411 REFERENCE · Wikipedia
1364 Safara
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Main-belt asteroid
October 2019
yes
1364 Safara
#D6D6D6
001364-asteroid shape model (1364) Safara.png
Modelled shape of Safara from its lightcurve
L. Boyer
Algiers Obs.
18 November 1935
(1364) Safara
1935 VB1932 EK
André Safar(discoverer's acquaintance)
main-belt(outer)Eos
4 September 2017 (JD 2458000.5)
0
85.64 yr (31,279 days)
3.2114 AU
2.8133 AU
3.0124 AU
0.0661
5.23 yr (1,910 days)
8.7502°
0.1885 ms / day
11.488°
63.986°
220.38°
21.197 0.201 km21.508 0.266 km24.35 0.47 km25.73 km (calculated)32.63 0.46 km
7.14908 0.0004 h7.25 0.05 hlightcurveplot-PDO
0.087 0.0120.14 (assumed)0.173 0.0070.2231 0.0149
LS (assumed)
10.6010.64 0.1910.70
1364 Safara, incorrectly designated 1935 VB, is an Eoan asteroid from the outer regions of the asteroid belt, approximately 25 kilometers in diameter. It was discovered on 18 November 1935, by French astronomer Louis Boyer at the Algiers Observatory in Algeria, North Africa. The asteroid should have been designated 1935 WB, as the letter "V" only covers discoveries made during 1–15 November. It was named after André Safar, presumably an acquaintance of the discoverer from Algiers.
Orbit and classification
Safara is a member the Eos family (606), the largest asteroid family of the outer main belt consisting of nearly 10,000 asteroids.23 It orbits the Sun at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,910 days; semi-major axis of 3.01 AU). Its orbit has an eccentricity of 0.07 and an inclination of 11° with respect to the ecliptic.
The asteroid was first identified as 1932 EK at Heidelberg Observatory in March 1932. The body's observation arc begins at Algiers with its official discovery observation in November 1935.
Physical characteristics
The Collaborative Asteroid Lightcurve Link (CALL) assumes Safara to be a stony S-type asteroid, while it has also characterized as a rare L-type asteroid by Pan-STARRS photometric survey. The overall spectral type of the Eos family is that of a K-type.23
Rotation period and poles
In February 2002, a rotational lightcurve of Safara was obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave a rotation period of 7.25 hours with a brightness amplitude of 0.36 magnitude (U=3-).lightcurveplot-PDO
In 2018, the body's lightcurve has also been modeled in a focused study of Eoan asteroids. Modeling gave a period of 7.14908 hours and two spin axis in ecliptic coordinates (λ, β) of (197.0°, 32.0°) and (10.0°, 12.0°).
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Safara measures between 21.197 and 32.63 kilometers in diameter and its surface has an albedo between 0.087 and 0.2231.
CALL assumes an albedo of 0.14 – derived from 221 Eos, the family's largest member and namesake – and calculates a diameter of 25.73 kilometers based on an absolute magnitude of 10.7.
Naming
This minor planet was named after André Safar, presumably an acquaintance of the discoverer from Algiers. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 124).
Notes
lightcurveplot-PDO Lightcurve plot of 1364 Safara, Palmer Divide Observatory, Brian D. Warner (2010) Summary figures at the LCDB
References
30em 2017-10-29 last obs.
JPL Small-Body Database Browser: 1364 Safara (1935 VB)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001364
Jet Propulsion Laboratory
15 November 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
111
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1365 (1364) Safara
1364 Safara (1935 VB)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1364
15 November 2017
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
15 November 2017
Asteroid 1364 Safara – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1364+Safara#Asteroid%201364%20SafaraEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
26 October 2019 October 2026 InternetArchiveBot
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
9780816532131
1364
15 November 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
15 November 2017
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)
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
Warner, Brian D.
July 2010
Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 December - 2010 March
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37..112W
The Minor Planet Bulletin
37
3
112–118
1052-8091
2010MPBu...37..112W
15 November 2017
6
J. Hanus
M. Delbo'
V. Alí-Lagoa
B. Bolin
R. Jedicke
J. Durech
H. Cibulková
P. Pravec
P. Kusnirák
R. Behrend
F. Marchis
P. Antonini
L. Arnold
M. Audejean
M. Bachschmidt
L. Bernasconi
L. Brunetto
S. Casulli
R. Dymock
N. Esseiva
M. Esteban
O. Gerteis
H. de Groot
H. Gully
Hiroko Hamanowa
Hiromi Hamanowa
P. Krafft
M. Lehký
F. Manzini
J. Michelet
E. Morelle
J. Oey
F. Pilcher
F. Reignier
R. Roy
P. A. Salom
B. D. Warner
January 2018
Spin states of asteroids in the Eos collisional family
Icarus
299
84–96
2018Icar..299...84H
10.1016/j.icarus.2017.07.007
1707.05507
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
15 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
1364
1363 Herberta 1364 1365 Henyey
001364
Category:Discoveries by Louis Boyer (astronomer)
Category:Named minor planets
001364
19351118