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1067 Lunaria
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Itha asteroid
October 2019
yes
1067 Lunaria
#D6D6D6
K. Reinmuth
Heidelberg Obs.
9 September 1926
(1067) Lunaria
1926 RG1974 PJ1974 QC 3
l uː ˈ n ɛər i əlunarian
Lunaria (flowering plant)
main-belt(outer)Itha
4 September 2017 (JD 2458000.5)
0
90.74 yr (33,142 days)
3.4206 AU
2.3207 AU
2.8706 AU
0.1916
4.86 yr (1,777 days)
222.90°
0.2026 ms / day
10.547°
289.59°
115.03°
15.43 0.73 km18.02 1.33 km18.07 km (derived)20.011 0.100 km22.968 0.243 km
6.057 0.001 h7.74 h
0.1240 0.02250.185 0.0120.20 (assumed)0.221 0.0340.298 0.057
L/SS
10.85 0.3110.9911.08
1067 Lunaria, provisional designation 1926 RG, is a stony Itha asteroid from the outer regions of the asteroid belt, approximately 18 kilometers in diameter. It was discovered on 9 September 1926, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named after the flowering plant Lunaria (honesty).
Orbit and classification
Lunaria is a member of the Itha family, a very small family of asteroids, named after its parent body 918 Itha.23
It orbits the Sun in the outer asteroid belt at a distance of 2.3–3.4 AU once every 4 years and 10 months (1,777 days; semi-major axis of 2.87 AU). Its orbit has an eccentricity of 0.19 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins at Heidelberg in October 1926, one month after its official discovery observation.
Physical characteristics
Lunaria has been characterized as both L- and S-type asteroid by Pan-STARRS photometric survey. The overall spectral type for the Itha family is that of a stony S-type.23
Rotation period
In July 1984, a first rotational lightcurve of Lunaria was obtained by American astronomer Richard Binzel. Lightcurve analysis gave a rotation period of 7.74 hours with a brightness variation of 0.13 magnitude (U=2). In September 2004, Donald Pray at the Carbuncle Hill Observatory (I00) derived a refined period of 6.057 hours with an amplitude of 0.27 magnitude from photometric observations (U=3).
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lunaria measures between 15.43 and 22.968 kilometers in diameter and its surface has an albedo between 0.1240 and 0.298.
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 18.07 kilometers based on an absolute magnitude of 11.08.
Naming
This minor planet was named after Lunaria (commonly known as "honesty"), a flowering plant in the mustard family. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 101).
Reinmuth's flowers
Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between 1009 (1009) and 1200 (1200). This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were exclusively named after plants, in particular flowering plants (also see list of minor planets named after animals and plants).
References
30em 2017-06-05 last obs.
JPL Small-Body Database Browser: 1067 Lunaria (1926 RG)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001067
Jet Propulsion Laboratory
7 December 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
91
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1068 (1067) Lunaria
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
90
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1055 (1054) Forsytia
1067 Lunaria (1926 RG)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1067
7 December 2017
6
Joseph R. Masiero
T. Grav
A. K. Mainzer
C. R. Nugent
J. M. Bauer
R. Stevenson
S. Sonnett
August 2014
Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
Asteroid 1067 Lunaria – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1067+Lunaria#Asteroid%201067%20LunariaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
26 October 2019
3 October 2020
https://web.archive.org/web/20201003181940/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1067+Lunaria#Asteroid%201067%20LunariaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
dead
D. Nesvorný
M. Broz
V. Carruba
December 2014
Identification and Dynamical Properties of Asteroid Families
Asteroids IV
297–321
2015aste.book..297N
10.2458/azu_uapress_9780816532131-ch016
1502.01628
9780816532131
1067
7 December 2017
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
C. Nugent
M. S. Cabrera
November 2012
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
1
5
2012ApJ...759L...8M
10.1088/2041-8205/759/1/L8
1209.5794
7 December 2017
6
A. Mainzer
T. Grav
J. Masiero
E. Hand
J. Bauer
D. Tholen
R. S. McMillan
T. Spahr
R. M. Cutri
E. Wright
J. Watkins
W. Mo
C. Maleszewski
November 2011
NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407
6
Fumihiko Usui
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
October 2011
Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
Publications of the Astronomical Society of Japan
63
5
1117–1138
2011PASJ...63.1117U
10.1093/pasj/63.5.1117
(online, AcuA catalog p. 153)
Binzel, R. P.
October 1987
A photoelectric survey of 130 asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1987Icar...72..135B
Icarus
72
1
135–208
0019-1035
1987Icar...72..135B
10.1016/0019-1035(87)90125-4
7 December 2017
Pray, Donald P.
March 2005
Lightcurve analysis of asteroids 276, 539, 1014, 1067, 3693 and 4774
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005MPBu...32....8P
The Minor Planet Bulletin
32
1
8–9
1052-8091
2005MPBu...32....8P
7 December 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
Christopher Waters
November 2015
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V
Icarus
261
34–47
2015Icar..261...34V
10.1016/j.icarus.2015.08.007
1506.00762
7 December 2017
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
1067
1066 Lobelia 1067 1068 Nofretete
001067
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
19260909