List of exceptional asteroids - wikipedia List of exceptional asteroids Ceres is the largest and most massive asteroid and the only one that is a dwarf planet. Vesta is the brightest and second-most - massive asteroid. It suffered a crust - penetrating impact approximately one billion years ago. The following is a collection of lists of exceptional asteroids in the Solar System. For the purposes of this article `` asteroid '' means minor planet up to the orbit of Jupiter, which includes the dwarf planet Ceres. For a complete list of minor planets in numerical order, see List of minor planets. Asteroids are given a unique sequential identifying number once their orbit is precisely determined. Prior to this, they are known only by their systematic name or provisional designation, such as 1950 DA. Contents 1 Physical characteristics 1.1 Largest by diameter 1.2 Most massive 1.3 Brightest from Earth 1.4 Slowest rotators 1.5 Fastest rotators 2 Orbital characteristics 2.1 Retrograde 2.2 Highly inclined 2.3 Trojans 2.4 Record - setting close approaches to Earth 3 Timeline 3.1 Landmark asteroids 3.2 Spacecraft targets 3.3 Numbered minor planets that are also comets 3.4 Minor planets that were misnamed and renamed 4 See also 5 Books 6 References 7 External links Physical characteristics Largest by diameter Estimating the sizes of asteroids from observations is difficult due to their irregular shapes, varying albedo, and small angular diameter. For example, pure C - type asteroids are much darker than most. Asteroids with only one or two axes measured may have a falsely inflated geometric mean diameter if the unknown second or third axis is significantly smaller than the primary axis. Asteroid 16 Psyche has an IRAS diameter of 253 km, yet has a more recent and accurate geometric mean of only 186 km. Name Diameter ( km ) ( geometric mean ) Dimensions ( km ) Mean distance from Sun ( in AU ) Date discovered Discoverer Class 1 Ceres 7002946000000000000 ♠ 946 ± 2 965 × 962 × 891 2.766 January 1, 1801 Piazzi, G. 4 Vesta 7002525400000000000 ♠ 525.4 ± 0.2 572.6 × 557.2 × 446.4 ± 0.2 2.362 March 29, 1807 Olbers, H.W. V 2 Pallas 7002512000000000000 ♠ 512 ± 3 7002550000000000000 ♠ 550 ± 4 × 7002516000000000000 ♠ 516 ± 3 × 7005476000000000000 ♠ 476 ± 3 km 2.773 March 28, 1802 Olbers, H.W. 10 Hygiea 7002431000000000000 ♠ 431 ± 7 530 × 407 × 370 3.139 April 12, 1849 de Gasparis, A. 704 Interamnia 326 350 × 304 3.062 October 2, 1910 Cerulli, V. 52 Europa 315 380 × 330 × 250 3.095 February 4, 1858 Goldschmidt, H. 511 Davida 289 357 × 294 × 231 3.168 May 30, 1903 Dugan, R.S. 87 Sylvia 286 385 × 265 × 230 3.485 May 16, 1866 Pogson, N.R. X 65 Cybele 273 302 × 290 × 232 3.439 March 8, 1861 Tempel, E.W. 15 Eunomia 268 357 × 255 × 212 2.643 July 29, 1851 de Gasparis, A. 3 Juno 258 320 × 267 × 200 2.672 September 1, 1804 Harding, K.L. 31 Euphrosyne 256 255.9 ± 5.8 km 3.149 September 1, 1854 Ferguson, J. 624 Hektor 241 370 × 195 ( × 195 ) 5.235 February 10, 1907 Kopff, A. 88 Thisbe 232 221 × 201 × 168 2.769 June 15, 1866 Peters, C.H.F. 324 Bamberga 229 229 × 235 × 229 2.684 February 25, 1892 Palisa, J. 451 Patientia 225 225 × 234 3.059 December 4, 1899 Charlois, A. 532 Herculina 222 260 × 220 × 215 2.772 April 20, 1904 Wolf, M. 48 Doris 222 278 × 142 3.108 September 19, 1857 Goldschmidt, H. 375 Ursula 216 189 × 192 × 194 3.126 September 18, 1893 Charlois, A. 107 Camilla 215 285 × 205 × 170 3.476 November 17, 1868 Pogson, N.R. 45 Eugenia 213 305 × 220 × 145 2.720 June 27, 1857 Goldschmidt, H. 7 Iris 213 240 × 200 × 200 2.386 August 13, 1847 Hind, J.R. 29 Amphitrite 212 233 × 212 × 193 2.554 March 1, 1854 Marth, A. 423 Diotima 209 171 × 138 3.065 December 7, 1896 Charlois, A. 19 Fortuna 208 225 × 205 × 195 2.442 August 22, 1852 Hind, J.R. 13 Egeria 206 217 × 196 2.576 November 2, 1850 de Gasparis, A. 24 Themis 198 spheroid 198 3.136 April 5, 1853 de Gasparis, A. 94 Aurora 197 225 × 173 3.160 September 6, 1867 Watson, J.C. 702 Alauda 195 97.365 ± 1.6 km 3.195 July 16, 1910 Helffrich, J. C / B 121 Hermione 190 268 × 186 × 183 3.457 May 12, 1872 Watson, J.C. 259 Aletheia 190 178 × 190 3.135 June 28, 1886 Peters, C.H.F. C / P / X 372 Palma 189 188 3.149 August 19, 1893 Charlois, A. 128 Nemesis 188 188 2.751 November 25, 1872 Watson, J.C. 6 Hebe 186 205x185x170 2.426 July 1, 1847 Hencke, K.L. 16 Psyche 186 240 × 185 × 145 2.924 March 17, 1852 de Gasparis, A. 120 Lachesis 174 184x144 3.301 April 10, 1872 Borrelly, A. 41 Daphne 174 213x160 2.765 May 22, 1856 Goldschmidt, H. 9 Metis 174 222x182x130 2.385 April 25, 1848 Graham, A. The number of bodies grows rapidly as the size decreases. Based on IRAS data there are about 140 main - belt asteroids with a diameter greater than 120 km. For a more complete list, see List of Solar System objects by size. The inner asteroid belt ( defined as the region interior to the 3 : 1 Kirkwood gap at 2.50 AU ) has few large asteroids. Of those in the above list, only 4 Vesta, 