Time of discovery of asteroids which came closer to Earth than the Moon in 2017 | ||
|
Below is the list of asteroid close approaches to Earth in 2017.
A list of known near-Earth asteroid close approaches less than 1 lunar distance (0.0025696 AU (384,410 km; 238,860 mi)) from Earth in 2017. [lower-alpha 1]
For reference, the radius of Earth is approximately 0.0000426 AU (6,370 km; 3,960 mi) or 0.0166 lunar distances.
Geosynchronous satellites have an orbit with semi-major axis length of 0.000282 AU (42,200 km; 26,200 mi) or 0.110 lunar distances. In 2017, five known asteroids have traveled nearer than this, 2017 GM, 2017 UJ2, YU95BEF, 2017 EA, and 2017 WE30. P10ELNY and A104Vqx probably have traveled nearer, but knowledge of their orbits is too poor to be sure.
While most asteroids on this list are confirmed, well-observed unconfirmed objects with a 50% or greater chance of passing within 1 LD of the Earth are included as well.
This list does not include any of the 29 objects that collided with earth in 2017, none of which were discovered in advance, but were recorded by sensors designed to detect detonation of nuclear devices (of the 29 objects detected, 6 had an impact energy greater than that of a 1 kiloton device). [1]
Rows highlighted red indicate objects which were not discovered until after closest approach
Rows highlighted yellow indicate objects discovered less than 24 hours before closest approach
Rows highlighted green indicate objects discovered more than one week before closest approach
Rows highlighted turquoise indicate objects discovered more than 7 weeks before closest approach
Rows highlighted blue indicate objects discovered more than one year before closest approach (i.e.
objects successfully cataloged on a previous orbit, rather than being detected during final approach)
Date of closest approach | Date discovered | Object | Nominal geocentric distance (AU) [lower-alpha 2] | Nominal geocentric dist. (LD) | Size (m) (approx.) | (H) (mag) | Closer to Moon? |
---|---|---|---|---|---|---|---|
2017-01-09 | 2017-01-07 [2] | 2017 AG13 | 0.00139 AU (208,000 km ; 129,000 mi ) | 0.54 | 13–41 | 26.1 [3] | |
2017-01-25 | 2017-01-20 [4] | 2017 BX | 0.00178 AU (266,000 km; 165,000 mi) | 0.69 | 5–18 | 28.0 [5] | |
2017-01-30 | 2017-01-29 [6] | 2017 BH30 | 0.000347 AU (51,900 km; 32,300 mi) | 0.13 [lower-alpha 3] | 4–12 | 28.8 [7] | |
2017-02-02 | 2017-01-30 [8] | 2017 BS32 | 0.00109 AU (163,000 km; 101,000 mi) | 0.42 | 7–24 | 27.3 [9] | |
2017-02-23 | 2017-02-21 [10] | 2017 DG16 | 0.000920 AU (137,600 km; 85,500 mi) | 0.36 | 3–9 | 29.3 [11] | Yes |
2017-02-25 | 2017-02-22 [12] | 2017 DR34 | 0.00149 AU (223,000 km; 139,000 mi) | 0.58 | 3–11 | 29.1 [13] | |
2017-03-02 | 2017-03-02 [14] | 2017 EA | 0.000140 AU (20,900 km; 13,000 mi) | 0.054 | 1–5 | 30.8 [15] | |
2017-03-05 | 2017-02-27 [16] | 2017 DS109 | 0.00236 AU (353,000 km; 219,000 mi) | 0.92 | 13–43 | 25.9 [17] | |
