411 REFERENCE · Wikipedia
1764 Cogshall
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Carbonaceous Themistian asteroid
October 2019
yes
1764 Cogshall
#D6D6D6
Indiana University(Indiana Asteroid Program)
Goethe Link Obs.
7 November 1953
(1764) Cogshall
1953 VM 11935 MF1939 CC1942 VB1951 LC1952 SM1953 XJ1964 XG1967 GO1969 TN 2
Wilbur A. Cogshall(professor of astronomy at IU)
main-belt(outer)Themis
4 September 2017 (JD 2458000.5)
0
82.02 yr (29,956 days)
3.4671 AU
2.7193 AU
3.0932 AU
0.1209
5.44 yr (1,987 days)
84.951°
0.1812 ms / day
2.2355°
152.23°
79.719°
25.14 0.64 km26.13 km (derived)26.21 2.0 km26.970 0.232 km29.671 0.179 km
3.624 0.0052 h (R)3.62417 0.00007 h3.630 0.0052 h (S)
0.0606 0.00860.0712 (derived)0.0852 0.0150.094 0.0050.109 0.010
S/C (generically assumed)
11.2011.248 0.002 (R)11.311.4
1764 Cogshall, provisional designation 1953 VM 1, is a carbonaceous Themistian asteroid from the outer regions of the asteroid belt, approximately 26 kilometers in diameter. It was discovered on 7 November 1953 by astronomers of the Indiana Asteroid Program at Goethe Link Observatory in Indiana, United States. The asteroid was named after Wilbur Cogshall, professor of astronomy at Indiana University.
Orbit and classification
Cogshall is a Themistian asteroid that belongs to the Themis family (602), a very large family of carbonaceous asteroids named after 24 Themis.23 It orbits the Sun in the outer main belt at a distance of 2.7–3.5 AU once every 5 years and 5 months (1,987 days). Its orbit has an eccentricity of 0.12 and an inclination of 2° concerning to the ecliptic.
The asteroid was first identified as 1935 MF at Johannesburg Observatory in June 1935. The body's observation arc begins with its identification as 1939 CC at Turku Observatory in February 1939, more than 14 years before its official discovery observation at Goethe Link.
Physical characteristics
Rotation period
In May 2005, French amateur astronomer Pierre Antonini obtained a rotational lightcurve of Cogshall from photometric observations. Lightcurve analysis gave a well-defined rotation period of 3.62417 hours with a brightness variation of 0.21 magnitude (U=3).
Observations at the Palomar Transient Factory in 2012 gave a concurring period of 3.624 and 3.630 hours with an amplitude of 0.22 and 0.20 magnitude in the R- and S-band, respectively (U=2/2).
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, Cogshall measures between 25.14 and 29.671 kilometers in diameter, and its surface has an albedo between 0.0606 and 0.109.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0712 and a diameter of 26.13 kilometers based on an absolute magnitude of 11.4.
Naming
This minor planet was named after American astronomer Wilbur A. Cogshall, a professor of astronomy at Indiana University and director of the Kirkwood Observatory for more than four decades (1900–1944). His research included visual binary stars and the photography of solar eclipses. The name was proposed by Frank K. Edmondson, who initiated the Indiana Asteroid Program. The Minor Planet Center published the official 1764 naming citation on 20 February 1971 (M.P.C. 3143).
References
30em 2017-07-05 last obs.
JPL Small-Body Database Browser: 1764 Cogshall (1953 VM1)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001764
Jet Propulsion Laboratory
6 September 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
141
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1765 (1764) Cogshall
Farseeing and Abiding at IU
Lauren J. Bryant
Indiana University
http://www.indiana.edu/~rcapub/v27n1/farseeing.shtml
6 September 2017
1764 Cogshall (1953 VM1)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1764
6 September 2017
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
Asteroids and comets rotation curves – (1764) Cogshall
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001764
6 September 2017
1 April 2019
https://web.archive.org/web/20190401181659/http://obswww.unige.ch/~behrend/page4cou.html#001764
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
1764
6 September 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
(online, AcuA catalog p. 153)
E. F. Tedesco
P. V. Noah
M. Noah
S. D. Price
October 2004
IRAS Minor Planet Survey V6.0
NASA Planetary Data System
2004PDSS...12.....T
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
6
Adam Waszczak
Chan-Kao Chang
Eran O. Ofek
Russ Laher
Frank Masci
David Levitan
Jason Surace
Yu-Chi Cheng
Wing-Huen Ip
Daisuke Kinoshita
George Helou
Thomas A. Prince
Shrinivas Kulkarni
September 2015
Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
The Astronomical Journal
150
3
35
2015AJ....150...75W
10.1088/0004-6256/150/3/75
1504.04041
Asteroid 1764 Cogshall – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1764+Cogshall#Asteroid%201764%20CogshallEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
31 October 2019
https://web.archive.org/web/20201107221807/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1764+Cogshall#Asteroid%201764%20CogshallEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
7 November 2020
dead
Asteroid 1764 Cogshall – Proper Elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1764
31 October 2019
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
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
1764
1763 Williams 1764 1765 Wrubel
001764
001764
Category:Named minor planets
19531107