19 Fortuna, 6 Hebe, 7 Iris and 9 Metis orbit there. Most massive Below are the nineteen most massive measured asteroids. The masses of asteroids are calculated from perturbations they induce on the orbits of other asteroids, except for asteroids that have been visited by spacecraft or have an observable moon, where a direct mass determination is possible. Different sets of astrometric observations lead to different mass determinations ; the biggest problem is accounting for the aggregate perturbations caused by all of the smaller asteroids. The relative masses of the top twelve asteroids known, compared to the remaining mass of the asteroid belt. 1 Ceres 4 Vesta 2 Pallas 10 Hygiea 31 Euphrosyne 704 Interamnia 511 Davida 532 Herculina 15 Eunomia 3 Juno 16 Psyche 52 Europa all others Name Mass ( × 10 kg ) Precision Approx. prop'n all asteroids Diameter ranking 1 Ceres 939.3 0.05 % ( 939 -- 940 ) 31 % 4 Vesta 259.076 0.0004 % ( 259.075 -- 259.077 ) 8.6 % 2 Pallas 201 6.4 % ( 188 -- 214 ) 6.7 % 10 Hygiea 86.7 1.7 % ( 85.2 -- 88.4 ) 2.9 % 31 Euphrosyne 58.1 34 % ( 38.4 -- 77.8 ) 1.9 % 12 704 Interamnia 38.8 4.6 % ( 37.0 -- 40.6 ) 1.3 % 5 511 Davida 37.7 5.2 % ( 35.7 -- 39.7 ) 1.3 % 7 532 Herculina 33 17 % ( 27 -- 39 ) 1.1 % 17 15 Eunomia 31.8 0.9 % ( 31.5 -- 32.1 ) 1.1 % 10 3 Juno 28.6 16 % ( 24.0 -- 33.2 ) 0.95 % 11 16 Psyche 22.7 3.7 % ( 21.9 -- 23.5 ) 0.76 % 35 52 Europa 22.7 7 % ( 21.1 -- 24.3 ) 0.76 % 6 88 Thisbe 18.3 6 % ( 17.2 -- 19.4 ) 0.61 % 14 7 Iris 16.2 5.6 % ( 15.3 -- 17.1 ) 0.54 % 21 13 Egeria 16 27 % ( 12 -- 20 ) 0.53 % 26 423 Diotima 16 Unknown 0.53 % 24 29 Amphitrite 15.2 4 % ( 14.8 -- 15.6 ) 0.51 % 23 87 Sylvia 14.78 0.4 % ( 14.72 -- 14.84 ) 0.49 % 8 48 Doris 12 50 % ( 6 -- 18 ) 0.4 % 18 Total 1868.0 NA 62.0 % NA ( All the data above are from Baer et al. 2011, apart from 48 Doris and 532 Herculina, which are Kochetova, 2004. The proportions assume that the total mass is 3.0 × 10 kg, or 6991150000000000000 ♠ ( 15.0 ± 1.0 ) × 10 M. Significant uncertainties remain. For example, the uncertainty in the estimate of 31 Euphrosyne is enough for its low end to overlap with both 704 Interamnia and 511 Davida, which overlap each other and also with 532 Herculina, which overlaps with 15 Eunomia and 3 Juno. Juno barely overlaps 52 Europa, which in turn overlaps with 16 Psyche. That is, outside the top four, the order of all the asteroids is uncertain. However, none of the lesser asteroids, of which the most massive are thought to be 88 Thisbe ( at 17 -- 19 × 10 kg ), 7 Iris, 29 Amphitrite and 48 Doris ( all in the range of ≈ 15 × 10 kg ), overlap with Europa or Psyche, so the first 12 asteroids in the chart above are likely to be the top dozen unless a hitherto unmeasured asteroid proves to be unexpectedly massive. The largest asteroids with an accurately measured mass, due to the fact that they have been ( and are being ) studied by the probe Dawn, are 1 Ceres with a mass of 939.3 ± 0.5 × 10 kg, and 4 Vesta at 259.076 ± 0.001 × 10 kg. The third - largest asteroid with an accurately measured mass, due to the fact that it has moons, is 87 Sylvia at 14.78 ± 0.06 × 10 kg. For a more complete list, see List of Solar System objects by size. Other large asteroids such as 423 Diotima currently only have estimated masses. Brightest from Earth Only Vesta regularly attains a brightness sufficient to be visible to the naked eye. The following asteroids can all reach an apparent magnitude brighter than or equal to the + 8.3 attained by Saturn 's moon Titan at its brightest, which was discovered 145 years before the first asteroid was found owing to its closeness to the easily observed Saturn. None of the asteroids in the outer part of the asteroid belt can ever attain this brightness. Even Hygiea and Interamnia rarely reach magnitudes of above 10.0. This is due to the different distribution of spectral types within different sections of the asteroid belt being such that the highest - albedo asteroids are all concentrated closer to Mars, and much lower albedo C and D types being common in the outer belt. Those asteroids with very high eccentricities will only reach their maximum magnitude on unusual occasions when their perihelion is very close to a heliocentric conjunction with Earth, or ( in the case of 99942 Apophis ) when the asteroid passes very close to Earth. Asteroid Magnitude when brightest Semi-major axis ( AU ) Eccentricity of orbit Diameter ( km ) Year of discovery 99942 Apophis 3.4 0.922 0.191 0.32 4 Vesta 5.20 2.361 0.089172 529 1807 2 Pallas 6.49 2.773 0.230725 544 1802 1 Ceres 6.65 2.766 0.079905 952 1801 7 Iris 6.73 2.385 0.231422 200 1847 433 Eros 6.8 1.458 0.222725 34 × 11 × 11 1898 6 Hebe 7.5 2.425 0.201726 186 1847 3 Juno 7.5 2.668 0.258194 233 1804 18 Melpomene 7.5 2.296 0.218708 141 1852 15 Eunomia 7.9 2.643 0.187181 268 1851 8 Flora 7.9 2.202 0.156207 128 1847 324 Bamberga 8.0 2.682 0.338252 229 1892 1036 Ganymed 8.1 2.6657 0.533710 32 1924 9 Metis 8.1 2.387 0.121441 190 1848 192 Nausikaa 8.2 2.404 0.246216 103 1879 20 Massalia 8.3 2.409 0.142880 145 1852 * Apophis will only achieve that brightness on April 13, 2029. It typically has an apparent magnitude of 20 -- 22. Slowest rotators For a more comprehensive list, see List of slow rotators ( minor planets ). This list contains the slowest - rotating known minor planets with a period of at least 1000 hours, or 41 ​ ⁄ days, while most bodies have rotation periods between 2 and 20 hours. Also see Potentially slow rotators for minor planets with an insufficiently accurate period ( U < 2 ). # Minor planet designation Rotation period ( hours ) Δ mag Quality ( U ) Orbit or family Spectral type Diameter ( km ) Abs. mag ( H ) Refs 1. 