2017-03-17 | 2017-03-19 [18] | 2017 FD3 | 0.00120 AU (180,000 km; 112,000 mi) | 0.47 | 6–20 | 27.7 [19] | |
2017-03-17 | 2017-03-19 [20] | 2017 FW158 | 0.000815 AU (121,900 km; 75,800 mi) | 0.32 | 5–14 | 28.4 [21] | |
2017-03-19 | 2017-03-17 [22] | 2017 FS | 0.000730 AU (109,200 km; 67,900 mi) | 0.28 | 3–11 | 29.0 [23] | |
2017-03-20 | 2017-03-21 [24] | 2017 FX158 | 0.00182 AU (272,000 km; 169,000 mi) | 0.71 | 3–11 | 29.0 [25] | |
2017-03-20 | 2017-03-20 [26] | 2017 FN1 | 0.000423 AU (63,300 km; 39,300 mi) | 0.16 | 2–5 | 30.6 [27] | |
2017-03-20 | 2017-03-20 [28] | 2017 FM1 | 0.000856 AU (128,100 km; 79,600 mi) | 0.33 | 3–9 | 29.5 [29] | |
2017-03-30 | 2017-03-25 [30] | 2017 FJ101 | 0.00217 AU (325,000 km; 202,000 mi) | 0.85 | 4–15 | 28.5 [31] | |
2017-04-02 | 2017-03-29 [32] | 2017 FU102 | 0.00146 AU (218,000 km; 136,000 mi) | 0.57 | 4–13 | 28.7 [33] | |
2017-04-04 | 2017-04-03 [34] | 2017 GM | 0.000109 AU (16,300 km; 10,100 mi) | 0.042 | 2–7 | 29.9 [35] | |
2017-04-16 | 2017-04-17 [36] | 2017 HJ | 0.000908 AU (135,800 km; 84,400 mi) | 0.35 | 7–22 | 27.5 [37] | |
2017-04-22 | 2017-04-26 [38] | 2017 HG4 | 0.00156 AU (233,000 km; 145,000 mi) | 0.61 | 6–21 | 27.6 [39] | |
2017-04-23 | 2017-04-22 [40] | 2017 HV2 | 0.000838 AU (125,400 km; 77,900 mi) | 0.33 | 3–12 | 28.9 [41] | |
2017-05-02 | 2017-05-01 [42] | 2017 JA | 0.000666 AU (99,600 km; 61,900 mi) | 0.26 | 3–13 | 28.9 [43] | |
2017-05-04 | 2017-05-02 [44] | 2017 JQ1 | 0.00114 AU (171,000 km; 106,000 mi) | 0.44 | 3–9 | 29.4 [45] | |
2017-05-04 | 2017-05-06 [46] | 2017 JB2 | 0.000372 AU (55,700 km; 34,600 mi) | 0.14 | 3–11 | 29.0 [47] | |
2017-07-21 | 2017-07-23 [48] | 2017 OO1 | 0.000852 AU (127,500 km; 79,200 mi) | 0.33 | 26–93 | 24.4 [49] | |
2017-08-14 | 2017-08-16 [50] | 2017 QP1 | 0.000419 AU (62,700 km; 38,900 mi) | 0.16 | 31–91 | 24.3 [51] | |
2017-08-20 | 2017-08-18 [52] | 2017 QN2 | 0.00145 AU (217,000 km; 135,000 mi) | 0.56 | 5–22 | 27.9 [53] | |
2017-09-03 | 2017-08-31 [54] | 2017 QB35 | 0.00238 AU (356,000 km; 221,000 mi) | 0.93 | 3–9 | 29.3 [55] | |
2017-09-14 | 2017-09-18 [56] | 2017 SQ2 | 0.00133 AU (199,000 km; 124,000 mi) | 0.52 | 14–49 | 25.8 [57] | |
2017-09-20 | 2017-09-17 [58] | 2017 SM2 | 0.00207 AU (310,000 km; 192,000 mi) | 0.81 | 6–26 | 27.3 [59] | |
2017-09-20 | 2017-09-21 [60] | 2017 SZ32 | 0.00137 AU (205,000 km; 127,000 mi) | 0.53 | 3–9 | 29.2 [61] | Yes |
2017-09-20 | 2017-09-20 [62] | 2017 SR2 | 0.000623 AU (93,200 km; 57,900 mi) | 0.24 | 4–12 | 28.5 [63] | |
2017-09-24 | 2017-09-25 [64] | 2017 SS12 | 0.00172 AU (257,000 km; 160,000 mi) | 0.67 | 8–27 | 27.0 [65] | Yes |
2017-09-30 | 2017-10-01 [66] | 2017 TQ2 | 0.000691 AU (103,400 km; 64,200 mi) | 0.27 | 3–8 | 29.4 [67] | |
2017-10-02 | 2017-09-29 [68] | 2017 SX17 | 0.00058 AU (87,000 km; 54,000 mi) | 0.23 | 4–16 | 28.1 [69] | |
2017-10-10 | 2017-10-14 [70] | 2017 TF5 | 0.00187 AU (280,000 km; 174,000 mi) | 0.73 | 20–95 | 24.7 [71] | |
