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1372 Haremari
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Asteroid
October 2019
yes
1372 Haremari
#D6D6D6
K. Reinmuth
Heidelberg Obs.
31 August 1935
(1372) Haremari
1935 QK1928 DX1937 BD1944 QK1951 EW 11953 OM1953 PZ
all female staff members of ARI
main-belt(middle)WatsoniaCeres trojan
4 September 2017 (JD 2458000.5)
0
89.18 yr (32,574 days)
3.1761 AU
2.3557 AU
2.7659 AU
0.1483
4.60 yr (1,680 days)
243.89°
0.2143 ms / day
16.450°
327.45°
88.484°
21.96 0.72 km23.90 0.53 km24.18 km (derived)26.491 0.292 km27.724 0.158 km31.17 8.52 km
15.25 0.03 h
0.0303 0.00210.039 0.0120.09 0.030.1097 (derived)0.126 0.0060.146 0.027
SMASS L
11.0011.112.2
1372 Haremari, provisional designation 1935 QK, is a rare-type Watsonian asteroid and a suspected trojan of Ceres from the central regions of the asteroid belt, approximately 26 kilometers in diameter. It was discovered on 31 August 1935, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named for all female staff members of the Astronomical Calculation Institute.
Orbit and classification
Haremari is a member of the very small Watsonia family (537), named after its parent body, namesake and largest member, 729 Watsonia.23
It orbits the Sun in the central main-belt at a distance of 2.4–3.2 AU once every 4 years and 7 months (1,680 days). Its orbit has an eccentricity of 0.15 and an inclination of 16° with respect to the ecliptic. The body's observation arc begins with its first observation at Heidelberg in February 1928, more than seven years prior to its official discovery observation.
Trojan of Ceres
Long-term numerical integrations suggest that Haremari is a trojan of Ceres, staying a 1:1 orbital resonance with the only dwarf planet of the asteroid belt. It is thought that Haremari is currently transiting from a tadpole to a horseshoe orbit. Other suspected co-orbitals are the asteroids 855 Newcombia, 4608 Wodehouse, and 8877 Rentaro.
Physical characteristics
In the SMASS classification, Haremari is a rare L-type asteroid with a moderate albedo. This type corresponds with the overall spectral type of the Watsonia family.23
Rotation period
In November 2009, a rotational lightcurve of Haremari was obtained from photometric observations by Richard Durkee at the Shed of Science Observatory (H39). Lightcurve analysis gave a rotation period of 15.25 hours with a brightness amplitude of 0.12 magnitude (U=2).
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, Haremari measures between 21.96 and 31.17 kilometers in diameter and its surface has an albedo between 0.0303 and 0.146.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1097 and a diameter of 24.18 kilometers based on an absolute magnitude of 11.1.
Naming
This minor planet jointly honors all the female staff members of the Astronomical Calculation Institute (Heidelberg University) (de Astronomisches Rechen-Institut), commonly known as ARI. In often published versions, "Haremari" is a composed name and means "the harem of A.R.I.".
Alternative version
According to Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg, Reinmuth had often been asked by his colleges at ARI to name some of his discoveries after their female friends, as well as after popular actresses (and not just the female staff at ARI). He then compiled all these proposals to the name "Haremari". However, as Groeneveld recorded, "Reinmuth did not want to publish the original meaning and he, therefore, devised the interpretation of the first sentence in 1948".
References
30em 2017-05-04 last obs.
JPL Small-Body Database Browser: 1372 Haremari (1935 QK)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001372
Jet Propulsion Laboratory
31 October 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
111
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1373 (1372) Haremari
1372 Haremari (1935 QK)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1372
31 October 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
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
119293330 31 October 2017
Asteroid 1372 Haremari – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1372+Haremari#Asteroid%201372%20HaremariEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
26 October 2019
20 August 2020
https://web.archive.org/web/20200820012614/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1372%20Haremari#Asteroid%201372%20HaremariEAR-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 119280014
Christou, A. A.
April 2000
Co-orbital objects in the main asteroid belt
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2000A&A...356L..71C
Astronomy and Astrophysics
356
L71–L74
2000A&A...356L..71C
31 October 2017
Christou, A.
November 2001
The Trojans of Ceres and Vesta
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2001DPS....33.5205C
American Astronomical Society
33
1134
2001DPS....33.5205C
31 October 2017
1372
31 October 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
46350317 31 October 2017
6
C. R. Nugent
A. Mainzer
J. Masiero
J. Bauer
R. M. Cutri
T. Grav
E. Kramer
S. Sonnett
R. Stevenson
E. L. Wright
December 2015
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
2
13
2015ApJ...814..117N
10.1088/0004-637X/814/2/117
1509.02522
9341381 31 October 2017
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)
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 35447010
Durkee, Russell I.
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http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37..125D
The Minor Planet Bulletin
37
3
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External links
Nueva órbita del asteroide 1.372 Haremari, José María González Aboin, Universidad de Madrid (1954) es
Les noms des astéroïdes, M.-A. Combes, L'Astronomie, Vol. 87, (1974) fr
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
1372
1371 Resi 1372 1373 Cincinnati
001372
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
001372
Category:Ceres trojans
001372
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