846 Lipperta 1641 0.30 2 Themis CBU : 52.41 10.26 LCDB List 2. 912 Maritima 1332 0.18 3 - MBA ( outer ) 82.14 9.30 LCDB List 3. 9165 Raup 1320 1.34 3 - Hungaria 4.62 13.60 LCDB List 4. 1235 Schorria 1265 1.40 3 Hungaria CX : 5.04 13.10 LCDB List 5. ( 50719 ) 2000 EG 140 1256 0.42 2 Eunomia 3.40 14.65 LCDB List 6. ( 75482 ) 1999 XC 173 1234.2 0.69 2 Vestian 2.96 15.01 LCDB List 7. 288 Glauke 1170 0.90 3 MBA ( outer ) 32.24 10.00 LCDB List 8. ( 39546 ) 1992 DT 5 1167.4 0.80 2 MBA ( outer ) 5.34 15.09 LCDB List 9. 4524 Barklajdetolli 1069 1.26 2 Flora 7.14 12.90 LCDB List 10. 2675 Tolkien 1060 0.75 2 + Flora 9.85 12.20 LCDB List 11. ( 219774 ) 2001 YY 145 1007.7 0.86 2 MBA ( inner ) 1.54 16.43 LCDB List back to top Fastest rotators For a more comprehensive list, see List of fast rotators ( minor planets ). This list contains the fastest - rotating minor planets with a period of less than 100 seconds, or 0.027 hours. Bodies with a highly uncertain period, having a quality of less than 2, are highlighted in dark - grey. The fastest rotating bodies are all unnumbered near - Earth objects ( NEOs ) with a diameter of less than 100 meters ( see table ). Among the numbered minor planets with an unambiguous period solution are ( 459872 ) 2014 EK 24, a 60 - meter sized stony NEO with a period of 352 seconds, as well as ( 335433 ) 2005 UW 163 and ( 60716 ) 2000 GD 65, two main - belt asteroids, with a diameter of 0.86 and 2.25 kilometers and a period of 1.29 and 1.95 hours, respectively ( see full list ). # Minor planet designation Rotation period Δ mag Quality ( U ) Orbit or family Spectral type Diameter ( km ) Abs. mag ( H ) Refs ( seconds ) ( hours ) 1. 2014 RC 16 0.004389 0.10 n.a. NEO 0.01 26.80 LCDB MPC 2. 2010 JL 88 25 0.0068295 0.52 3 NEO 0.01 26.80 LCDB MPC 3. 2010 WA 31 0.0085799 0.22 3 NEO 0.00 30.00 LCDB MPC 4. 2016 GE 34 0.009438 0.13 2 NEO 0.01 26.60 LCDB MPC 5. 2008 HJ 43 0.01185 0.80 3 - NEO 0.02 25.80 LCDB MPC 6. 2009 TM 43 0.012 -- n.a. NEO 0.01 28.40 LCDB MPC 7. 2010 SK 52 0.0144 -- n.a. NEO 0.01 27.40 LCDB MPC 8. 2009 BF 57 0.01593 0.80 3 NEO 0.02 25.90 LCDB MPC 9. 2016 GS 66 0.0182725 0.06 1 NEO 0.08 23.00 LCDB MPC 10. 2010 TG 70 0.0193935 1.10 3 NEO 0.05 23.90 LCDB MPC 11. 2008 WA 70 0.0195 -- n.a. NEO 0.08 23.00 LCDB MPC 12. 2007 KE 77 0.021408 0.38 3 - NEO 0.03 25.20 LCDB MPC 13. 2000 DO 78 0.0217 1.39 3 NEO 0.04 24.54 LCDB MPC 14. 2014 TV 79 0.02190 0.32 2 NEO 0.04 24.40 LCDB MPC 15. 2000 WH 80 0.02221 0.66 3 - NEO 0.09 22.50 LCDB MPC 16. 2012 HG 82 0.0227 -- n.a. NEO 0.01 27.00 LCDB MPC 17. 2010 TD 54 83 0.0229317 0.92 3 NEO 0.01 28.90 LCDB MPC 18. 2010 TS 83 0.023 -- n.a. NEO 0.02 25.70 LCDB MPC 19. 2009 UD 84 0.023246 0.66 2 + NEO 0.01 27.20 LCDB MPC 20. 2015 RF 90 0.025 0.15 2 NEO 0.06 23.40 LCDB MPC 21. 2010 XE 96 0.0265846 0.50 3 NEO 0.08 23.00 LCDB MPC 22. 2000 UK 96 0.026599 0.28 2 NEO 0.03 25.30 LCDB MPC 23. 2008 TC 3 97 0.0269409 1.02 3 NEO 0.00 30.90 LCDB MPC back to top Orbital characteristics Retrograde Minor planets with orbital inclinations greater than 90 ° ( the greatest possible is 180 ° ) orbit in a retrograde direction. As of September 2016, of the more than 700,000 minor planets known, there are only 95 known retrograde minor planets. In comparison, there are over 1920 comets with retrograde orbits. This makes retrograde minor planets the rarest group of all. High - inclination asteroids are either Mars - crossers ( possibly in the process of being ejected from the Solar System ) or damocloids. Some of these are temporarily captured in retrograde resonance with the gas giants. Minor planet designation Inclination ( ° ) First observed / Discovery date Condition code Obs. × arc Comment Refs 2015 TN 90.937 ° October 8, 2015 2542 -- MPC 2005 SB 91.419 ° September 30, 2005 12200 Has a well - determined orbit MPC 2014 MH 91.478 ° June 29, 2014 9 96 -- MPC 2015 RK 91.597 ° September 12, 2015 182880 -- MPC 2010 EQ 91.606 ° March 8, 2010 9 32 -- MPC 2016 TK 92.343 ° July 13, 2016 5 3486 -- MPC 2016 FH 93.486 ° March 29, 2016 6 1638 -- MPC 2014 PP 93.627 ° August 5, 2014 5 4816 -- MPC 2015 BH 95.575 ° January 20, 2015 9 39 -- MPC 2014 JJ 95.958 ° May 9, 2014 61802 -- MPC 2014 HS 96.456 ° April 16, 2014 8 200 -- MPC 2013 