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(164121) 2003 YT1
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Asteroid
April 2018
yes
(164121) 2003 YT 1
#FFC2E0
2003YT1.may4.mos.gif
Mosaic of radar images of 2003 YT 1 and its moon by Arecibo Observatory on 4 May 2004
Catalina Sky Srvy.
Catalina Stn.
18 December 2003
(164121) 2003 YT 1
ApolloNEOPHA
23 March 2018 (JD 2458200.5)
0
35.41 yr (12,934 d)
1.4335 AU
0.7857 AU
1.1096 AU
0.2919
1.17 yr (427 d)
11.417°
0.8433 ms / day
44.064°
38.335°
91.042°
0.0027 AU (1.0519 LD)
1 (D: 210 m; P: 30 h)
1.0 km1.100 0.088 km1.561 0.202 km1.717 0.550 km
2.34 h2.343 h2.343 h3.0025 0.0001 h
0.198 0.1530.240 0.0670.36 0.200.486 0.0400.4861 0.03950.5848 (derived)
V
16.216.20 0.3
(164121) 2003 YT 1 is a bright asteroid and synchronous binary system on a highly eccentric orbit, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 2 km mi off 2 us in diameter. It was discovered on 18 December 2003, by astronomers with the Catalina Sky Survey at the Catalina Station near Tucson, Arizona, in the United States. The V-type asteroid has a short rotation period of 2.3 hours. Its 210-meter sized minor-planet moon was discovered at Arecibo Observatory in May 2004.
Orbit and classification
2003 YT 1 is a member of the Earth-crossing group of Apollo asteroids, the largest group of near-Earth objects with approximately 10 thousand known members.
It orbits the Sun at a distance of 0.8–1.4 AU once every 1 years and 2 months (427 days; semi-major axis of 1.11 AU). Its orbit has an eccentricity of 0.29 and an inclination of 44° with respect to the ecliptic. The body's observation arc begins with a precovery taken at the Siding Spring Observatory in November 1989, more than 14 years prior to its official discovery observation at Catalina.
Close approaches and Torino rating
The asteroid has an Earth minimum orbital intersection distance of 0.0027 AU km mi on off 3, which corresponds to 1.05 lunar distances and makes it a potentially hazardous asteroid due to its sufficiently large size. On the Torino Scale, this object was rated level 1 on 27 December 2003 with an observation arc of 8.7 days. It was removed from the risk table on 29 December 2003. Over the next ten million years the asteroid has a 6% chance of impacting Earth.
On 30 April 2004 it made a close approach at a nominal distance of 0.073 AU LD on, and on 31 October 2016, it passed Earth at 0.035 AU LD on. The asteroid's closest encounter with Earth will be on 29 April 2073, when it is projected to pass at 0.0113 AU LD on only (see table).
2003 YT 1 has unique orbital characteristics among minor planets. It is the only known binary asteroid to have an Earth MOID within the Moon's Apogee.NASA.gov
+Earth Approach on 3 November 2023 Date JPL Horizonsnominal geocentricdistance (AU) uncertaintyregion(3-sigma)2023-Nov-03 12:33 0.05936 AU e6km unit on ±18 km
Meteor stream
On 28 April 2017, a 2.7 cm 1 fragment of 2013 YT 1 is suspected of having impacted Earth creating a fireball over Kyoto, Japan. The fragment would have broken off the parent body within the last ten thousand years.
Physical characteristics
thumb|left|Animation of Arecibo radar images showing 2003 YT 1's rotation and its satellite's orbital motion on 3 May 2004
This object has been characterized as a bright Vestian-like V-type asteroid.
Rotation period
Several rotational lightcurve of this asteroid have been obtained from photometric observations (U=2/n.a./3/3). Analysis of the best-rated lightcurve gave a short rotation period of 2.343 hours with a brightness amplitude between 0.16 and 0.27 magnitude.
Diameter and albedo
According to radar observations with the Arecibo Observatory and the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, this asteroid measures between 1.0 and 1.717 kilometers in diameter and its surface has an albedo between 0.198 and 0.4861.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.5848 and adopts a diameter of 1.0 kilometer based on an absolute magnitude of 16.2.
Satellite
The Arecibo radar observations in May 2004 revealed that 2003 YT 1 is a synchronous binary asteroid. Follow-up observations confirmed a 210-meter sized minor-planet moon orbiting its primary every 30 hours at a distance of 2.7 km.
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 26 September 2007 (M.P.C. 60686). As of 2018, it has not been named.
References
30em 2018-04-18 last obs.
