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1573 Väisälä
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Asteroid
October 2019
yes
1573 Väisälä
#D6D6D6
27 October 1949
S. Arend
Uccle Obs.
(1573) Väisälä
1949 UA
Yrjö Väisälä (astronomer)
main-beltPhocaea
4 September 2017 (JD 2458000.5)
0
67.51 yr (24,659 days)
2.9192 AU
1.8243 AU
2.3717 AU
0.2308
3.65 yr (1,334 days)
225.00°
0.2698 ms / day
24.553°
202.38°
173.91°
8.43 1.90 km9.083 0.055 km9.146 0.066 km9.77 km (IRAS:2)
252 hLCDB-Pravec-2012
0.2226 (IRAS:2)0.25 0.120.2818 0.03190.284 0.045
S
12.212.3012.4712.84 0.50
1573 Väisälä, provisional designation 1949 UA, is a stony Phocaea asteroid, slow rotator and suspected tumbler from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 27 October 1949, by Belgian astronomer Sylvain Arend at the Royal Observatory of Belgium in Uccle, Belgium. It was named for Finnish astronomer Yrjö Väisälä.
Orbit and classification
The stony S-type asteroid is a member of the Phocaea family (701), a group of asteroids with similar orbital characteristics. It orbits the Sun at a distance of 1.8–2.9 AU once every 3 years and 8 months (1,334 days). Its orbit has an eccentricity of 0.23 and an inclination of 25° with respect to the ecliptic. Väisäläs observation arc begins on the night following its official discovery observation at Uccle, as no precoveries were taken and no prior identifications were made.
Physical characteristics
Slow rotator
In September 2011, a rotational lightcurve of Väisälä was obtained from photometric observations made by Czech astronomer Petr Pravec at Ondřejov Observatory.IMG-Light-Curve-Analysis Its analysis gave a rotation period of 252 hours with a brightness variation of 0.76 magnitude (U=2).LCDB-Pravec-2012 This makes Väisälä one of the Top 200 slow rotators known to exist. The body is also suspected to be in a non-principal axis rotation (NPAR), colloquially called as "tumbling". As of 2017, no follow-up observations have been made of these provisional results.
Diameter and albedo
According to the space-based surveys carried out by the Infrared Astronomical Satellite IRAS, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Väisälä measures between 8.43 and 9.77 kilometers in diameter, and its surface has an albedo between 0.222 and 0.284. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.2226 and a diameter of 9.77 kilometers using on an absolute magnitude of 12.30.
Naming
This minor planet was named after Finnish astronomer, Yrjö Väisälä (1891–1971), a prolific discoverer of minor planets during the late 1930s and early 1940s. In addition, a second minor planet, 2804 Yrjö, was named in his honor by pioneering Finnish female astronomer Liisi Oterma, and the lunar crater Väisälä also bears his name. The official 1573 naming citation was published by the Minor Planet Center on 31 January 1962 (M.P.C. 2116).
Notets
LCDB-Pravec-2012 Pravec (2012) web: rotation period 252 hours with a brightness amplitude of 0.76 mag. Pravec, P.; Wolf, M.; Sarounova, L. (2012) Summary figures at DEFPage_Local.php?AstInfo=1573%7CVaisala Collaborative Asteroid Lightcurve Link (CALL) for (1573) Vaisala
IMG-Light-Curve-Analysis Light-Curve-Analysis of (1573) Väisälä Screenshot from data
References
30em 2017-05-02 last obs.
JPL Small-Body Database Browser: 1573 Vaisala (1949 UA)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001573
Jet Propulsion Laboratory
5 June 2017
Dictionary of Minor Planet Names – (1573) Väisälä
Schmadel Lutz D.
Springer Berlin Heidelberg
125
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1574 (1573) Väisälä
1573 Vaisala (1949 UA)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1573
29 December 2016
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
2009
https://archive.org/details/dictionaryminorp2008schm
limited
Appendix – Publication Dates of the MPCs
Schmadel Lutz D.
Springer Berlin Heidelberg
221
978-3-642-01964-7
10.1007/978-3-642-01965-4 2009dmpn.book.....S
E. F. Tedesco
P. V. Noah
M. Noah
S. D. Price
October 2004
IRAS Minor Planet Survey V6.0
https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0
2004PDSS...12.....T
17 October 2019
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
J. Dailey
P. R. M. Eisenhardt
R. S. McMillan
T. B. Spahr
M. F. Skrutskie
D. Tholen
R. G. Walker
E. L. Wright
E. DeBaun
D. Elsbury
T. IV Gautier
S. Gomillion
A. Wilkins
November 2011
Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M
The Astrophysical Journal
741
2
20
2011ApJ...741...68M
10.1088/0004-637X/741/2/68
1109.4096
118745497 29 December 2016
6
Joseph R. Masiero
T. Grav
A. K. Mainzer
C. R. Nugent
J. M. Bauer
R. Stevenson
S. Sonnett
August 2014
Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
119293330 29 December 2016
Asteroid 1573 Vaisala – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1573+Vaisala#Asteroid%201573%20VaisalaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
26 October 2019 October 2026 InternetArchiveBot
1573
29 December 2016
6
A. Mainzer
T. Grav
J. Masiero
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
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407 35447010
6
C. R. Nugent
A. Mainzer
J. Bauer
R. M. Cutri
E. A. Kramer
T. Grav
J. Masiero
S. Sonnett
E. L. Wright
September 2016
NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos
The Astronomical Journal
152
3
12
2016AJ....152...63N
10.3847/0004-6256/152/3/63
1606.08923
free
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
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
November 2015
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V
Icarus
261
34–47
2015Icar..261...34V
10.1016/j.icarus.2015.08.007
1506.00762
53493339 29 December 2016
External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20241208174218/http://obswww.unige.ch/~behrend/page_cou.html 8 December 2024 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1573
1572 Posnania 1573 1574 Meyer
001573
Category:Discoveries by Sylvain Arend
Category:Named minor planets
001573
19491027