BL 76 98.607 ° January 20, 2013 46716 Has a semi-major axis of 1254 AU, giving it the third largest semi-major axis of any known minor planet MPC 2010 GW 99.623 ° April 14, 2010 93632 -- MPC 2011 MM 100.446 ° June 24, 2011 36036 -- MPC 2014 XS 100.934 ° December 8, 2014 9 55 -- MPC 2013 BN 101.780 ° January 17, 2013 7 1425 -- MPC 2008 KV 42 103.483 ° May 31, 2008 5 10449 -- MPC ( 342842 ) 2008 YB 105.031 ° December 18, 2008 864896 -- MPC 2016 PN 105.111 ° August 14, 2016 15219 -- MPC 2010 GW 105.273 ° April 6, 2010 9576 -- MPC 2012 YO 106.914 ° December 22, 2012 6674 -- MPC 2009 DD 107.431 ° February 27, 2009 7 1584 -- MPC 2007 VW 108.345 ° November 12, 2007 7 2280 -- MPC 2015 MJ 108.876 ° June 27, 2015 9 -- MPC 2011 SP 108.987 ° September 20, 2011 5 3712 -- MPC ( 471325 ) 2011 KT 19 110.154 ° May 21, 2011 350463 -- MPC 2011 OR 110.345 ° May 21, 2010 75548 -- MPC 2005 TJ 110.368 ° October 3, 2005 7 1488 -- MPC 2005 VX 3 112.459 ° November 1, 2005 4050 Semi-major axis of 837AU, but has a somewhat short 81 - day observation arc for such a large orbit MPC 2016 LS 114.360 ° June 27, 2015 16800 -- MPC 2015 YY 118.232 ° December 29, 2015 6901 -- MPC 2010 OM 118.689 ° July 28, 2010 5 3232 -- MPC ( 65407 ) 2002 RP 120 119.106 ° September 4, 2002 660275 This outer - planet crosser is a damocloid and SDO ). MPC 2010 PO 121.229 ° August 5, 2010 9 168 -- MPC 2010 LG 123.732 ° June 2, 2010 9 770 -- MPC ( 468861 ) 2013 LU 125.414 ° June 8, 2013 5 21560 -- MPC 2014 SQ 128.499 ° September 9, 2014 7 1276 -- MPC 2000 DG 8 129.478 ° February 25, 2000 44460 A damocloid and SDO. Crosses all the outer planets except Neptune. Came within 0.03 AU of Ceres in 1930. MPC 2016 CO 129.852 ° February 14, 2016 8820 -- MPC 2013 NS 130.340 ° July 5, 2013 71929 -- MPC 2005 NP 130.549 ° July 6, 2005 6 8769 -- MPC 2006 RG 133.195 ° September 1, 2006 6 750 Has an orbit with a data arc of 25 days ( Uncertainty Parameter = 4 ) MPC 2012 YE 136.136 ° December 21, 2012 7 1189 -- MPC 2009 QY 137.654 ° August 17, 2009 43560 -- MPC 2016 TP 138.324 ° October 9, 2016 7 704 -- MPC 2015 AO 139.974 ° November 27, 2014 102600 -- MPC ( 336756 ) 2010 NV 1 140.818 ° July 2, 2010 266805 Perihelion at 9.4 AU, only 2008 KV has perihelion further out ( 154 - day data arc ) MPC 2011 WS 141.645 ° November 24, 2011 8 108 -- MPC 2010 OR 143.861 ° January 25, 2010 35416 -- MPC 2010 BK 118 143.910 ° January 30, 2010 385148 Semi-major axis of 408 AU with perihelion at 6.1 AU in April 2012 ( 1 year data arc ) MPC 2016 NM 144.045 ° July 14, 2016 39960 -- MPC 2010 CG 146.246 ° February 15, 2010 124816 -- MPC 2012 HD 146.897 ° April 18, 2012 32314 -- MPC 2009 YS 147.797 ° December 17, 2009 199547 -- MPC 2006 EX 150.240 ° March 5, 2006 62930 q = 2.58 AU and period = 274 yr MPC 1999 LE 31 151.807 ° June 12, 1999 51943 A damocloid, Jupiter - and Saturn - crossing minor planet. MPC 2016 JK 152.313 ° March 3, 2016 7 2448 -- MPC 2017 CW 152.436 ° June 9, 2016 46500 -- MPC ( 343158 ) 2009 HC 82 154.496 ° April 29, 2009 0 385700 NEO that sometimes has the highest relative velocity to Earth ( 79 km / s ) of known objects that come within 0.5 AU of Earth. However, the relative velocity at 1 AU from the sun is less than 72 km / s. MPC 2013 LD 154.748 ° June 6, 2013 14148 -- MPC 2015 FK 155.971 ° March 20, 2015 7 748 -- MPC 2010 EB 156.531 ° March 12, 2010 7 2610 -- MPC 2015 XR 157.532 ° December 9, 2015 5580 -- MPC 2000 HE 158.448 ° April 29, 2000 26400 -- MPC 2015 XX 159.106 ° December 9, 2015 20790 -- MPC 2012 TL 160.036 ° October 8, 2012 6 900 -- MPC 20461 Dioretsa 160.404 ° June 8, 1999 256779 most highly inclined known minor planet from 1999 / 06 / 08 - 2004 / 07 / 13 MPC ( 514107 ) 2015 BZ 509 163.001 ° November 26, 2014 72846 A Jupiter co-orbital. First known example of a retrograde co-orbital asteroid with any of the planets. Might have an interstellar origin. MPC Src 2006 RJ 164.582 ° September 14, 2006 7 2812 -- MPC 2006 BZ 165.315 ° January 23, 2006 214312 -- MPC 2004 NN 165.466 ° July 13, 2004 23944 Came within 0.80 AU of Saturn on 2007 - Jun - 05, most highly inclined known minor planet from 2004 / 07 / 13 - 2005 / 11 / 01 MPC 2014 AT 165.554 ° January 3, 2014 42517 -- MPC 2016 DF 167.030 ° February 28, 2016 9 26 -- MPC ( 330759 ) 2008 SO 170.318 ° September 30, 2008 733950 -- MPC 2014 UV 170.510 ° October 26, 2014 9 34 -- MPC 2014 CW 170.747 ° February 10, 2014 7 1938 MPC 2016 EJ 170.911 ° March 11, 2016 7 1740 -- MPC 2006 LM 172.138 ° June 3, 2006 9 48 Has a data arc of only 2 days ( Uncertainty Parameter = E ), but has a very high inclination MPC ( 434620 ) 2005 VD 172.866 ° November 1, 2005 130989 most highly inclined known minor planet from 2005 / 11 / 01 - 2013 / 06 / 01 MPC 2013 LA 2 175.189 ° June 1, 2013 8 1075 Has the highest inclination of any known minor planet MPC ^ the value given when the number of observations is multiplied by the observation arc ; larger values are generally better than smaller values depending on