JPL Small-Body Database Browser: 164121 (2003 YT1)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2164121
Jet Propulsion Laboratory
20 April 2018
164121 (2003 YT1)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=164121
20 April 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
20 April 2018
Asteroids and comets rotation curves – (164121)
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page5cou.html#0g4121
21 April 2018
https://web.archive.org/web/20181111134209/http://obswww.unige.ch/~behrend/page5cou.html#0g4121
11 November 2018
dead
6
A. Mainzer
T. Grav
J. Bauer
J. Masiero
R. S. McMillan
R. M. Cutri
R. Walker
E. Wright
P. Eisenhardt
D. J. Tholen
T. Spahr
R. Jedicke
L. Denneau
E. DeBaun
D. Elsbury
T. Gautier
S. Gomillion
E. Hand
W. Mo
J. Watkins
A. Wilkins
G. L. Bryngelson
A. Del Pino Molina
S. Desai
M. Gómez Camus
S. L. Hidalgo
I. Konstantopoulos
J. A. Larsen
C. Maleszewski
M. A. Malkan
J.-C. Mauduit
B. L. Mullan
E. W. Olszewski
J. Pforr
A. Saro
J. V. Scotti
L. H. Wasserman
December 2011
NEOWISE Observations of Near-Earth Objects: Preliminary Results
The Astrophysical Journal
743
2
17
2011ApJ...743..156M
10.1088/0004-637X/743/2/156
1109.6400 239991
Asteroids with Satellites Database – (164121) 2003 YT1
Johnston's Archive
20 September 2014
Johnston, Wm. Robert
http://www.johnstonsarchive.net/astro/astmoons/am-164121.html
20 April 2018
2003-12-27
Major News about Minor Objects (2003 YT1)
hohmanntransfer
http://www.hohmanntransfer.com/mn/0312/27.htm#risks
20 April 2018
25 April 2013
https://web.archive.org/web/20130425080914/http://www.hohmanntransfer.com/mn/0312/27.htm#risks
dead
NEOs Removed from Impact Risks Tables
Near Earth Object Program
NASA
http://neo.jpl.nasa.gov/risk/removed.html
https://web.archive.org/web/20020602101400/http://neo.jpl.nasa.gov/risk/removed.html
dead
2 June 2002
20 April 2018
164121
20 April 2018
M. C. Nolan
E. S. Howell Ellen Howell
A. A. Hine
May 2004
2003 YT_1
IAU Circ.
8336
3
2004IAUC.8336....3N
Marco Delbo
Kevin Walsh
Michael Mueller
Alan W. Harris
Ellen S. Howell Ellen Howell
March 2011
The cool surfaces of binary near-Earth asteroids
Icarus
212
1
138–148
2011Icar..212..138D
10.1016/j.icarus.2010.12.011
122586509
https://hal.archives-ouvertes.fr/hal-00725402/file/PEER_stage2_10.1016%252Fj.icarus.2010.12.011.pdf
6
A. Mainzer
T. Grav
J. Masiero
J. Bauer
R. M. Cutri
R. S. McMillan
C. R. Nugent
D. Tholen
R. Walker
E. L. Wright
November 2012
Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey
The Astrophysical Journal Letters
760
1
6
2012ApJ...760L..12M
10.1088/2041-8205/760/1/L12
1210.0502 41459166
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
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2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407 118700974
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S. M. Larson
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E. Beshore
E. Christensen
P. Pravec
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M. C. Nolan
E. S. Howell Ellen Howell
A. A. Hine
A. Galad
B. S. Gajdos
C. L. Kornos
D. J. Vilagi
November 2004
Physical Characteristics of the Binary PHA 2003 YT1
American Astronomical Society
36
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2004DPS....36.3207L
6
P. Pravec
P. Scheirich
P. Kusnirák
L. Sarounová
S. Mottola
G. Hahn
P. Brown
G. Esquerdo
N. Kaiser
Z. Krzeminski
D. P. Pray
B. D. Warner
A. W. Harris
M. C. Nolan
E. S. Howell Ellen Howell
L. A. M. Benner
J.-L. Margot
A. Galád
W. Holliday
M. D. Hicks
Yu. N. Krugly
D. Tholen
R. Whiteley
F. Marchis
D. R. DeGraff
A. Grauer
S. Larson
F. P. Velichko
W. R. Cooney
R. Stephens
J. Zhu
K. Kirsch
R. Dyvig
L. Snyder
V. Reddy
S. Moore
S. Gajdos
J. Világi
G. Masi
D. Higgins
G. Funkhouser
B. Knight
S. Slivan
R. Behrend
M. Grenon
G. Burki
R. Roy
C. Demeautis
D. Matter
N. Waelchli
Y. Revaz
A. Klotz
M. Rieugné
P. Thierry
V. Cotrez
L. Brunetto
G. Kober
March 2006
Photometric survey of binary near-Earth asteroids
Icarus
181
1
63–93
2006Icar..181...63P
10.1016/j.icarus.2005.10.014
Cristina A. Thomas
Joshua P. Emery
David E. Trilling
Marco Delbó
Joseph L. Hora
Michael Mueller
January 2014
Physical characterization of Warm Spitzer-observed near-Earth objects
Icarus
228
217–246
2014Icar..228..217T
10.1016/j.icarus.2013.10.004
1310.2000 119278697
Juan A. Sanchez
René Michelsen
Vishnu Reddy
Andreas Nathues
July 2013
Surface composition and taxonomic classification of a group of near-Earth and Mars-crossing asteroids
Icarus
225
1
131–140
2013Icar..225..131S
10.1016/j.icarus.2013.02.036
1302.4449 119207812
Kasuga Toshihiro
Sato Mikiya
Ueda Masayoshi
A Fireball and Potentially Hazardous Binary Near-Earth Asteroid (164121) 2003 YT1
The Astronomical Journal
2020
159
2
47
10.3847/1538-3881/ab4e1b
1910.06527 2020AJ....159...47K
204576074
free
Horizons Batch for 2023-11-03 Close Approach
JPL Horizons
https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%272003+YT1%27&START_TIME=%272023-11-03%2012:33%27&STOP_TIME=%272023-11-04%27&STEP_SIZE=%271%20day%27&QUANTITIES=%2720,39%27
https://web.archive.org/web/20221029143216/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%272003+YT1%27&START_TIME=%272023-11-03%2012:33%27&STOP_TIME=%272023-11-04%27&STEP_SIZE=%271%20day%27&QUANTITIES=%2720,39%27
2022-10-29
live
2022-10-29 RNG_3sigma = uncertainty range in km. (JPL#162/Soln.date: 2022-Oct-10 generates RNG_3sigma = 18 km)
External links
2003 YT1, IAUC 8336, 6 May 2004
List of the Potentially Hazardous Asteroids (PHAs), Minor Planet Center
Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
PHA Close Approaches To The Earth, Minor Planet Center
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
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
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