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词条 1105 Fragaria
释义

  1. Orbit and classification

  2. Physical characteristics

      Rotation period    Diameter and albedo  

  3. Naming

      Reinmuth's flowers  

  4. References

  5. External links

{{Infobox planet
| minorplanet = yes
| name = 1105 Fragaria
| background = #D6D6D6
| image = 1105orbit.png
| image_size = 260
| caption = Orbital diagram of Fragaria
| discovery_ref =  
| discoverer = K. Reinmuth
| discovery_site = Heidelberg Obs.
| discovered = 1 January 1929
| mpc_name = (1105) Fragaria
| alt_names = 1929 AB{{·}}1947 KB
1977 EU{{·}}A916 MA
A917 UH
| pronounced = {{IPAc-en|f|r|ə|ˈ|ɡ|ɛər|i|ə}}
| named_after = Fragaria[2]
{{small|(flowering plant)}}
| mp_category = {{nowrap|main-belt{{·}}{{small|(outer)}}{{·}}Eos [3][4]}}
| orbit_ref =  
| epoch = 23 March 2018 (JD 2458200.5)
| uncertainty = 0
| observation_arc = 89.13 yr (32,553 days)
| aphelion = 3.3288 AU
| perihelion = 2.6915 AU
| semimajor = 3.0101 AU
| eccentricity = 0.1059
| period = 5.22 yr (1,908 days)
| mean_anomaly = 110.60°
| mean_motion = {{Deg2DMS|0.1887|sup=ms}} / day
| inclination = 10.968°
| asc_node = 116.90°
| arg_peri = 225.01°
| mean_diameter = {{val|27.92|3.41}} km[6]
{{val|31.518|0.346}} km[7]
36.95 km {{small|(derived)}}[3]
{{val|37.03|3.8}} km[9]
{{val|38.206|0.703}} km[10]
{{val|38.41|0.46}} km[11]
| rotation = {{val|10.88|ul=h}}[12]
| albedo = {{val|0.1017|0.0167}}[10]
0.1086 {{small|(derived)}}[3]
{{val|0.113|0.003}}[11]
{{val|0.1186|0.029}}[9]
{{val|0.128|0.008}}[7]
{{val|0.166|0.058}}[6]
| spectral_type =Tholen {{=}} ST [3]{{·}}U/L [21]
B–V {{=}} {{val|0.776|029}}
U–B {{=}} {{val|0.419|0.049}}
| abs_magnitude = 10.09[9][11]
10.19[3][10][12]
10.34[6]
}}1105 Fragaria ({{IPAc-en|f|r|ə|ˈ|ɡ|ɛər|i|ə}}), provisional designation {{mp|1929 AB}}, is an uncommon Eoan asteroid from the outer regions of the asteroid belt, approximately {{convert|37|km|mi|abbr=off|sp=us}} in diameter. It was discovered on 1 January 1929, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany.[31] The asteroid was named after the flowering plant Fragaria (strawberry).[2]

Orbit and classification

Fragaria belongs to the Eos family ({{small|606}}),[3][4] the largest asteroid family of the outer asteroid belt consisting of nearly 10,000 members.[35] It orbits the Sun in the outer asteroid belt at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,908 days; semi-major axis of 3.01 AU). Its orbit has an eccentricity of 0.11 and an inclination of 11° with respect to the ecliptic.

The asteroid was first observed as {{mp|1916 MA}} at Simeiz Observatory in June 1916. The body's observation arc begins at Heidelberg in December 1928, three weeks prior to its official discovery observation.[31]

Physical characteristics

In the Tholen classification, Fragaria has an ambiguous spectral type, closest to an S-type and somewhat similar to the darker and uncommon T-type asteroids (ST),[3] while polarimetric observations characterized it as an U/L-type asteroid.[21] The overall spectral type for members of the Eos family is that of a K-type.[35]{{rp|23}}

Rotation period

In the 1990s, a rotational lightcurve of Fragaria was obtained from photometric observations by French and Italian astronomers at ESO's La Silla Observatory using the ESO 1-metre telescope. Lightcurve analysis gave a fragmentary rotation period of 10.88 hours with a brightness amplitude of 0.12 magnitude ({{small|U=1}}).[12] As of 2018, no secure period has been obtained.[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, Fragaria measures between 27.92 and 38.41 kilometers in diameter and its surface has an albedo between 0.1017 and 0.166.[6][7][9][10][11]