residuals. Highly inclined Minor planet designation Inclination Discovery date Comment Refs 1 Ceres 10.593 ° January 1, 1801 most highly inclined known minor planet from 1801 / 01 / 01 - 1802 / 03 / 28 MPC 2 Pallas 34.841 ° March 28, 1802 most highly inclined known minor planet from 1802 / 03 / 28 - 1920 / 10 / 31 MPC 944 Hidalgo 42.525 ° October 31, 1920 most highly inclined known minor planet from 1920 / 10 / 31 - 1950 / 05 / 22 MPC 1373 Cincinnati 38.949 ° August 30, 1935 First main - belt asteroid discovered to have an inclination greater than 2 Pallas. Most highly inclined known main - belt asteroid from 1935 / 08 / 30 - 1980 / 06 / 14 MPC 1580 Betulia 52.083 ° May 22, 1950 most highly inclined known minor planet from 1950 / 05 / 22 - 1973 / 07 / 04 MPC 2938 Hopi 41.436 ° June 14, 1980 Most highly inclined known main - belt asteroid from 1980 / 06 / 14 - 2000 / 09 / 20 MPC ( 5496 ) 1973 NA 67.999 ° July 4, 1973 An Apollo asteroid, Mars - crosser and + 1 km NEO ; most highly inclined known minor planet from 4 July 1973 to 8 August 1999. MPC ( 22653 ) 1998 QW 45.794 ° August 17, 1998 Most highly inclined known main - belt asteroid from 1998 / 08 / 17 - 1998 / 10 / 19 MPC ( 88043 ) 2000 UE 51.998 ° October 29, 2000 First main - belt asteroid discovered and numbered to have an inclination greater than 50 °. MPC ( 138925 ) 2001 AU 72.132 ° January 4, 2001 A Mars - crosser and near - Earth object. MPC ( 127546 ) 2002 XU 77.904 ° December 4, 2002 A damocloid and SDO. It is almost a Uranus outer - grazer. MPC ( 196256 ) 2003 EH 1 70.790 ° March 6, 2003 A Mars - crosser, near - Earth object and Jupiter inner - grazer. MPC 1998 UQ 64.281 ° October 19, 1998 Most highly inclined known main - belt asteroid from 1998 / 10 / 19 - 2007 / 11 / 01 MPC ( 467372 ) 2004 LG 70.725 ° June 9, 2004 A Mercury - through Mars - crosser and near - Earth object. MPC 2007 VR 68.659 ° November 1, 2007 Most highly inclined known main - belt asteroid from 2007 / 11 / 01 - 2008 / 09 / 26 MPC 2008 SB 74.247 ° September 26, 2008 Most highly inclined known main - belt asteroid from 2008 / 09 / 26 - 2010 / 03 / 08 ( ? ) MPC 2010 EQ 91.606 ° March 8, 2010 Most highly inclined known main - belt asteroid ( ? ) ( orbit is not well - known ) MPC Trojans Earth trojans : 2010 TK 7. Mars trojans : ( 121514 ) 1999 UJ 7, 5261 Eureka, ( 101429 ) 1998 VF 31, ( 311999 ) 2007 NS 2, ( 385250 ) 2001 DH 47, 2011 SC 191, 2011 UN 63, and the candidate 2011 SL 25. Jupiter trojans : the first one was discovered in 1906, 588 Achilles, and the current total is over 6,000. Record - setting close approaches to Earth Main article : List of asteroid close approaches to Earth Timeline Landmark asteroids Name Diameter ( km ) Discovered Comment 5 Astraea 117 December 8, 1845 First asteroid discovered after original four ( 38 years later ) 87 Sylvia 261 May 16, 1866 First asteroid known to have more than one moon ( determined in 2005 ) 90 Antiope 80 × 80 October 1, 1866 Double asteroid with two nearly equal components ; its double nature was discovered using adaptive optics in 2000 92 Undina 126 1867 July 7 Created in one of the largest asteroid - on - asteroid collisions of the past 100 million years 216 Kleopatra 217 × 94 April 10, 1880 Metallic asteroid with `` ham - bone '' shape and 2 satellites 243 Ida 56 × 24 × 21 September 29, 1884 First asteroid known to have a moon ( determined in 1993 ) 243 Ida I Dactyl 1.4 February 17, 1994 Moon of 243 Ida, first confirmed satellite of an asteroid 279 Thule 127 October 25, 1888 Orbits in the asteroid belt 's outermost edge in a 3 : 4 orbital resonance with Jupiter 288 Glauke 32 February 20, 1890 Exceptionally slow rotation period of about 1200 hours ( 2 months ) 323 Brucia 36 December 22, 1891 First asteroid discovered by means of astrophotography rather than visual observation 433 Eros 13 × 13 × 33 August 13, 1898 First near - Earth asteroid discovered and the second largest ; first asteroid to be detected by radar ; first asteroid orbited and landed upon 490 Veritas 115 September 3, 1902 Created in one of the largest asteroid - on - asteroid collisions of the past 100 million years 588 Achilles 135.5 February 22, 1906 First Jupiter trojan discovered 624 Hektor 370 × 195 February 10, 1907 Largest Jupiter trojan discovered 719 Albert 2.4 October 3, 1911 Last numbered asteroid to be lost then recovered 1125 China October 30, 1957 First asteroid discovery to be credited to an institution rather than a person 1566 Icarus 1.4 June 27, 1949 First Mercury crosser discovered 1902 Shaposhnikov 97 April 18, 1972 The most recent main - belt asteroid discovered that is ~ 100 + km in diameter 2063 Bacchus 1.1 × 1.1 × 2.6 April 24, 1977 3200 Phaethon 5 October 11, 1983 First asteroid discovered from space ; source of Geminids meteor shower. 