(164121) 2003 YT1

(164121) 2003 YT1, provisional designation 2003 YT1, is a bright asteroid and synchronous binary system on a highly eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 2 kilometers (1.2 miles) 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.[1] The V-type asteroid has a short rotation period of 2.3 hours.[12] Its 210-meter sized minor-planet moon was discovered at Arecibo Observatory in May 2004.[3][4]

(164121) 2003 YT1
Discovery [1]
Discovered byCatalina Sky Srvy.
Discovery siteCatalina Stn.
Discovery date18 December 2003
Designations
(164121) 2003 YT1
2003 YT1
Apollo · NEO · PHA [1][2]
Orbital characteristics [2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc35.41 yr (12,934 d)
Aphelion1.4335 AU
Perihelion0.7857 AU
1.1096 AU
Eccentricity0.2919
1.17 yr (427 d)
11.417°
0° 50m 35.88s / day
Inclination44.064°
38.335°
91.042°
Known satellites1 (D: 210 m; P: 30 h)[3][4]
Earth MOID0.0027 AU (1.0519 LD)
Physical characteristics
Mean diameter
1.0 km[3]
1.100±0.088 km[5]
1.561±0.202 km[6]
1.717±0.550 km[7]
2.34 h[8]
2.343 h[3]
2.343 h[9]
3.0025±0.0001 h[10]
0.198±0.153[7]
0.240±0.067[6]
0.36±0.20[11]
0.486±0.040[11]
0.4861±0.0395[5]
0.5848 (derived)[12]
V [12][13][14]
16.2[2][5][12]
16.20±0.3[7]

    Orbit and classification

    2003 YT1 is a member of the Earth-crossing group of Apollo asteroids, the largest group of near-Earth objects with approximately 10 thousand known members.[1][2]

    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.[2] 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.[1]

    Close approaches and Torino rating

    The asteroid has an Earth minimum orbital intersection distance of 0.0027 AU (404,000 km; 251,000 mi), which corresponds to 1.05 lunar distances and makes it a potentially hazardous asteroid due to its sufficiently large size.[2] On the Torino Scale, this object was rated level 1 on 27 December 2003 with an observation arc of 8.7 days.[15] It was removed from the risk table on 29 December 2003.[16] Over the next ten million years the asteroid has a 6% chance of impacting Earth.[17]

    On 30 April 2004 it made a close approach at a nominal distance of 0.073 AU (28 LD), and on 31 October 2016, it passed Earth at 0.034 AU (13 LD). The asteroid's closest encounter with Earth will be on 29 April 2073, when it is projected to pass at 0.0113 AU (4.4 LD) only (see table).[2]

    History of close approaches of large near-Earth objects since 1908 (A)
    PHA Date Approach distance (lunar dist.) Abs.
    mag
    (H)    		 Diameter (C)
    (m)    		 Ref (D)
    Nomi-
    nal(B)    		 Mini-
    mum    		 Maxi-
    mum
    (33342) 1998 WT241908-12-163.5423.5373.54717.9556–1795data
    (458732) 2011 MD51918-09-170.9110.9090.91317.9556–1795data
    (7482) 1994 PC11933-01-172.9272.9272.92816.8749–1357data
    69230 Hermes1937-10-301.9261.9261.92717.5668–2158data
    69230 Hermes1942-04-261.6511.6511.65117.5668–2158data
    (137108) 1999 AN101946-08-072.4322.4292.43517.9556–1795data
    (33342) 1998 WT241956-12-163.5233.5233.52317.9556–1795data
    (163243) 2002 FB31961-04-124.9034.9004.90616.41669–1695data
    (192642) 1999 RD321969-08-273.6273.6253.63016.31161–3750data
    (143651) 2003 QO1041981-05-182.7612.7602.76116.01333–4306data
    2017 CH11992-06-054.6913.3916.03717.9556–1795data
    (170086) 2002 XR141995-06-244.2594.2594.26018.0531–1714data
    (33342) 1998 WT242001-12-164.8594.8594.85917.9556–1795data
    4179 Toutatis2004-09-294.0314.0314.03115.302440–2450data
    2014 JO252017-04-194.5734.5734.57317.8582–1879data
    (137108) 1999 AN102027-08-071.0141.0101.01917.9556–1795data
    (35396) 1997 XF112028-10-262.4172.4172.41816.9881–2845data
    (154276) 2002 SY502071-10-303.4153.4123.41817.6714–1406data
    (164121) 2003 YT12073-04-294.4094.4094.40916.21167–2267data
    (385343) 2002 LV2076-08-044.1844.1834.18516.61011–3266data
    (52768) 1998 OR22079-04-164.6114.6114.61215.81462–4721data
    (33342) 1998 WT242099-12-184.9194.9194.91917.9556–1795data
    (85182) 1991 AQ2130-01-274.1404.1394.14117.11100data
    314082 Dryope2186-07-163.7092.9964.78617.5668–2158data
    (137126) 1999 CF92192-08-214.9704.9674.97318.0531–1714data
    (290772) 2005 VC2198-05-051.9511.7912.13417.6638–2061data
    (A) List includes near-Earth approaches of less than 5 lunar distances (LD) of objects with H brighter than 18.
    (B) Nominal geocentric distance from the Earth's center to the object's center (earth radius≈6400 km).
    (C) Diameter: estimated, theoretical mean-diameter based on H and albedo range between X and Y.
    (D) Reference: data source from the JPL SBDB, with AU converted into LD (1 AU≈390 LD)
    (E) Color codes:   unobserved at close approach   observed during close approach   upcoming approaches