2017-10-12 | 2012-10-04 [72] | 2012 TC4 | 0.000335 AU (50,100 km; 31,100 mi) | 0.13 [lower-alpha 4] | 10–31 | 26.7 [73] | |
2017-10-13 | 2017-10-21 [74] (Unconfirmed) | YT80190 | 0.000537 AU (80,300 km; 49,900 mi) | 0.21 [lower-alpha 5] | 2–6 | 30.4 | |
2017-10-15 | 2017-10-16 [75] | 2017 UF | 0.00255 AU (381,000 km; 237,000 mi) | 0.992 | 5–20 | 27.9 [76] | |
2017-10-16 | 2017-10-15 [77] | 2017 TH5 | 0.000668 AU (99,900 km; 62,100 mi) | 0.26 | 4–18 | 28.2 [78] | |
2017-10-17 | 2017-10-19 [79] | 2017 UR2 | 0.00213 AU (319,000 km; 198,000 mi) | 0.83 | 6–19 | 27.8 [80] | |
2017-10-19 | 2017-10-11 [81] | 2017 TD6 | 0.00128 AU (191,000 km; 119,000 mi) | 0.50 | 7–28 | 27.2 [82] | Yes |
2017-10-20 | 2017-10-21 [83] | 2017 UJ2 | 0.000120 AU (18,000 km; 11,200 mi) | 0.047 | 1–5 | 30.8 [84] | |
2017-10-21 | 2017-10-25 [85] | 2017 UA52 | 0.00132 AU (197,000 km; 123,000 mi) | 0.51 | 4–15 | 28.5 [86] | Yes |
2017-10-22 | 2017-10-30 [74] (Unconfirmed) | YU92F9B | 0.00121 AU (181,000 km; 112,000 mi) | 0.47 [lower-alpha 6] | 3–10 | 29.2 | |
2017-10-22 | 2017-10-30 [74] (Unconfirmed) | YU95BEF | 0.000130 AU (19,400 km; 12,100 mi) | 0.051 [lower-alpha 7] | 5–15 | 28.2 | |
2017-10-28 | 2017-10-27 [87] | 2017 UL6 | 0.000398 AU (59,500 km; 37,000 mi) | 0.16 | 1–3 | 32.0 [88] | |
2017-10-30 | 2017-10-29 [89] | 2017 UK8 | 0.00151 AU (226,000 km; 140,000 mi) | 0.59 | 4–17 | 28.3 [90] | |
2017-11-04 | 2017-11-05 [91] | 2017 VE | 0.00227 AU (340,000 km; 211,000 mi) | 0.88 | 10–31 | 26.6 [92] | |
2017-11-08 | 2017-11-16 [74] (Unconfirmed) | A104Vqx | 0.000222 AU (33,200 km; 20,600 mi) | 0.086 [lower-alpha 8] | 4–14 | 28.4 | |
2017-11-09 | 2017-11-10 [93] | 2017 VL2 | 0.000787 AU (117,700 km; 73,200 mi) | 0.31 | 13–42 | 26.1 [94] | |
2017-11-13 | 2017-11-15 [95] | 2017 VF14 | 0.00205 AU (307,000 km; 191,000 mi) | 0.80 | 4–14 | 28.5 [96] | |
2017-11-14 | 2017-11-20 [74] (Unconfirmed) | P10ELNY | 0.000212 AU (31,700 km; 19,700 mi) | 0.083 [lower-alpha 9] | 4–12 | 28.8 | |
2017-11-21 | 2017-11-20 [97] | 2017 WW1 | 0.000942 AU (140,900 km; 87,600 mi) | 0.37 | 3–7 | 29.7 [98] | |
2017-11-21 | 2017-11-22 [99] | 2017 WA14 | 0.000633 AU (94,700 km; 58,800 mi) | 0.25 | 6–26 | 27.5 [100] | |
2017-11-26 | 2017-11-26 [101] | 2017 WE30 | 0.000201 AU (30,100 km; 18,700 mi) | 0.078 | 1–3 | 31.9 [102] | |
2017-12-28 | 2017-12-25 [103] | 2017 YZ4 | 0.00149 AU (223,000 km; 139,000 mi) | 0.58 | 4–18 | 28.2 [104] | |
2017-12-30 | 2017-12-28 [105] | 2017 YE7 | 0.00206 AU (308,000 km; 191,000 mi) | 0.80 | 4–13 | 28.5 [106] |
This sub-section visualises the warning times of the close approaches listed in the above table, depending on the size of the asteroid. The sizes of the charts show the relative sizes of the asteroids to scale. For comparison, the approximate size of a person is also shown. This is based the absolute magnitude of each asteroid, an approximate measure of size based on brightness.