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1086 and a diameter of 36.95 kilometers based on an absolute magnitude of 10.19.[3]

Naming

This minor planet was named after Fragaria, the genus of flowering plants in the rose family, commonly known as strawberries.[2] The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 ({{small|H 104}}).[2]

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 {{MoMP|1009|(1009)}} and {{MoMP|1200|(1200)}}. This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were all named after plants, in particular flowering plants (also see list of minor planets named after animals and plants).[52]

References

1. ^{{cite book |title = Dictionary of Minor Planet Names – (1105) Fragaria |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 94 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1106 |chapter = (1105) Fragaria }}
2. ^{{cite book |title = Dictionary of Minor Planet Names – (1054) Forsytia |last = Schmadel |first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 90 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1055 |chapter = (1054) Forsytia }}
3. ^{{cite web |title = 1105 Fragaria (1929 AB) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=1105 |accessdate = 28 February 2018}}
4. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 }}
5. ^{{cite web |title = Small Bodies Data Ferret |work = Nesvorny HCM Asteroid Families V3.0 |url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action |accessdate = 28 February 2018}}
6. ^{{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 }}
7. ^{{cite web |title = LCDB Data for (1105) Fragaria |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1105%7CFragaria |accessdate = 28 February 2018}}
8. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = C. |last6 = Nugent |first7 = M. S. |last7 = Cabrera |date = November 2012 |title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids |journal = The Astrophysical Journal Letters |volume = 759 |issue = 1 |page = 5 |bibcode = 2012ApJ...759L...8M |doi = 10.1088/2041-8205/759/1/L8 |arxiv = 1209.5794 }}
9. ^{{cite journal |display-authors = 6 |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |first7 = R. S. |last7 = McMillan |first8 = T. |last8 = Spahr |first9 = R. M. |last9 = Cutri |first10 = E. |last10 = Wright |first11 = J. |last11 = Watkins |first12 = W. |last12 = Mo |first13 = C. |last13 = Maleszewski |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407 }}
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 = 28 February 2018 |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 = 3 June 2016 |dead-url = yes |df = dmy-all }}
11. ^{{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= 28 February 2018}}
12. ^{{Cite journal |first1 = M. A. |last1 = Barucci |first2 = M. |last2 = di Martino |first3 = E. |last3 = Dotto |first4 = M. |last4 = Fulchignoni |first5 = A. |last5 = Rotundi |first6 = R. |last6 = Burchi |date = June 1994 |title = Rotational properties of small asteroids: Photoelectric observations of 16 asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1994Icar..109..267B |journal = Icarus |volume = 109 |issue = 2 |pages = 267–273 |issn = 0019-1035 |bibcode = 1994Icar..109..267B |doi = 10.1006/icar.1994.1092 |access-date= 28 February 2018}}
13. ^{{Cite journal |display-authors = 6 |first1 = I. N. |last1 = Belskaya |first2 = S. |last2 = Fornasier |first3 = G. P. |last3 = Tozzi |first4 = R. |last4 = Gil-Hutton |first5 = A. |last5 = Cellino |first6 = K. |last6 = Antonyuk |first7 = Yu. N. |last7 = Krugly |first8 = A. N. |last8 = Dovgopol |first9 = S. |last9 = Faggi |date = March 2017 |title = Refining the asteroid taxonomy by polarimetric observations |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2017Icar..284...30B |journal = Icarus |volume = 284 |pages = 30–42 |bibcode = 2017Icar..284...30B |doi = 10.1016/j.icarus.2016.11.003 |access-date= 28 February 2018}}
[1][2][3][4][5][6][7][8][9][10][11][12][13]

}}

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}}
{{use dmy|date=February 2018}}{{Minor planets navigator |1104 Syringa |number=1105 |1106 Cydonia}}{{Small Solar System bodies}}{{DEFAULTSORT:Fragaria}}

6 : Eos asteroids|Discoveries by Karl Wilhelm Reinmuth|Minor planets named for plants|Named minor planets|ST-type asteroids (Tholen)|Astronomical objects discovered in 1929

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