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(219774) 2001 YY145
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Main-belt asteroid
June 2018
yes
(219774) 2001 YY 145
#D6D6D6
18 December 2001
LONEOS
Anderson Mesa Stn.
(219774) 2001 YY 145
2005 TA 170
main-belt(middle)background
23 March 2018 (JD 2458200.5)
0
15.92 yr (5,815 d)
2.9215 AU
2.2404 AU
2.5810 AU
0.1320
4.15 yr (1,515 d)
48.043°
0.2377 ms / day
9.6001°
315.61°
18.718°
1.54 km (calculated)
1007.6706 86.3718 h
0.20 (assumed)
S (assumed)
15.915.977 0.011 (R)16.43
(219774) 2001 YY 145 is a stony background asteroid and exceptionally slow rotator from the central region of the asteroid belt, approximately 1.5 km mi off 1 us in diameter. It was discovered on 18 December 2001, by astronomers with the Lowell Observatory Near-Earth-Object Search at Anderson Mesa Station near Flagstaff, Arizona, in the United States. The assumed S-type asteroid is likely elongated and has a rarely seen rotation period of 1007 hours, making it the 13th slowest rotator.
Orbit and classification
2001 YY 145 is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 2.2–2.9 AU once every 4 years and 2 months (1,515 days; semi-major axis of 2.58 AU). Its orbit has an eccentricity of 0.13 and an inclination of 10° with respect to the ecliptic. A first precovery was taken at Lincoln Lab's ETS in October 2001, extending the asteroid's observation arc by 2 months prior to its official discovery observation at Anderson Mesa.
Physical characteristics
The object is an assumed, common S-type asteroid.
Slow rotator
In October 2013, a rotational lightcurve was obtained of this asteroid from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. It gave a rotation period of 1007.7 hours – or nearly 42 days – with an assigned error margin of ±86 hours. According to the Light Curve Data Base, it is the 13th slowest rotating minor planet known to exist among more than 15,000 observed small Solar System bodies. Due to its high brightness variation of 0.86 magnitude, the body is likely to have a non-spheroidal shape (U=2). As of 2018, no follow-up observation have been published.
Diameter and albedo
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.54 kilometers, based on an absolute magnitude of 16.43.
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 4 October 2009. As of 2018, it has not been named.
References
30em 2017-09-26 last obs.
JPL Small-Body Database Browser: 219774 (2001 YY145)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2219774
Jet Propulsion Laboratory
6 June 2018
219774 (2001 YY145)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=219774
6 June 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
24 February 2018
Asteroid (219774) – Proper elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?n=219774&pc=1.1.6
25 May 2018
Asteroid (219774) 2001 YY145
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=219774
6 June 2018
219774
13 September 2016
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 (215001)-(220000) – Minor Planet Center
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