Rotation Period,14.22,h,[5]
Quality,3,-,[5]
Amplitude,0.68,mag,[5]
Rotation Direction,-,-,[-]
Spinvector L,-,deg,[-]
Spinvector B,-,deg,[-]
Taxonomy,S,-,[1]
Taxonomy,Q,-,[2]
Taxonomy (all),-,-,[3]
Taxonomy (all),Q,R;S,-,[4]
Absolute Magnitude (H),14.986,mag,[6]
Absolute Magnitude (H),15.1,mag,[5]
Slope Parameter (G),0.15**,-,[6]
Albedo,0.228,-,[7]
Albedo,0.52,-,[8]
Diameter,2730,m,[7]
Diameter,2800,m,[8]
Color Index Information,-,mag,[-]
Sightings,Visual S,-,[9]
Sightings,Radar R,-,[10]

REFERENCES

[1],EARN,1.) Michaël Marsset et al 2022 AJ 163 165
[2],EARN,1.) Whiteley, R.J. (2001) PhD. Thesis, University of Hawaii. (A Compositional and Dynamical Survey of the Near-Earth Asteroids)
[3],EARN,Earth Asteroids Research Node: https://earn.dlr.de
[4],EARN,1.) Hicks, M.D. et al. (1998) Icarus 133, 69-78. (The Unusual Spectra of 15 Near-Earth Asteroids and Extinct Comet Candidates)(1566,1620,2063,2102,2201,3200,4953,6053,6489,7092,8176,1994ES1,1995CR,1996JA1) 2.) Whiteley, R.J. (2001) PhD. Thesis, University of Hawaii. (A Compositional and Dynamical Survey of the Near-Earth Asteroids)
[5],EARN,1.) Mottola, S. et al. (1995) Icarus 117, 62-70. (The near-earth objects follow-up program: First results.)(1981,2062,4953,5633,5797,5836,1993BX3,1994AW1,1994JF1,1994LC1) 2.) Erikson, A. et al. (2000) Icarus 147, 487-497. (The Near-Earth Objects Follow-Up Program III: 32 Lightcurves for 12 Objects from 1992 to 1995) (433,1917,2368,3753,4769,4953,6491, 1995 EK1, 1995 FJ; 5738,7467,1995 LH)
[6],ESA Aegis,ESA orbit determination and impact monitoring system
[7],EARN,1.) Joseph R. Masiero et al 2021 Planet. Sci. J. 2 162
[8],EARN,1.) Harris(DLR), A.W. et al. (2011) Astron. J. 141, 75. (ExploreNEOs. II. THE ACCURACY OF THE WARM SPITZER NEAR-EARTH OBJECT SURVEY) 2.) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 255-271. (Physical Properties of NEOs) 3.) Trilling, D.E. et al. (2010) Astron. J. 140, 770-784. (EXPLORENEOs. I. DESCRIPTION AND FIRST RESULTS FROM THE WARM SPITZER NEAR-EARTH OBJECT SURVEY) (diameters & albedos for 101 NEOs)
[9],EARN,1.) Hicks, M.D. et al. (1998) Icarus 133, 69-78. (The Unusual Spectra of 15 Near-Earth Asteroids and Extinct Comet Candidates)(1566,1620,2063,2102,2201,3200,4953,6053,6489,7092,8176,1994ES1,1995CR,1996JA1) 2.) Fevig. R.A. and U. Fink (2007) Icarus 188, 175-188. (Spectral observations of 19 weathered and 23 fresh NEAs and their correlations with orbital parameters)(433,1036,1627,1685,1862,1866,1943,1980,3103,3122,3199,3671,4183,4341,4954,5587,5751,5836,6037,7358,7482,7753,7822,7977,8201,10563,11066,13651,13651,19356,20236,20255,35107,85490,J97GD32,J97UH9,J97US9,J98HE3,J98HT31,J98ME3,J98MS2,K04LC2)
[10],EARN,1.) <a href="http://echo.jpl.nasa.gov/asteroids/index.html">JPL's NEO Radar Detection Program Webpage</A> 2.) Taylor, P.A. et al. (2012) CBET <A HREF="http://www.cbat.eps.harvard.edu/iau/cbet/003100/CBET003176.txt"><B> 3176.</B></A> ((5143) HERACLES) (Radar binary detection)