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词条 1392 Pierre
释义

  1. Orbit and classification

  2. Physical characteristics

      Rotation period    Diameter and albedo  

  3. Naming

  4. References

  5. External links

{{Infobox planet
| minorplanet = yes
| name = 1392 Pierre
| background = #D6D6D6
| image =
| image_size =
| caption =
| discovery_ref =  
| discoverer = L. Boyer
| discovery_site = Algiers Obs.
| discovered = 16 March 1936
| mpc_name = (1392) Pierre
| alt_names = 1936 FO{{·}}1938 SZ
1955 TZ{{·}}1959 SH
A917 UB
| pronounced =
| named_after = Pierre [2] {{small|(discoverer's nephew)}}
| mp_category = main-belt{{·}}{{small|(middle)}}
Eunomia [3]{{·}}background [4]
| orbit_ref =  
| epoch = 4 September 2017 (JD 2458000.5)
| uncertainty = 0
| observation_arc = 81.30 yr (29,695 days)
| aphelion = 3.1355 AU
| perihelion = 2.0788 AU
| semimajor = 2.6071 AU
| eccentricity = 0.2026
| period = 4.21 yr (1,538 days)
| mean_anomaly = 244.35°
| mean_motion = {{Deg2DMS|0.2341|sup=ms}} / day
| inclination = 12.263°
| asc_node = 358.24°
| arg_peri = 44.290°
| dimensions = {{val|26.16|0.34}} km[6]
{{val|26.44|1.6}} km[3][8]
{{val|27.02|5.29}} km[9]
{{val|28.94|8.81}} km[10]
| rotation = {{val|18}} h[11]
{{val|24}} h {{small|(poor)}}[12]
| albedo = {{val|0.04|0.01}}[9]
{{val|0.04|0.02}}[10]
{{val|0.0519|0.007}}[3][8]
{{val|0.054|0.002}}[6]
| spectral_type = Tholen {{=}} DX [3]{{·}}C [20]
B–V {{=}} 0.757 
U–B {{=}} 0.258 
| abs_magnitude = 11.72[3][6][8][10]{{·}}{{val|11.74|0.34}}[20]{{·}}12.03[9]
}}1392 Pierre, provisional designation {{mp|1936 FO}}, is a dark, dynamical Eunomian asteroid from the central regions of the asteroid belt, approximately 26 kilometers in diameter. It was discovered on 16 March 1936, by astronomer Louis Boyer at the Algiers Observatory in Algeria, North Africa.[30] The asteroid was named after the discoverer's nephew, Pierre.[2]

Orbit and classification

Pierre is a dynamical member of the Eunomia family ({{small|502}}),[3] a prominent family of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members.[4] However, it is a non-family asteroid of the main belt's background population when applying the Hierarchical Clustering Method to its proper orbital elements.[4] As Pierre{{'}}s spectral type is also different from that of the Eunomia family (see below), it is possibly an interloper to the Eunomia family rather than a true member.{{citation needed|date=October 2017}}

It orbits the Sun in the central main-belt at a distance of 2.1–3.1 AU once every 4 years and 3 months (1,538 days). Its orbit has an eccentricity of 0.20 and an inclination of 12° with respect to the ecliptic.

The asteroid was first identified as {{mp|A917 UB}} at Simeiz Observatory in October 1917. The body's observation arc begins with its official discovery observation at Algiers in March 1936.[30]

Physical characteristics

Pierre has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey.[20] In the Tholen classification, the asteroid's spectral type is ambiguous, closest to a dark D-type and somewhat similar to a generic X-type asteroid. Conversely, the Eunomia family consists of S-type asteroids.[39]{{rp|23}}

Rotation period

In August 1984, a first rotational lightcurve of Pierre was obtained from photometric observations with the ESO 1-metre telescope at the La Silla Observatory in Chile. Lightcurve analysis gave a rotation period of 18 hours with a brightness variation of 0.09 magnitude ({{small|U=2}}).[11] A poorly rated lightcurve by Pierre Antonini in Januar 2007, gave a period of 24 hours with an amplitude of 0.05 magnitude.[12]

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, Pierre measures between 26.16 and 28.94 kilometers in diameter and its surface has an albedo between 0.04 and 0.054.[6][8][9][10]

The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0519 and a diameter of 26.44 kilometers based on an absolute magnitude of 11.72.[3][8]

Naming

This minor planet was named after Pierre, a nephew of the discoverer Louis Boyer. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 ({{small|H 126}}).[2]

