Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Orbit and classification  



1.1  Trojan of Ceres  







2 Physical characteristics  



2.1  Rotation period  





2.2  Diameter and albedo  







3 Naming  



3.1  Alternative version  







4 References  





5 External links  














1372 Haremari






Asturianu
 / Bân-lâm-gú
Deutsch
Ελληνικά
Español
Esperanto
Euskara
فارسی
Français
Հայերեն
Italiano
Latina
Magyar
مصرى
Нохчийн
Norsk bokmål
Norsk nynorsk
Occitan
Polski
Português
Română
Slovenčina
Српски / srpski
Srpskohrvatski / српскохрватски
Svenska
Tagalog
Татарча / tatarça
Українська
Tiếng Vit
Yorùbá

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


1372 Haremari
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date31 August 1935
Designations

MPC designation

(1372) Haremari

Named after

all female staff members of ARI[2]

Alternative designations

1935 QK · 1928 DX
1937 BD · 1944 QK
1951 EW1 · 1953 OM
1953 PZ

Minor planet category

main-belt · (middle)
Watsonia[3] · Ceres trojan[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc89.18 yr (32,574 days)
Aphelion3.1761 AU
Perihelion2.3557 AU

Semi-major axis

2.7659 AU
Eccentricity0.1483

Orbital period (sidereal)

4.60 yr (1,680 days)

Mean anomaly

243.89°

Mean motion

0° 12m 51.48s / day
Inclination16.450°

Longitude of ascending node

327.45°

Argument of perihelion

88.484°
Physical characteristics
Dimensions21.96±0.72km[5]
23.90±0.53km[6]
24.18 km (derived)[7]
26.491±0.292km[8]
27.724±0.158km[9]
31.17±8.52km[10]

Synodic rotation period

15.25±0.03 h[11]

Geometric albedo

0.0303±0.0021[9]
0.039±0.012[8]
0.09±0.03[10]
0.1097 (derived)[7]
0.126±0.006[6]
0.146±0.027[5]

Spectral type

SMASS = L[1][7]

Absolute magnitude (H)

11.00[5][6][10] · 11.1[1][7] · 12.2[9]

1372 Haremari, provisional designation 1935 QK, is a rare-type Watsonian asteroid and a suspected trojanofCeres 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.[12] The asteroid was named for all female staff members of the Astronomical Calculation Institute.[2]

Orbit and classification[edit]

Haremari is a member of the very small Watsonia family (537), named after its parent body, namesake and largest member, 729 Watsonia.[3][13]: 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.[1] 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.[12]

Trojan of Ceres[edit]

Long-term numerical integrations suggest, that Haremari is a trojanofCeres, 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.[4][14]

Physical characteristics[edit]

In the SMASS classification, Haremari is a rare L-type asteroid with a moderate albedo.[1][7] This type corresponds with the overall spectral type of the Watsonia family.[13]: 23 

Rotation period[edit]

In November 2009, a rotational lightcurveofHaremari 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).[11]

Diameter and albedo[edit]

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.[5][6][8][9][10]

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.[7]

Naming[edit]

This minor planet jointly honors all the female staff members of the Astronomical Calculation Institute (Heidelberg University) (German: Astronomisches Rechen-Institut), commonly known as ARI. In often published versions, "Haremari" is a composed name and means "the harem of A.R.I.".[2]

Alternative version[edit]

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 wells 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".[2]

References[edit]

  1. ^ a b c d e f "JPL Small-Body Database Browser: 1372 Haremari (1935 QK)" (2017-05-04 last obs.). Jet Propulsion Laboratory. Retrieved 31 October 2017.
  • ^ a b c d Schmadel, Lutz D. (2007). "(1372) Haremari". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 111. doi:10.1007/978-3-540-29925-7_1373. ISBN 978-3-540-00238-3.
  • ^ a b "Asteroid 1372 Haremari – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
  • ^ a b Christou, A. A. (April 2000). "Co-orbital objects in the main asteroid belt". Astronomy and Astrophysics. 356: L71–L74. Bibcode:2000A&A...356L..71C. Retrieved 31 October 2017.
  • ^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317. Retrieved 31 October 2017.
  • ^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
  • ^ a b c d e f "LCDB Data for (1372) Haremari". Asteroid Lightcurve Database (LCDB). Retrieved 31 October 2017.
  • ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. S2CID 119293330. Retrieved 31 October 2017.
  • ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 35447010.
  • ^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID 9341381. Retrieved 31 October 2017.
  • ^ a b Durkee, Russell I. (July 2010). "Asteroids Observed from the Shed of Science Observatory: 2009 October - 2010 March". The Minor Planet Bulletin. 37 (3): 125–127. Bibcode:2010MPBu...37..125D. ISSN 1052-8091. Retrieved 31 October 2017.
  • ^ a b "1372 Haremari (1935 QK)". Minor Planet Center. Retrieved 31 October 2017.
  • ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. S2CID 119280014.
  • ^ Christou, A. (November 2001). "The Trojans of Ceres and Vesta". American Astronomical Society. 33: 1134. Bibcode:2001DPS....33.5205C. Retrieved 31 October 2017.
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=1372_Haremari&oldid=1191755871"

    Categories: 
    Minor planet object articles (numbered)
    Watsonia asteroids
    Discoveries by Karl Wilhelm Reinmuth
    Named minor planets
    Ceres (dwarf planet)
    Ceres trojans
    L-type asteroids (SMASS)
    Astronomical objects discovered in 1935
    Hidden categories: 
    Use dmy dates from October 2019
    Articles containing German-language text
    Articles with Spanish-language sources (es)
    Articles with French-language sources (fr)
    Webarchive template wayback links
    Articles with JPL SBDB identifiers
    Articles with MPC identifiers
     



    This page was last edited on 25 December 2023, at 15:47 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki