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1200 Imperatrix
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Hygiean asteroid
October 2019
yes
1200 Imperatrix
#D6D6D6
K. Reinmuth
Heidelberg Obs.
14 September 1931
(1200) Imperatrix
1931 RH1929 CX1950 DC 11957 OYA913 ECA915 TLA924 GC
ɪ m p ə ˈ r eɪ t r ɪ k simperator
empress (in Latin)
main-belt(outer)Hygiea
4 September 2017 (JD 2458000.5)
0
101.75 yr (37,165 days)
3.3873 AU
2.7436 AU
3.0654 AU
0.1050
5.37 yr (1,960 days)
114.85°
0.1836 ms / day
4.5935°
204.77°
51.583°
36.00 0.42 km37.36 9.71 km39.39 km (derived)39.52 3.9 km42.006 0.390 km42.777 0.309 km43.64 0.61 km
13.34 0.11 h17.769 0.002 h
0.04 0.040.0545 (derived)0.060 0.0020.0609 0.01180.065 0.0090.0714 0.017
C (assumed)
10.5010.74 0.2810.8010.910.91
1200 Imperatrix (provisional designation 1931 RH) is a carbonaceous Hygiean asteroid from the outer regions of the asteroid belt, approximately 40 km in diameter. It was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory on 14 September 1931. The asteroid was named after the Latin word for empress.
Orbit and classification
Imperatrix is a member of the Hygiea family (601), a very large asteroid family named after 10 Hygiea, the main belt's fourth-largest asteroid. 'mperatrix orbits the Sun in the outer main-belt at a distance of 2.7–3.4 AU once every 5 years and 4 months (1,960 days). Its orbit has an eccentricity of 0.11 and an inclination of 5° with respect to the ecliptic.
The body's observation arc begins with its first identification as A913 EC at Simeiz Observatory in March 1913, more than 18 years prior to its official discovery observation at Heidelberg.
Physical characteristics
Imperatrix is an assumed C-type asteroid which is also the overall spectral type of the Hygiea family.23
Rotation period
In August 2000, a rotational lightcurve of Imperatrix was obtained from photometric observations at the River Oaks Observatory (915) in Texas. Lightcurve analysis gave a rotation period of 13.34 hours with a brightness variation of 0.23 magnitude (U=2). In September 2011, photometric observations by French amateur astronomers Pierre Antonini and René Roy gave a refined period of 17.769 hours with an amplitude of 0.21 magnitude (U=3).
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, Imperatrix measures between 36.00 and 43.64 kilometers in diameter and its surface has an albedo between 0.04 and 0.0714.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0545 and a diameter of 39.39 kilometers based on an absolute magnitude of 10.8.
Four stellar occultation events by 1200 Imperatrix have been observed, all in 2021.
Naming
This minor planet was named "Imperatrix", which is Latin for empress. The naming was proposed by German ARI-astronomer Gustav Stracke, after whom 1019 Strackea was named. Any specific reference to an occurrence or person is unknown, according to the author of the Dictionary of Minor Planets, Lutz Schmadel and his communications with Ingrid van Houten-Groeneveld, who also worked at Heidelberg).
References
30em 2017-07-03 last obs.
JPL Small-Body Database Browser: 1200 Imperatrix (1931 RH)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001200
Jet Propulsion Laboratory
26 September 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
100
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1201 (1200) Imperatrix
1200 Imperatrix (1931 RH)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1200
26 September 2017
Asteroids and comets rotation curves – (1200) Imperatrix
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page3cou.html#001200
26 September 2017
23 April 2019
https://web.archive.org/web/20190423121547/http://obswww.unige.ch/~behrend/page3cou.html#001200
dead
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
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
26 September 2017
Asteroid 1200 Imperatrix – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1200+Imperatrix#Asteroid%201200%20ImperatrixEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
26 October 2019
https://web.archive.org/web/20201004034009/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1200+Imperatrix#Asteroid%201200%20ImperatrixEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
4 October 2020
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
1200
26 September 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
26 September 2017
6
C. R. Nugent
A. Mainzer
J. Bauer
R. M. Cutri
E. A. Kramer
T. Grav
J. Masiero
S. Sonnett
E. L. Wright
September 2016
NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos
The Astronomical Journal
152
3
12
2016AJ....152...63N
10.3847/0004-6256/152/3/63
1606.08923
free
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)
E. F. Tedesco
P. V. Noah
M. Noah
S. D. Price
October 2004
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
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
Holliday, B.
March 2001
Photometry of Asteroid 191 Kolga and 1200 Imperatrix
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2001MPBu...28...13H
The Minor Planet Bulletin
28
13
2001MPBu...28...13H
26 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
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
26 September 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
1200
1199 Geldonia 1200 1201 Strenua
001200
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
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