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14627 Emilkowalski
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Main-belt asteroid
October 2019
yes
14627 Emilkowalski
#D6D6D6
014627-asteroid shape model (14627) Emilkowalski.png
Emilkowalski modeled from its lightcurve
R. A. Kowalski
Quail Hollow Obs. 761
7 November 1998
(14627) Emilkowalski
1998 VA
Emil Kowalski(discoverer's family)
main-belt(middle)Emilkowalski24
4 September 2017 (JD 2458000.5)
0
62.93 yr (22,985 days)
2.9885 AU
2.2112 AU
2.5998 AU
0.1495
4.19 yr (1,531 days)
151.54°
0.2351 ms / day
17.751°
41.443°
44.474°
6.98 2.55 km7.105 0.106 km7.84 2.33 km10.61 km (calculated)
11.131 0.005 hlcdb-Pravec11.131 h
0.057 (assumed)0.09 0.100.120 0.1080.201 0.017
CDLS
13.113.38 (R)13.613.713.8514.19 0.75
14627 Emilkowalski (prov. designation: 1998 VA) is a stony asteroid from the central region of the asteroid belt, approximately 7 km mi off 2 us in diameter. It was discovered on 7 November 1998, by American astronomer Richard Kowalski at the Quail Hollow Observatory (761) in Zephyrhills, Florida, United States. The asteroid is the namesake of the recently formed Emilkowalski family of asteroids. It was named after Emil Kowalski, mentor of the discoverer.
Orbit and classification
Emilkowalski orbits the Sun in the central main-belt at a distance of 2.2–3.0 AU once every 4 years and 2 months (1,531 days). Its orbit has an eccentricity of 0.15 and an inclination of 18° with respect to the ecliptic.
The first unused observation at Palomar Observatory (DSS) dates back to 1953. The first used precovery was taken at Siding Spring Observatory in 1975, extending the asteroid's observation arc by 23 years prior to its discovery.
Emilkowalski family
Emilkowalski is the biggest member and namesake of a collisional group of asteroids, that resulted from the destruction of a larger parent body. The disruption happened approximately 220,000 years ago and it is one of the most recent asteroid breakups discovered in the main belt. The recently formed stony Emilkowalski family (family identification number: 523) consist of only 4 identified members.8,24 The other members are 126761 (126761) 2002 DW 10, 224559 (224559) 2005 WU 178 and 256124 (256124) 2006 UK 337.
Naming
This minor planet is named after American Emil Kowalski (1918–1994) from Syosset, New York, who inspired the discoverer of space science when he was still a child. The approved naming citation was published by the Minor Planet Center on 4 August 2001 (M.P.C. 43192).
Physical characteristics
Emilkowalski has been characterized as a rare DL-type by Pan-STARRS photometric survey. It has also been assigned a taxonomic type of a darker carbonaceous and a common stony asteroid, respectively.24
Rotation period
Between January and March 2012, photometric observations for this asteroid were made by a team led by Petr Pravec at Ondřejov Observatory, Czech Republic. The three obtained rotational lightcurves gave an identical period of 11.131 hours with a brightness variation of 0.55, 0.64 and 0.65 in magnitude, respectively (U=3/2+/3-).lcdb-Pravec Previously, in 2008, a lightcurve was obtained from observations at the Simeiz Observatory and the Chuguev Observing Station (121) in Ukraine, as well as at Maidanak Observatory in Uzbekistan. It also gave a period of 11.131 hours with an amplitude of 0.85 in magnitude, which implies an elongated shape (U=n.a.).
Diameter and albedo
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Emilkowalski measures between 6.98 and 7.84 kilometers in diameter and its surface has an albedo of 0.09 and 0.201.
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and hence calculates a larger diameter of 10.6 kilometers.
Notes
lcdb-Pravec Pravec (2012) web: 3 rotational light-curves constructed in January, February and March 2012, gave a rotation period 11.131 hours (for all three lightcurves) with a brightness amplitude of 0.55, 0.64 and 0.66 in magnitude, respectively. Summary figures for (14627) Emilkowalski at LCDB and at Ondrejov Asteroid Photometry Project
References
30em 2017-05-05 last obs.
JPL Small-Body Database Browser: 14627 Emilkowalski (1998 VA)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2014627
Jet Propulsion Laboratory
25 June 2017
Dictionary of Minor Planet Names
Schmadel Lutz D.
Springer Berlin Heidelberg
(14627) Emilkowalski
815
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_9030
14627 Emilkowalski (1998 VA)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=14627
6 April 2016
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
20 May 2016
D. Nesvorný
D. Vokrouhlický
November 2006
New Candidates for Recent Asteroid Breakups
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006AJ....132.1950N
The Astronomical Journal
132
5
1950–1958
2006AJ....132.1950N
10.1086/507989
6 April 2016
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
978-0-8165-3213-1
M. Broz
A. Morbidelli
W. F. Bottke
J. Rozehnal
D. Vokrouhlický
D. Nesvorný
March 2013
Constraining the cometary flux through the asteroid belt during the late heavy bombardment
Astronomy and Astrophysics
551
16
2013A&A...551A.117B
10.1051/0004-6361/201219296
1301.6221
Krugly
etal
May 2008
Photometry of asteroids: detection of the YORP effect
The Solar System Bodies: from Optics to Geology
http://www.astron.kharkov.ua/conference/ssb/08/index.php
Astronomical Institute of Kharkiv
Kharkiv, Ukraine
http://www.astron.kharkov.ua/conference/ssb/08/abstracts/SSB08-Krugly.pdf
7 December 2008
14627
25 June 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
20 May 2016
6
A. Mainzer
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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
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M
The Astrophysical Journal
741
2
25
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1109.6407
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6
Peter Veres
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Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
Christopher Waters
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Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
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1506.00762
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6
Joseph R. Masiero
A. K. Mainzer
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J. M. Bauer
R. M. Cutri
J. Dailey
P. R. M. Eisenhardt
R. S. McMillan
T. B. Spahr
M. F. Skrutskie
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E. DeBaun
D. Elsbury
T. IV Gautier
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C. R. Nugent
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free
External links
Maidanak astronomical observatory (MAO), of the Ulugh Beg Astronomical Institute (UBAI), Uzbekistan Academy of Sciences
Lightcurve Database Query (LCDB), at www.minorplanet.info
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 – Geneva Observatory, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
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Category:Discoveries by Richard Kowalski
Category:Named minor planets
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