3753 Cruithne 5 October 10, 1986 Unusual Earth - associated orbit 4179 Toutatis 4.5 × 2.4 × 1.9 January 4, 1989 Closely approached Earth on September 29, 2004 4769 Castalia 1.8 × 0.8 August 9, 1989 First asteroid to be radar - imaged in sufficient detail for 3D modeling 5261 Eureka ~ 2 -- 4 June 20, 1990 First Mars trojan ( Lagrangian point L ) discovered 11885 Summanus September 25, 1990 First automated discovery of a near - Earth object ( NEO ) ( 29075 ) 1950 DA 1.1 February 23, 1950 Will approach Earth very closely in 2880, collision unlikely ( 1 in 8,300 or 0.012 % ) 69230 Hermes 0.3 October 28, 1937 Named but not numbered until its recovery in 2003 ( 65 years later ) 99942 Apophis 0.3 June 19, 2004 First asteroid to rank greater than one on the Torino Scale ( it was ranked at 2, then 4 ; now down to 0 ). Previously better known by its provisional designation 2004 MN. ( 433953 ) 1997 XR 2 0.23 December 4, 1997 First asteroid to rank greater than zero on the impact - risk Torino Scale ( it was ranked 1 ; now at 0 ) 1998 KY 26 0.030 June 2, 1998 Approached within 800,000 km of Earth 2002 AA 29 0.1 January 9, 2002 Unusual Earth - associated orbit 2004 FH 0.030 March 15, 2004 Discovered before it approached within 43,000 km of Earth on March 18, 2004. 2008 TC 3 ~ 0.003 October 6, 2008 First Earth - impactor to be spotted before impact ( on October 7, 2008 ) 2010 TK 7 ~ 0.3 October 2010 First Earth trojan to be discovered 2014 RC ~ 0.017 September 1, 2014 Asteroid with fastest rotation : 16.2 seconds Spacecraft targets See also : List of minor planets and comets visited by spacecraft Name Diameter ( km ) Discovered Spacecraft Year ( s ) Closest approach ( km ) closest approach ( asteroid radii ) Notes Landmark ( s ) 1 Ceres 952 January 1, 1801 Dawn 2014 -- present 7002200000000000000 ♠ approx. 200 ( planned ) 0.42 Dawn took its first `` close up '' picture of Ceres in December 2014, and entered orbit in March 2015 First dwarf planet visited by a spacecraft, largest asteroid visited by a spacecraft 4 Vesta 529 March 29, 1807 Dawn 2011 -- 2012 7002210000000000000 ♠ 210 0.76 Dawn broke orbit on 5 September 2012 and headed to Ceres, where it arrived in March 2015 First `` big four '' asteroid visited by a spacecraft, largest asteroid visited by a spacecraft at the time 21 Lutetia 120 × 100 × 80 November 15, 1852 Rosetta 7003316200000000000 ♠ 3,162 64.9 Flyby on 10 July 2010 Largest asteroid visited by a spacecraft at the time 243 Ida 56 × 24 × 21 September 29, 1884 Galileo 7003239000000000000 ♠ 2,390 152 Flyby ; discovered Dactyl First asteroid with a moon visited by a spacecraft, largest asteroid visited by spacecraft at the time 253 Mathilde 66 × 48 × 46 November 12, 1885 NEAR Shoemaker 7003121200000000000 ♠ 1,212 49.5 Flyby Largest asteroid visited by a spacecraft at the time 433 Eros 13 × 13 × 33 August 13, 1898 NEAR Shoemaker 1998 -- 2001 5000000000000000000 ♠ 0 0 1998 flyby ; 2000 orbited ( first asteroid studied from orbit ) ; 2001 landing First asteroid landing, first asteroid orbited by a spacecraft, first near - Earth asteroid ( NEA ) visited by a spacecraft 951 Gaspra 18.2 × 10.5 × 8.9 July 30, 1916 Galileo 1991 7003160000000000000 ♠ 1,600 262 Flyby first asteroid visited by a spacecraft 2867 Šteins 4.6 November 4, 1969 Rosetta 2008 7002800000000000000 ♠ 800 302 Flyby First asteroid visited by the ESA 4179 Toutatis 4.5 × ~ 2 February 10, 1934 Chang'e 2 2012 7000320000000000000 ♠ 3.2 0.70 Flyby Closest asteroid flyby, first asteroid visited by China 5535 Annefrank 4.0 March 23, 1942 Stardust 2002 7003307900000000000 ♠ 3,079 1230 Flyby 9969 Braille 2.2 × 0.6 May 27, 1992 Deep Space 1 1999 7001260000000000000 ♠ 26 12.7 Flyby ; followed by flyby of Comet Borrelly 25143 Itokawa 0.5 × 0.3 × 0.2 September 26, 1998 Hayabusa 2005 5000000000000000000 ♠ 0 0 Landed ; returned dust samples to Earth First asteroid with returned samples, smallest asteroid visited by a spacecraft, first asteroid visited by a non-NASA spacecraft Numbered minor planets that are also comets Name Cometary name Comment 2060 Chiron 95P / Chiron First centaur discovered in 1977, later identified to exhibit cometary behaviour. Also one of two minor planets known to have a ring system 4015 Wilson -- Harrington 107P / Wilson -- Harrington In 1992, it was realized that asteroid 1979 VA 's orbit matched it with the positions of the lost comet Wilson -- Harrington ( 1949 III ) 7968 Elst -- Pizarro 133P / Elst -- Pizarro Discovered in 1996 as a comet, but orbitally matched to asteroid 1979 OW 60558 Echeclus 174P / Echeclus Centaur discovered in 2000, comet designation assigned in 2006 118401 LINEAR 176P / LINEAR ( LINEAR 52 ) Main - belt comet -- asteroid discovered to have a coma on November 26, 2005 The above table lists only numbered asteroids that are also comets. Note there are several cases where a non-numbered minor planets turned out to be a comet, e.g. C / 2001 OG108 ( LONEOS ), which was provisionally designated 2001 OG. Minor planets that were misnamed and renamed In earlier times, before the modern numbering and naming rules were in effect, asteroids