References

1. ^{{cite book |title = Dictionary of Minor Planet Names – (1392) Pierre |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 112 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1393 |chapter = (1392) Pierre }}
2. ^{{cite web |title = 1392 Pierre (1936 FO) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1392 |accessdate = 26 October 2017}}
3. ^{{cite web |title = Asteroids and comets rotation curves – (1392) Pierre |last = Behrend |first = Raoul |publisher = Geneva Observatory |url = http://obswww.unige.ch/~behrend/page4cou.html#001392 |accessdate = 26 October 2017}}
4. ^{{cite web |title = Small Bodies Data Ferret |work = Nesvorny HCM Asteroid Families V3.0 |url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action |accessdate = 26 October 2017}}
5. ^{{Cite book |first1 = D. |last1 = Nesvorný |first2 = M. |last2 = Broz |first3 = V. |last3 = Carruba |date = December 2014 |title = Identification and Dynamical Properties of Asteroid Families |journal = Asteroids IV |pages = 297–321 |bibcode = 2015aste.book..297N |doi = 10.2458/azu_uapress_9780816532131-ch016 |arxiv = 1502.01628 |isbn = 9780816532131 }}
6. ^{{cite web |title = LCDB Data for (1392) Pierre |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1392%7CPierre |accessdate = 26 October 2017}}
7. ^{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Masiero |first4 = J. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = T. |last6 = Grav |first7 = E. |last7 = Kramer |first8 = S. |last8 = Sonnett |first9 = R. |last9 = Stevenson |first10 = E. L. |last10 = Wright |date = December 2015 |title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N |journal = The Astrophysical Journal |volume = 814 |issue = 2 |page = 13 |bibcode = 2015ApJ...814..117N |doi = 10.1088/0004-637X/814/2/117 |arxiv = 1509.02522 |access-date= 26 October 2017}}
8. ^{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Bauer |first4 = R. M. |last4 = Cutri |first5 = E. A. |last5 = Kramer |first6 = T. |last6 = Grav |first7 = J. |last7 = Masiero |first8 = S. |last8 = Sonnett |first9 = E. L. |last9 = Wright |date = September 2016 |title = NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016AJ....152...63N |journal = The Astronomical Journal |volume = 152 |issue = 3 |page = 12 |bibcode = 2016AJ....152...63N |doi = 10.3847/0004-6256/152/3/63 |arxiv = 1606.08923 |access-date= 26 October 2017}}
9. ^{{cite journal |display-authors = 6 |first1 = Fumihiko |last1 = Usui |first2 = Daisuke |last2 = Kuroda |first3 = Thomas G. |last3 = Müller |first4 = Sunao |last4 = Hasegawa |first5 = Masateru |last5 = Ishiguro |first6 = Takafumi |last6 = Ootsubo |first7 = Daisuke |last7 = Ishihara |first8 = Hirokazu |last8 = Kataza |first9 = Satoshi |last9 = Takita |first10 = Shinki |last10 = Oyabu |first11 = Munetaka |last11 = Ueno |first12 = Hideo |last12 = Matsuhara |first13 = Takashi |last13 = Onaka |date = October 2011 |title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey |url = http://pasj.oxfordjournals.org/content/63/5/1117.full.pdf+html |journal = Publications of the Astronomical Society of Japan |volume = 63 |issue = 5 |pages = 1117–1138 |bibcode = 2011PASJ...63.1117U |doi = 10.1093/pasj/63.5.1117 |access-date= 26 October 2017}}
10. ^{{cite journal |first1 = E. F. |last1 = Tedesco |first2 = P. V. |last2 = Noah |first3 = M. |last3 = Noah |first4 = S. D. |last4 = Price |date = October 2004 |title = IRAS Minor Planet Survey V6.0 |url = https://sbn.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab |journal = NASA Planetary Data System |pages = IRAS-A-FPA-3-RDR-IMPS-V6.0 |bibcode = 2004PDSS...12.....T |access-date = 26 October 2017 |archive-url = https://web.archive.org/web/20160603231123/http://sbn.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab |archive-date = 2016-06-03 |dead-url = yes |df = }}
11. ^{{Cite journal |first1 = M. A. |last1 = Barucci |first2 = M. |last2 = di Martino |first3 = M. |last3 = Fulchignoni |date = May 1992 |title = Rotational properties of small asteroids - Photoelectric observations |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1992AJ....103.1679B |journal = Astronomical Journal |volume = 103 |pages = 1679–1686 |issn = 0004-6256 |bibcode = 1992AJ....103.1679B |doi = 10.1086/116185 |access-date= 26 October 2017}}
12. ^{{cite journal |display-authors = 6 |first1 = Peter |last1 = Veres |first2 = Robert |last2 = Jedicke |first3 = Alan |last3 = Fitzsimmons |first4 = Larry |last4 = Denneau |first5 = Mikael |last5 = Granvik |first6 = Bryce |last6 = Bolin |first7 = Serge |last7 = Chastel |first8 = Richard J. |last8 = Wainscoat |first9 = William S. |last9 = Burgett |first10 = Kenneth C. |last10 = Chambers |first11 = Heather |last11 = Flewelling |first12 = Nick |last12 = Kaiser |first13 = Eugen A. |last13 = Magnier |first14 = Jeff S. |last14 = Morgan |first15 = Paul A. |last15 = Price |first16 = John L. |last16 = Tonry |first17 = Christopher |last17 = Waters |date = November 2015 |title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 26 October 2017}}
[1][2][3][4][5][6][7][8][9][10][11][12]

}}

External links

  • Asteroid Lightcurve Database (LCDB), query form (info)
  • [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • {{JPL small body}}
{{Minor planets navigator |1391 Carelia |number=1392 |1393 Sofala}}{{Small Solar System bodies}}{{DEFAULTSORT:Pierre}}

6 : Eunomia asteroids|Discoveries by Louis Boyer (astronomer)|Minor planets named for people|Named minor planets|DX-type asteroids (Tholen)|Astronomical objects discovered in 1936

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