    Meteor stream

    On 28 April 2017, a 2.7 cm (1 in) fragment of 2013 YT1 is suspected of having impacted Earth creating a fireball over Kyoto, Japan.[17] The fragment would have broken off the parent body within the last ten thousand years.

    Physical characteristics

    This object has been characterized as a bright Vestian-like V-type asteroid.[12][14][13]

    Rotation period

    Several rotational lightcurve of this asteroid have been obtained from photometric observations (U=2/n.a./3/3).[8][3][9][10] 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.[12]

    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.[3][5][6][7][11][11]

    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.[12]

    Satellite

    The Arecibo radar observations in May 2004 revealed that 2003 YT1 is a synchronous binary asteroid.[3] Follow-up observations confirmed a 210-meter sized minor-planet moon orbiting its primary every 30 hours at a distance of 2.7 km.[4][9]

    Numbering and naming

    This minor planet was numbered by the Minor Planet Center on 26 September 2007 (M.P.C. 60686).[18] As of 2018, it has not been named.[1]

    References
    1. "164121 (2003 YT1)". Minor Planet Center. Retrieved 20 April 2018.
    2. "JPL Small-Body Database Browser: 164121 (2003 YT1)" (2018-04-18 last obs.). Jet Propulsion Laboratory. Retrieved 20 April 2018.
    3. Nolan, M. C.; Howell, E. S.; Hine, A. A. (May 2004). "2003 YT_1". IAU Circ. 8336 (8336): 3. Bibcode:2004IAUC.8336....3N.
    4. Johnston, Wm. Robert (20 September 2014). "Asteroids with Satellites Database – (164121) 2003 YT1". Johnston's Archive. Retrieved 20 April 2018.
    5. Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90.
    6. Delbo, Marco; Walsh, Kevin; Mueller, Michael; Harris, Alan W.; Howell, Ellen S. (March 2011). "The cool surfaces of binary near-Earth asteroids" (PDF). Icarus. 212 (1): 138–148. Bibcode:2011Icar..212..138D. doi:10.1016/j.icarus.2010.12.011.
    7. Mainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; Cutri, R. M.; McMillan, R. S.; et al. (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. arXiv:1210.0502. Bibcode:2012ApJ...760L..12M. doi:10.1088/2041-8205/760/1/L12.
    8. Larson, S. M.; Grauer, A. D.; Beshore, E.; Christensen, E.; Pravec, P.; Kaasalainen, M.; et al. (November 2004). "Physical Characteristics of the Binary PHA 2003 YT1". American Astronomical Society. 36: 1139. Bibcode:2004DPS....36.3207L.
    9. Pravec, P.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Mottola, S.; Hahn, G.; et al. (March 2006). "Photometric survey of binary near-Earth asteroids". Icarus. 181 (1): 63–93. Bibcode:2006Icar..181...63P. doi:10.1016/j.icarus.2005.10.014.
    10. Behrend, Raoul. "Asteroids and comets rotation curves – (164121)". Geneva Observatory. Retrieved 21 April 2018.
    11. Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results". The Astrophysical Journal. 743 (2): 17. arXiv:1109.6400. Bibcode:2011ApJ...743..156M. doi:10.1088/0004-637X/743/2/156.
    12. "LCDB Data for (164121)". Asteroid Lightcurve Database (LCDB). Retrieved 20 April 2018.
    13. Sanchez, Juan A.; Michelsen, René; Reddy, Vishnu; Nathues, Andreas (July 2013). "Surface composition and taxonomic classification of a group of near-Earth and Mars-crossing asteroids". Icarus. 225 (1): 131–140. arXiv:1302.4449. Bibcode:2013Icar..225..131S. doi:10.1016/j.icarus.2013.02.036.
    14. Thomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014). "Physical characterization of Warm Spitzer-observed near-Earth objects". Icarus. 228: 217–246. arXiv:1310.2000. Bibcode:2014Icar..228..217T. doi:10.1016/j.icarus.2013.10.004.
    15. "Major News about Minor Objects (2003 YT1)". hohmanntransfer. 27 December 2003. Retrieved 20 April 2018.
    16. "NEOs Removed from Impact Risks Tables". Near Earth Object Program. NASA. Retrieved 20 April 2018.
    17. Kasuga, Toshihiro; Sato, Mikiya; Ueda, Masayoshi (2019). "A Fireball and Potentially Hazardous Binary Near-Earth Asteroid (164121) 2003 YT". arXiv:1910.06527.
    18. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 20 April 2018.

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