were sometimes given numbers and names before their orbits were precisely known. And in a few cases duplicate names were given to the same object ( with modern use of computers to calculate and compare orbits with old recorded positions, this type of error no longer occurs ). This led to a few cases where asteroids had to be renamed. Minor planet name Description 330 Adalberta An object discovered March 18, 1892 by Max Wolf with provisional designation `` 1892 X '' was named 330 Adalberta, but was lost and never recovered. In 1982 it was determined that the observations leading to the designation of 1892 X were stars, and the object never existed. The name and number 330 Adalberta was then reused for another asteroid discovered by Max Wolf on February 2, 1910, which had the provisional designation A910 CB. 525 Adelaide The object A904 EB discovered March 14, 1904 by Max Wolf was named 525 Adelaide and was subsequently lost. Later, the object 1930 TA discovered October 3, 1930 by Sylvain Arend was named 1171 Rusthawelia. In those pre-computer days, it was not realized until 1958 that these were one and the same object. The name Rusthawelia was kept ( and discovery credited to Arend ) ; the name 525 Adelaide was reused for the object 1908 EKa discovered October 21, 1908 by Joel Hastings Metcalf. 715 Transvaalia and 933 Susi The object 1911 LX discovered April 22, 1911 by H.E. Wood was named 715 Transvaalia. On April 23, 1920, the object 1920 GZ was discovered and named 933 Susi. In 1928 it was realized that these were one and the same object. The name Transvaalia was kept, and the name and number 933 Susi was reused for the object 1927 CH discovered February 10, 1927 by Karl Reinmuth. 864 Aase and 1078 Mentha The object A917 CB discovered February 13, 1917 by Max Wolf was named 864 Aase, and the object 1926 XB discovered December 7, 1926 by Karl Reinmuth was named 1078 Mentha. In 1958 it was discovered that these were one and the same object. In 1974, this was resolved by keeping the name 1078 Mentha and reusing the name and number 864 Aase for the object 1921 KE, discovered September 30, 1921 by Karl Reinmuth. 1095 Tulipa and 1449 Virtanen The object 1928 DC discovered February 24, 1928 by Karl Reinmuth was named 1095 Tulipa, and the object 1938 DO discovered February 20, 1938 by Yrjö Väisälä was named 1449 Virtanen. In 1966 it was discovered that these were one and the same object. The name 1449 Virtanen was kept and the name and number 1095 Tulipa was reused for the object 1926 GS discovered April 14, 1926 by Karl Reinmuth. 1125 China and 3789 Zhongguo The object 1928 UF discovered October 25, 1928 by Zhang Yuzhe ( Y.C. Chang ) was named 1125 China, and was later lost. Later, the object 1957 UN was discovered on October 30, 1957 at Purple Mountain Observatory and was initially incorrectly believed to be the rediscovery of the object 1928 UF. The name and number 1125 China were then reused for the object 1957 UN, and 1928 UF remained lost. In 1986, the object 1986 QK 1 was discovered and proved to be the real rediscovery of 1928 UF. This object was given the new number and name 3789 Zhongguo. Note Zhongguo is the Mandarin Chinese word for `` China '', in pinyin transliteration. Asteroid 1317 The object 1914 UQ discovered April 20, 1914 by G.N. Neujmin was named 787 Moskva ( and retains that name to this day ). The object 1934 FD discovered on March 19, 1934 by C. Jackson was given the sequence number 1317. In 1938, G.N. Neujmin found that asteroid 1317 and 787 Moskva were one and the same object. The sequence number 1317 was later reused for the object 1935 RC discovered on September 1, 1935 by Karl Reinmuth ; that object is now known as 1317 Silvretta. See also Asteroid mining Asteroid Redirect Mission ( proposed NASA mission ) Centaur ( minor planet ) List of numbered Aten asteroids List of Amor asteroids List of Apollo asteroids List of asteroids named after people List of asteroids named after places List of instrument - resolved minor planets List of meteor air bursts List of minor planet moons List of Venus - crossing minor planets List of Earth - crossing minor planets List of Jupiter - crossing minor planets List of Mars - crossing minor planets List of Mercury - crossing minor planets List of Neptune - crossing minor planets List of Saturn - crossing minor planets List of Solar System objects by size List of Uranus - crossing minor planets Scattered disc object Oumuamua Books Dictionary of Minor Planet Names, 5th ed. : Prepared on Behalf of Commission 20 Under the Auspices of the International Astronomical Union, Lutz D. Schmadel, ISBN 3 - 540 - 00238 - 3 References Jump up ^ Savage, Don ; Jones, Tammy ; Villard, Ray ( 1995 ). `` Asteroid or Mini-Planet ? Hubble Maps the Ancient Surface of Vesta ''. Hubble Site News Release STScI - 1995 - 20. Retrieved 2006 - 10 - 17. Jump up ^ Carry, B. ; et al. ( 2009 ). `` Physical properties of ( 2 ) Pallas '' ( PDF ). Retrieved 13 September 2015. Jump up ^ `` JPL Small - Body Database Search Engine : asteroids and orbital class ( IMB or MBA or OMB ) and diameter > 120 ( km ) ''. JPL 's Solar System Dynamics Group. Retrieved 2012 - 04 - 16. ^ Jump up to : `` Recent Asteroid Mass Determinations ''. Maintained by Jim Baer. Last updated 2010 - 12 - 12. Access date 2011 - 09 - 02. Jump up ^ Baer, James ; Steven R. Chesley ( 2008 ). `` Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris '' ( PDF ). Celestial Mechanics and Dynamical Astronomy. Springer Science + Business Media B.V. 2007. 