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1330 Spiridonia
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Dark background asteroid of primitive composition
October 2019
yes
1330 Spiridonia
#D6D6D6
V. Albitzkij
Simeiz Obs.
17 February 1925
(1330) Spiridonia
1925 DB1931 FA1933 QK 11942 ED1950 OP1959 EZA922 SA
Spiridon Zaslavskij(discoverer's brother-in-law)
main-belt(outer)background
4 September 2017 (JD 2458000.5)
0
95.12 yr (34,741 days)
3.4092 AU
2.9306 AU
3.1699 AU
0.0755
5.64 yr (2,061 days)
104.05°
0.1746 ms / day
15.957°
158.82°
4.4832°
50.73 15.63 km51.96 16.95 km55.08 4.9 km55.17 km (derived)68.417 0.584 km69.917 1.110 km73.75 1.44 km78.496 27.90 km
9.626 0.002 h9.67 0.01 h10.3 0.03 h10.3 0.3 h10.302 0.001 h
0.029 0.0010.0297 0.01770.0309 0.00510.032 0.0040.0498 0.0100.0580 (derived)0.06 0.040.06 0.05
Tholen PB–V 0.670U–B 0.170
10.0010.0310.1710.26 0.10
1330 Spiridonia, provisional designation 1925 DB, is a dark background asteroid of primitive composition, located in the outer regions of the asteroid belt, approximately 65 kilometers in diameter. It was discovered on 17 February 1925, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after the discoverer's brother-in-law, Spiridon Zaslavskij.
Orbit and classification
Spiridonia is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.4 AU once every 5 years and 8 months (2,061 days; semi-major axis of 3.17 AU). Its orbit has an eccentricity of 0.08 and an inclination of 16° with respect to the ecliptic.
The asteroid was first identified as A922 SA at Heidelberg Observatory in September 1922. The body's observation arc begins at Yerkes Observatory in October 1934, more than 9 years after its official discovery observation at Simeiz.
Physical characteristics
In the Tholen classification, Spiridonia is a primitive P-type asteroid.
Rotation period
Several rotational lightcurves of Spiridonia have been obtained from photometric observations since 2004. Analysis of the best-rated lightcurve by American photometrist Robert Stephens at the Santana Observatory (646) from April 2005, gave a rotation period of 9.67 hours with a brightness amplitude of 0.16 magnitude (U=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, Spiridonia measures between 50.73 and 78.496 kilometers in diameter and its surface has an albedo between 0.029 and 0.06.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0580 and a diameter of 55.17 kilometers based on an absolute magnitude of 10.0.
1330 Spiridonia has been observed to occult 5 stars between 1993 and 2023.
Naming
This minor planet was named after the discoverer's brother-in-law, Spiridon Zaslavskij (1883–1942), who was also the uncle of Viktorovich Zaslavskij (1925–1944), after whom the discoverer named the asteroid 1030 Vitja. The official 1330 naming citation was published by the Minor Planet Center on 15 July 1968 (M.P.C. 2882).
References
30em 2017-11-02 last obs.
JPL Small-Body Database Browser: 1330 Spiridonia (1925 DB)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001330
Jet Propulsion Laboratory
29 November 2017
Dictionary of Minor Planet Names – (1330) Spiridonia
Schmadel Lutz D.
Springer Berlin Heidelberg
108
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1331 (1330) Spiridonia
1330 Spiridonia (1925 DB)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1330
29 November 2017
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
Appendix – Publication Dates of the MPCs
Schmadel Lutz D.
2009
Springer Berlin Heidelberg
221
978-3-642-01964-7
10.1007/978-3-642-01965-4 2009dmpn.book.....S
Asteroids and comets rotation curves – (1330) Spiridonia
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001330
29 November 2017
3 August 2003
https://web.archive.org/web/20030803183423/http://obswww.unige.ch/~behrend/page4cou.html#001330
dead
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
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645 119293330
Asteroid 1330 Spiridonia – Proper Elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1330
29 October 2019
1330
29 November 2017
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
Fumihiko Usui
Daisuke Kuroda
Thomas G. Müller
Sunao Hasegawa
Masateru Ishiguro
Takafumi Ootsubo
Daisuke Ishihara
Hirokazu Kataza
Satoshi Takita
Shinki Oyabu
Munetaka Ueno
Hideo Matsuhara
Takashi Onaka
October 2011
Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
Publications of the Astronomical Society of Japan
63
5
1117–1138
2011PASJ...63.1117U
10.1093/pasj/63.5.1117
free
(online, AcuA catalog p. 153)
E. F. Tedesco
P. V. Noah
M. Noah
S. D. Price
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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
C. Nugent
A. K. Mainzer
E. L. Wright
J. M. Bauer
R. M. Cutri
T. Grav
E. Kramer
S. Sonnett
October 2017
NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos
The Astronomical Journal
154
4
10
2017AJ....154..168M
10.3847/1538-3881/aa89ec
1708.09504 free
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
C. R. Nugent
A. Mainzer
J. Masiero
J. Bauer
R. M. Cutri
T. Grav
E. Kramer
S. Sonnett
R. Stevenson
E. L. Wright
December 2015
NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N
The Astrophysical Journal
814
2
13
2015ApJ...814..117N
10.1088/0004-637X/814/2/117
1509.02522
9341381 29 November 2017
Stephens, Robert D.
January 2013
Asteroids Observed from Santana and CS3 Observatories: 2012 July - September
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013MPBu...40...34S
The Minor Planet Bulletin
40
1
34–35
1052-8091
2013MPBu...40...34S
29 November 2017
Stephens, Robert D.
September 2005
Asteroid lightcurve photometry from Santana Observatory - winter 2005
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005MPBu...32...66S
The Minor Planet Bulletin
32
3
66–68
1052-8091
2005MPBu...32...66S
29 November 2017
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
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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
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261
34–47
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1506.00762
53493339 29 November 2017
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/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1330
1329 Eliane 1330 1331 Solvejg
001330
Category:Discoveries by Vladimir Albitsky
Category:Named minor planets
001330
19250217