Abs Magnitude 30 and greater
(size of a person for comparison)
Abs Magnitude 29-30
Absolute Magnitude 28-29
Absolute Magnitude 27-28
Absolute Magnitude 26-27
Absolute Magnitude 25-26
Absolute Magnitude less than 25 (largest)
The number of asteroids listed here are significantly less than those of asteroids that approach Earth for several reasons. Asteroids that approach Earth not only move faster, but are brighter and are easier to detect with modern surveys because:
These factors severely limit the amount of Moon-approaching asteroids, to a level many times lower than the asteroids detected passing as close to Earth.
Date of closest approach | Object | Nominal lunocentric distance (AU) [lower-alpha 1] | Nominal lunocentric distance (LD) | Size (m) (approximate) | (H) | Approach distance to Earth (LD) |
---|---|---|---|---|---|---|
2017-01-25 | 2017 BA7 | 0.00187 AU (280,000 km; 174,000 mi) | 0.73 | 5–16 | 28.1 [107] | 1.12 |
2017-01-25 | 2017 BX | 0.00209 AU (313,000 km; 194,000 mi) | 0.81 | 5–18 | 28.0 [5] | 0.69 |
2017-01-30 | 2017 BH30 | 0.00187 AU (280,000 km; 174,000 mi) | 0.73 | 4–12 | 28.8 [7] | 0.13 |
2017-02-03 | 2017 BS32 | 0.00193 AU (289,000 km; 179,000 mi) | 0.75 | 7–24 | 27.3 [9] | 0.42 |
2017-02-24 | 2017 DG16 | 0.000555 AU (83,000 km; 51,600 mi) | 0.22 [lower-alpha 2] | 3–9 | 29.3 [11] | 0.36 |
2017-02-25 | 2017 DR34 | 0.00179 AU (268,000 km; 166,000 mi) | 0.70 | 3–11 | 29.1 [11] | 0.58 |
2017-03-02 | 2017 EA | 0.00224 AU (335,000 km; 208,000 mi) | 0.87 | 1–5 | 30.8 [15] | 0.054 |
2017-03-17 | 2017 FD3 | 0.00236 AU (353,000 km; 219,000 mi) | 0.92 | 6–20 | 27.7 [19] | 0.47 |
2017-03-17 | 2017 FW158 | 0.00104 AU (156,000 km; 97,000 mi) | 0.40 | 5–14 | 28.4 [21] | 0.32 |
2017-04-04 | 2017 GM | 0.00227 AU (340,000 km; 211,000 mi) | 0.88 | 2–7 | 29.9 [35] | 0.042 |
2017-04-21 | 2017 HG4 | 0.00177 AU (265,000 km; 165,000 mi) | 0.69 | 6–21 | 27.6 [39] | 0.61 |
2017-04-24 | 2017 HV2 | 0.00230 AU (344,000 km; 214,000 mi) | 0.90 | 3–12 | 28.9 [41] | 0.33 |
2017-05-02 | 2017 JA | 0.00251 AU (375,000 km; 233,000 mi) | 0.98 | 3–13 | 28.9 [43] | 0.26 |
2017-05-02 | 2017 JB2 | 0.00188 AU (281,000 km; 175,000 mi) | 0.73 | 3–11 | 29.0 [47] | 0.14 |
2017-05-03 | 2017 JQ1 | 0.00247 AU (370,000 km; 230,000 mi) | 0.96 | 3–9 | 29.4 [45] | 0.44 |
2017-05-31 | 2017 KW31 | 0.00114 AU (171,000 km; 106,000 mi) | 0.45 | 10–36 | 26.5 [108] | 1.23 |
2017-07-21 | 2017 OO1 | 0.00236 AU (353,000 km; 219,000 mi) | 0.92 | 25–90 | 24.5 [49] | 0.30 |
2017-08-14 | 2017 QP1 | 0.00230 AU (344,000 km; 214,000 mi) | 0.90 | 31–91 | 24.3 [51] | 0.16 |