100 ( 2008 ) : 27 -- 42. Bibcode : 2008CeMDA. 100... 27B. doi : 10.1007 / s10569 - 007 - 9103 - 8. Retrieved 2008 - 11 - 11. ^ Jump up to : Pitjeva, E.V. ( May 2005 ). `` High - Precision Ephemerides of Planets -- EPM and Determination of Some Astronomical Constants '' ( PDF ). Solar System Research. 39 ( 3 ) : 184. Bibcode : 2005SoSyR... 39... 176P. doi : 10.1007 / s11208 - 005 - 0033 - 2. Jump up ^ Pitjeva, E.V. ( 2004 ). `` Estimations of masses of the largest asteroids and the main asteroid belt from ranging to planets, Mars orbiters and landers ''. 35th COSPAR Scientific Assembly. Held 18 -- 25 July 2004, in Paris, France. p. 2014. Bibcode : 2004cosp... 35.2014 P. Jump up ^ Michalak, G. ( 2001 ). `` Determination of asteroid masses ''. Astronomy & Astrophysics. 374 ( 2 ) : 703 -- 711. Bibcode : 2001A&A... 374... 703M. doi : 10.1051 / 0004 - 6361 : 20010731. Retrieved 2008 - 11 - 10. Jump up ^ Michalak, G. ( 2001 ), assumed masses of perturbing asteroids used in calculations of perturbations of the test asteroids. Jump up ^ `` ( 99942 ) Apophis Ephemerides for 13 Apr 2029 ''. NEODyS ( Near Earth Objects - Dynamic Site ). Retrieved 2011 - 05 - 05. Jump up ^ `` ( 99942 ) Apophis Ephemerides for 13 Apr 2029 ''. Minor Planet Center Ephemeris Service - Dynamic Site ). Jump up ^ `` JPL Small - Body Database Search Engine : Asteroids and i > 90 ( deg ) ''. JPL Solar System Dynamics. Retrieved 2016 - 09 - 12. Jump up ^ Morais, M.H.M. ; F. Namouni. `` Asteroids in retrograde resonance with Jupiter and Saturn ''. Monthly Notices of the Royal Astronomical Society Letters ( in press ). arXiv : 1308.0216. Bibcode : 2013MNRAS. 436L... 30M. doi : 10.1093 / mnrasl / slt106. Jump up ^ 2008 DG8 and Ceres in 1930 Jump up ^ 1999 LE31 approaches to Jupiter and Saturn Jump up ^ `` 1994 Release # 9412 '' ( Press release ). NASA. 1994 - 02 - 18. Retrieved 2008 - 04 - 17. Jump up ^ `` 29075 ( 1950 DA ) Earth Impact Risk Summary ''. NASA / JPL Near - Earth Object Program Office. 7 December 2015. Retrieved 11 March 2018. Jump up ^ Chang'E 2 images of Toutatis -- December 13, 2012 -- The Planetary Society Jump up ^ `` Archived copy ''. Archived from the original on 2004 - 07 - 03. Retrieved 2004 - 04 - 27. External links Lists and plots : Minor Planets PDS Asteroid Data Archive SBN Small Bodies Data Archive NASA Near Earth Object Program Major News About Minor Objects Asteroids Main Notable asteroids Physical characteristics dynamic method Impact avoidance Tracking Capture Gravitational keyhole Earth - crosser Close approaches Binary moon contact P -- L Distribution Interior to Earth vulcanoids Mercury - crossers Venus - crossers Main - belt Kirkwood gap comets Trojans Venus trojan Earth Mars Jupiter Uranus trojan Neptune trojan Near - Earth Aten Amor Apollo Apohele Earth - crossers Between Earth and the main belt Mars crossers Mars trojans Outer Solar System, does not include distant minor planets Jupiter - crossers Jupiter trojan Classification Orbital Group Family ( list ) Spectral Tholen C - group B - type F - type G - type C - type S - type X-group M - type E-type P - type small classes A-type D - type J - type T - type Q - type R - type V - type SMASS C - group B - type C - type Cg Ch Cgh Cb S - group A-type Q - type R - type K - type L - type S - type Sa Sq Sr Sk Sl X-group X-type Xe Xc Xk small types T - type D - type Ld - type O - type V - type Exploration Asteroid Redirect Mission Asteroids visited by spacecraft Human mission Mining Ceres Colonization Lists Near - Earth Minor planets Lost Discovering observatories Space missions See also : Asteroids in fiction Asteroids in astrology occultation Comet Minor planet Retrieved from `` https://en.wikipedia.org/w/index.php?title=List_of_exceptional_asteroids&oldid=852227202 '' Categories : Lists of asteroids Hidden categories : All articles with unsourced statements Articles with unsourced statements from July 2017 Articles with hCards Articles containing potentially dated statements from September 2016 All articles containing potentially dated statements Talk Contents About Wikipedia Deutsch Français Galego Italiano עברית Қазақша 日本 語 Português Română Suomi Vèneto 中文 4 more Edit links This page was last edited on 27 July 2018, at 13 : 26 ( UTC ). 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Question: what is the biggest asteroid in the solar system
Answer: Ceres