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1159 Granada
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Dark background asteroid
October 2019
yes
1159 Granada
#D6D6D6
K. Reinmuth
Heidelberg Obs.
2 September 1929
(1159) Granada
1929 RD1931 AR1940 RS
Granada (Spanish city and province)
main-belt(inner)
4 September 2017 (JD 2458000.5)
0
87.84 yr (32,083 days)
2.5184 AU
2.2409 AU
2.3797 AU
0.0583
3.67 yr (1,341 days)
35.176°
0.2685 ms / day
13.031°
347.89°
313.33°
27.839 0.283 km28.641 0.460 km29.94 km (derived)29.98 0.9 km30.14 9.34 km30.26 0.11 km30.26 0.29 km34.65 12.83 km
31 h72.852 0.2429 h
0.028 0.0140.031 0.0020.0379 0.00380.04 0.000.04 0.020.0439 (derived)0.047 0.0010.0471 0.003
S (assumed)B–V 0.680U–B 0.360
11.385 0.001 (R)11.5511.5811.6311.78 0.4311.81
1159 Granada, provisional designation 1929 RD, is a dark background asteroid and relatively slow rotator from the inner regions of the asteroid belt, approximately 30 kilometers in diameter. It was discovered on 2 September 1929, by astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The asteroid was named for the Spanish city and province of Granada.
Orbit and classification
Granada is a background asteroid that does not belong to any known asteroid family. It orbits the Sun in the inner main-belt at a distance of 2.2–2.5 AU once every 3 years and 8 months (1,341 days). Its orbit has an eccentricity of 0.06 and an inclination of 13° with respect to the ecliptic. The body's observation arc begins nine days after its official discovery observation at Heidelberg.
Physical characteristics
Although Granada is an assumed S-type asteroid, it has a notably low albedo (see below) for an asteroid of the inner main-belt, even below that of most carbonaceous asteroids.
Slow rotation
In September 1984, a rotational lightcurve of Granada was obtained from photometric observations by astronomer Richard Binzel. Lightcurve analysis gave a rotation period of 31 hours with a brightness variation of 0.28 magnitude (U=2). In October 2010, photometric observations in the R-band by astronomers at the Palomar Transient Factory gave a period of 72.852 hours and an amplitude of 0.24 (U=2). While not being a slow rotator, Granadas period is significantly longer than the typical 2 to 20 hours measures for most asteroids.
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, Granada measures between 27.839 and 34.65 kilometers in diameter and its surface has a low albedo between 0.028 and 0.0471.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0439 and a diameter of 29.94 kilometers based on an absolute magnitude of 11.63.
Naming
This minor planet was named after Granada, city and province in Andalusia in southern. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 108).
References
30em 2017-07-05 last obs.
JPL Small-Body Database Browser: 1159 Granada (1929 RD)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001159
Jet Propulsion Laboratory
7 September 2017
Dictionary of Minor Planet Names – (1159) Granada
Schmadel Lutz D.
Springer Berlin Heidelberg
98
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1160 (1159) Granada
1159 Granada (1929 RD)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1159
7 September 2017
6
Joseph R. Masiero
A. K. Mainzer
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J. M. Bauer
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M. F. Skrutskie
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E. DeBaun
D. Elsbury
T. IV Gautier
S. Gomillion
A. Wilkins
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The Astrophysical Journal
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7 September 2017
6
Joseph R. Masiero
A. K. Mainzer
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C. Nugent
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Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
The Astrophysical Journal Letters
759
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46350317 7 September 2017
6
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NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N
The Astrophysical Journal
814
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9341381 7 September 2017
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The Astronomical Journal
152
3
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2016AJ....152...63N
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Daisuke Kuroda
Thomas G. Müller
Sunao Hasegawa
Masateru Ishiguro
Takafumi Ootsubo
Daisuke Ishihara
Hirokazu Kataza
Satoshi Takita
Shinki Oyabu
Munetaka Ueno
Hideo Matsuhara
Takashi Onaka
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(online, AcuA catalog p. 153)
E. F. Tedesco
P. V. Noah
M. Noah
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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
A. Mainzer
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J. Masiero
E. Hand
J. Bauer
D. Tholen
R. S. McMillan
T. Spahr
R. M. Cutri
E. Wright
J. Watkins
W. Mo
C. Maleszewski
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The Astrophysical Journal
741
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2011ApJ...741...90M
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1109.6407 35447010
Binzel, R. P.
October 1987
A photoelectric survey of 130 asteroids
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Icarus
72
1
135–208
0019-1035
1987Icar...72..135B
10.1016/0019-1035(87)90125-4
7 September 2017
6
Adam Waszczak
Chan-Kao Chang
Eran O. Ofek
Russ Laher
Frank Masci
David Levitan
Jason Surace
Yu-Chi Cheng
Wing-Huen Ip
Daisuke Kinoshita
George Helou
Thomas A. Prince
Shrinivas Kulkarni
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Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
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8342929 7 September 2017
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
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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
1159
1158 Luda 1159 1160 Illyria
001159
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
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