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{{Short description|Phocaea asteroid and potentially slow rotator}}
{{Use dmy dates|date=October 2019}}
{{Infobox planet
| minorplanet = yes
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}}
'''3322 Lidiya''', provisional designation {{
== Orbit and classification ==
The body's [[observation arc]] begins with its first identification as {{
▲''Lidiya'' is a member of the [[Phocaea family]] ({{small|[[FIN tbl#701|701]]}}),<ref name="Ferret" /> a large [[asteroid family]] of [[Kirkwood gap|inner]]-belt asteroids with a stony composition.<ref name="Nesvorny-2014" />{{rp|23}} It orbits the Sun at a distance of 1.9–2.9 [[Astronomical unit|AU]] once every 3 years and 8 months (1,351 days). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.22 and an [[orbital inclination|inclination]] of 23[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" />
▲The body's [[observation arc]] begins with its first identification as {{mpf|1975 VJ|6}} at Nauchnij in November 1975, one month prior to its official discovery observation.<ref name="MPC-object" />
== Physical characteristics ==
▲''Lidiya'' has been characterized as a stony [[S-type asteroid]] by [[PanSTARRS]] photoemteric survey.<ref name="Veres-2015" />
=== Potentially slow rotator ===
In December 2012, a fragmentary rotational [[lightcurve]] of
▲In December 2012, a fragmentary rotational [[lightcurve]] of ''Lidiya'' was obtained from photometric observations at the Altimira Observatory ({{small|[[IAU code#G76|G76]]}}) in California. Lightcurve analysis gave a [[rotation period]] of 710 hours with a brightness amplitude of 0.60 [[Magnitude (astronomy)|magnitude]] ({{small|[[LCDB quality code|U=1]]}}).<ref name="Buchheim-2014" /> This would make ''Lidiya'' one of the [[List of slow rotators (minor planets)|slowest rotators]] known to exist. However, since the lightcurve has such a poor quality rating, it is only a [[List of slow rotators (minor planets)#Potentially slow rotators|potentially slow rotator]].
=== Diameter and albedo ===
According to the survey carried out by the [[NEOWISE]] mission of NASA's [[Wide-field Infrared Survey Explorer]],
▲According to the survey carried out by the [[NEOWISE]] mission of NASA's [[Wide-field Infrared Survey Explorer]], ''Lidiya'' measures 6.388 and 7.189 kilometers in diameter and its surface has an [[astronomical albedo|albedo]] of 0.350 and 0.3776, respectively.<ref name="Masiero-2014" /><ref name="WISE" />
The ''Collaborative Asteroid Lightcurve Link'' assumes an albedo of 0.23 – derived from [[25 Phocaea]], the Phocaea family's largest member and namesake – and calculates a diameter of 7.99 kilometers based on an [[absolute magnitude]] of 12.7.<ref name="lcdb" />
== Naming ==
This [[minor planet]] was named after Russian aviator Lidiya Vissarionovna Zvereva (1890–1916), the first Russian female pilot, who began flying in 1911. She was also an instructor of other pilots and involved in the construction of airplanes.<ref name="springer" /> The official naming citation was published by the [[Minor Planet Center]] on 4 October 1990 ({{small|[[Minor Planet Circulars|M.P.C.]] 17027}}).<ref name="MPC-Circulars-Archive" /> The crater on Venus, ''[[List of craters on Venus#Zvereva|Zvereva]]'' was also named in her honor in 1985.{{efn|name="crater"}}
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|type = 2017-05-02 last obs.
|title = JPL Small-Body Database Browser: 3322 Lidiya (1975 XY1)
|url =
|publisher = [[Jet Propulsion Laboratory]]
|
<ref name="springer">{{cite book
|last = Schmadel | first = Lutz D.
|title = Dictionary of Minor Planet Names |publisher = [[Springer Berlin Heidelberg]]
|page = 277
|date = 2007
|isbn = 978-3-540-00238-3
|doi = 10.1007/978-3-540-29925-7_3323 |chapter = (3322) Lidiya }}</ref>
<ref name="MPC-object">{{cite web
|title = 3322 Lidiya (1975 XY1)
|work = Minor Planet Center
|url =
|
<ref name="MPC-Circulars-Archive">{{cite web
|title = MPC/MPO/MPS Archive
|work = Minor Planet Center
|url =
|
<ref name="Masiero-2014">{{cite journal
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|title = LCDB Data for (3322) Lidiya
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/
|
<ref name="WISE">{{cite journal
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|date = November 2011
|title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
|journal = The Astrophysical Journal
|volume = 741
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|bibcode = 2011ApJ...741...90M
|doi = 10.1088/0004-637X/741/2/90
|arxiv = 1109.6407}}</ref>
<ref name="Buchheim-2014">{{Cite journal
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<ref name="Ferret">{{cite web
|title =
|work =
|url = https://sbntools.psi.edu/ferret/
|
<ref name="Nesvorny-2014">{{Cite
|first1 = D. |last1 = Nesvorný
|first2 = M. |last2 = Broz
|first3 = V. |last3 = Carruba
|date = December 2014
|
▲ |journal = Asteroids IV
|pages = 297–321
|bibcode = 2015aste.book..297N
|doi = 10.2458/azu_uapress_9780816532131-ch016
|arxiv = 1502.01628
|
}} <!-- end of reflist -->
== External links ==
* [http://www.minorplanet.info/PHP/lcdbsummaryquery.php Asteroid Lightcurve Database (LCDB)], query form ([http://www.minorplanet.info/lightcurvedatabase.html info] {{Webarchive|url=https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html |date=16 December 2017 }})
* [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
* [http://obswww.unige.ch/~behrend/page_cou.html Asteroids and comets rotation curves, CdR] – Observatoire de Genève, Raoul Behrend
* [
* {{AstDys|3322}}
* {{JPL small body}}
{{Minor planets navigator |3321 Dasha |number=3322 |3323 Turgenev}}
{{Small Solar System bodies}}
{{Authority control}}
{{DEFAULTSORT:Lidiya}}
[[Category:Phocaea asteroids|003322]]
[[Category:Discoveries by Tamara Mikhaylovna Smirnova]]
[[Category:Named minor planets]]
[[Category:Astronomical objects discovered in 1975|19751201]]
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