 VK1952 BV 1
Arnold Berliner(German physicist)
main-belt(central)
4 September 2017 (JD 2458000.5)
0
93.34 yr (34,092 days)
3.1649 AU
1.9180 AU
2.5414 AU
0.2453
4.05 yr (1,480 days)
204.40°
0.2433 ms / day
7.6444°
359.70°
342.97°
13.68 2.45 km15.29 0.53 km16.387 0.100 km16.42 1.5 km16.44 km (derived)16.557 0.224 km
10 h (unrated)11.97 h (dated)12.18 0.01 h14.57 0.01 hAznar-2016a14.617 0.004 h
0.29 0.130.3701 0.0790.371 0.0370.3760 (derived)0.3857 0.03290.439 0.034
S
10.6010.6211.3011.45 0.25
1018 Arnolda, provisional designation 1924 QM, is a stony asteroid from the central regions of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 3 March 1924, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named after physicist Arnold Berliner.
Classification and orbit
Arnolda is not a member of any known asteroid family. It orbits the Sun in the central main belt at a distance of 1.9–3.2 AU once every 4 years and 1 month (1,480 days). Its orbit has an eccentricity of 0.25 and an inclination of 8° with respect to the ecliptic. The body's observation arc begins nine days prior to its official discovery observation at Heidelberg.
Physical characteristics
Arnolda is an assumed stony S-type asteroid, a very common type in the inner and in parts of the central asteroid belt.
Lightcurves
In May 2005, the best-rated rotational lightcurve of Arnolda was obtained from photometric observations by Australian astronomers at the Oakley Southern Sky Observatory (E09). Lightcurve analysis gave a rotation period of 14.617 hours with a brightness variation of 0.33 magnitude (U=3). Several other astronomers obtained number of lesser-rated lightcurves with a shorter period (U=n.a./1/2/3-).Aznar-2016a
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, Arnolda measures between 13.68 and 16.557 kilometers in diameter and its surface has an albedo between 0.29 and 0.439.
The Collaborative Asteroid Lightcurve Link derives a high albedo of 0.3760 and a diameter of 16.44 kilometers based on an absolute magnitude of 10.60.
Naming
This minor planet was named after physicist Arnold Berliner (1862–1942), on the occasion of his 70th birthday in 1933. Berliner was the editor of the prominent German periodical scientific magazine Naturwissenschaften (AN 247).
Notes
Aznar-2016a Aznar (2016): rotation period of 14.57 0.01 hours with a brightness amplitude of 0.39 mag. The lightcurve has a quality code of 3-. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)
References
30em 2017-06-04 last obs.
JPL Small-Body Database Browser: 1018 Arnolda (1924 QM)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001018
Jet Propulsion Laboratory
29 August 2017
Dictionary of Minor Planet Names – (1018) Arnolda
Schmadel Lutz D.
Springer Berlin Heidelberg
88
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1019 (1018) Arnolda
1018 Arnolda (1924 QM)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1018
29 August 2017
Asteroids and comets rotation curves – (1018) Arnolda
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page3cou.html#001018
29 August 2017
3 December 2002
https://web.archive.org/web/20021203214643/http://obswww.unige.ch/~behrend/page3cou.html#001018
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Joseph R. Masiero
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A. K. Mainzer
C. R. Nugent
J. M. Bauer
R. Stevenson
S. Sonnett
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Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M
The Astrophysical Journal
791
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11
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10.1088/0004-637X/791/2/121
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119293330 29 August 2017
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29 August 2017
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NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos
The Astronomical Journal
152
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1606.08923
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Fumihiko Usui
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Thomas G. Müller
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Masateru Ishiguro
Takafumi Ootsubo
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Hirokazu Kataza
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Shinki Oyabu
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Publications of the Astronomical Society of Japan
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IRAS Minor Planet Survey V6.0
https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
NASA Planetary Data System
12
IRAS-A-FPA-3-RDR-IMPS-V6.0
2004PDSS...12.....T
22 October 2019
6
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NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
The Astrophysical Journal
741
2
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10.1088/0004-637X/741/2/90
1109.6407 35447010
Binzel, R. P.
October 1987
A photoelectric survey of 130 asteroids
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10.1016/0019-1035(87)90125-4
29 August 2017
Zachary Pligge
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Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2010 May
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External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1018
1017 Jacqueline 1018 1019 Strackea
001018
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
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