411 REFERENCE · Wikipedia
14789 GAISH
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Asteroid discovered in 1969
May 2018
yes
14789 GAISh
#D6D6D6
L. Chernykh
Crimean Astrophysical Obs.
8 October 1969
(14789) GAISH
1969 TY 11995 KQ 21996 QW 21999 CH 69
Sternberg Astronomical Institute (GAISh)(Moscow State University)
main-belt(outer)background
23 March 2018 (JD 2458200.5)
0
47.65 yr (17,405 d)
3.4121 AU
2.8333 AU
3.1227 AU
0.0927
5.52 yr (2,016 d)
301.75°
0.1786 ms / day
5.8175°
200.22°
161.64°
11.42 km (calculated)15.256 0.211 km
8.086 0.0032 h
0.057 (assumed)0.076 0.017
C (assumed)
12.512.812.990 0.008 (R)13.44
14789 GAISh, provisional designation 1969 TY 1, is a dark background asteroid from the outer regions of the asteroid belt, approximately 15 km mi off 1 us in diameter. It was discovered on 8 October 1969, by Soviet astronomer Lyudmila Chernykh of the Crimean Astrophysical Observatory at Nauchnij, on the Crimean peninsula. The assumed C-type asteroid has a rotation period of 8.1 hours and possibly an elongated shape. It was named for the Russian Sternberg Astronomical Institute (GAISh) of Moscow State University.
Orbit and classification
GAISh 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 2.8–3.4 AU once every 5 years and 6 months (2,016 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.09 and an inclination of 6° with respect to the ecliptic. The body's observation arc begins with its official discovery observation in October 1969.
Physical characteristics
GAISh is an assumed carbonaceous C-type asteroid.
Rotation period
In October 2010, a rotational lightcurve of GAISh was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 8.086 hours with a high brightness amplitude of 0.82 magnitude, indicative of a non-spherical shape (U=2).
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, GAISh measures 15.256 kilometers in diameter and its surface has an albedo of 0.076. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 11.42 kilometers based on an absolute magnitude of 13.44.
Naming
This minor planet was named after the Sternberg Astronomical Institute (GAISh, ГАИШ), a division of Moscow State University. Founded in 1931, it is one of Russia's leading astronomical institute and a principal educational facility for professional astronomers. The institute is located on the site of the 1931-built Sternberg Observatory. The official naming citation was published by the Minor Planet Center on 6 January 2007 (M.P.C. 58595).
References
30em 2017-06-03 last obs.
JPL Small-Body Database Browser: 14789 GAISH (1969 TY1)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2014789
Jet Propulsion Laboratory
14 May 2018
14789 GAISH (1969 TY1)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=14789
14 May 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
14 May 2018
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
The Astrophysical Journal
741
2
20
2011ApJ...741...68M
10.1088/0004-637X/741/2/68
1109.4096
118745497
Asteroid 14789 GAISH – Proper Elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=14789
29 October 2019
14789
14 May 2018
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 (catalog)
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
8342929
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
Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
14789
14789 14790 Beletskij
014789
Category:Discoveries by Lyudmila Chernykh
Category:Named minor planets
19691008