2017-08-21 | 2017 QN2 | 0.00176 AU (263,000 km; 164,000 mi) | 0.69 | 5–22 | 27.9 [53] | 0.56 |
2017-08-26 | 2017 QQ17 | 0.00242 AU (362,000 km; 225,000 mi) | 0.94 | 4–17 | 28.3 [109] | 1.02 |
2017-09-03 | 2017 QB35 | 0.00245 AU (367,000 km; 228,000 mi) | 0.95 | 3–9 | 29.3 [55] | 0.93 |
2017-09-16 | 2017 RW17 | 0.00175 AU (262,000 km; 163,000 mi) | 0.68 | 2–7 | 29.8 [110] | 1.08 |
2017-09-20 | 2017 SZ32 | 0.00129 AU (193,000 km; 120,000 mi) | 0.50 | 3–9 | 29.2 [61] | 0.53 |
2017-09-20 | 2017 SM2 | 0.00213 AU (319,000 km; 198,000 mi) | 0.83 | 6–26 | 27.3 [59] | 0.81 |
2017-09-24 | 2017 SS12 | 0.000320 AU (47,900 km; 29,700 mi) | 0.12 | 8–27 | 27.0 [65] | 0.67 |
2017-09-30 | 2017 TQ2 | 0.00221 AU (331,000 km; 205,000 mi) | 0.86 | 3–8 | 29.4 [67] | 0.27 |
2017-10-02 | 2017 SX17 | 0.00174 AU (260,000 km; 162,000 mi) | 0.68 | 4–16 | 28.1 [69] | 0.22 |
2017-10-12 | 2012 TC4 | 0.00186 AU (278,000 km; 173,000 mi) | 0.72 | 10–31 | 26.7 [73] | 0.23 |
2017-10-13 | YT80190 | 0.00208 AU (311,000 km; 193,000 mi) | 0.81 [lower-alpha 3] | 2–6 | 30.4 | 0.21 |
2017-10-17 | 2017 TH5 | 0.00142 AU (212,000 km; 132,000 mi) | 0.55 | 4–18 | 28.2 [78] | 0.26 |
2017-10-20 | 2017 UJ2 | 0.00166 AU (248,000 km; 154,000 mi) | 0.65 | 1–5 | 30.8 [84] | 0.047 |
2017-10-20 | 2017 TD6 | 0.000756 AU (113,100 km; 70,300 mi) | 0.29 | 7–28 | 27.2 [82] | 0.50 |
2017-10-20 | 2017 UA52 | 0.000288 AU (43,100 km; 26,800 mi) | 0.11 [lower-alpha 4] | 4–15 | 28.3 [86] | 0.51 |
2017-10-22 | YU95BEF | 0.000481 AU (72,000 km; 44,700 mi) | 0.19 [lower-alpha 5] | 5–15 | 28.2 | 0.051 |
2017-10-24 | 2017 UK3 | 0.00207 AU (310,000 km; 192,000 mi) | 0.80 | 7–28 | 27.2 [111] | 1.38 |
2017-11-09 | 2017 VL2 | 0.00254 AU (380,000 km; 236,000 mi) | 0.990 | 13–42 | 26.1 [94] | 0.31 |
2017-11-09 | A104Vqx | 0.00204 AU (305,000 km; 190,000 mi) | 0.80 [lower-alpha 6] | 4–14 | 28.4 | 0.086 |
2017-11-13 | 2017 VF14 | 0.00243 AU (364,000 km; 226,000 mi) | 0.94 | 4–14 | 28.5 [96] | 0.80 |
2017-11-14 | P10ELNY | 0.00196 AU (293,000 km; 182,000 mi) | 0.76 [lower-alpha 7] | 4–12 | 28.8 | 0.083 |
2017-12-18 | 2017 YJ1 | 0.00142 AU (212,000 km; 132,000 mi) | 0.55 | 6–26 | 27.5 [112] | 1.044 |
2017-12-28 | 2017 YZ4 | 0.00175 AU (262,000 km; 163,000 mi) | 0.68 | 4–18 | 28.2 [104] | 0.58 |
An example list of near-Earth asteroids that passed or will pass more than 1 lunar distance (384,400 km or 0.00256 AU) from Earth in 2017.
Object | Size (meters) | Lunar distances | Date |
---|---|---|---|
2017 AP19 | 65 | 3.34 | 6 January 2017 |
2017 BJ30 [113] | 16 | 1.03 | 31 January 2017 |
2017 BQ6 | 186 | 6.57 | 7 February 2017 |
2017 DZ37 [114] | 7 | 1.005 | 23 February 2017 |
2017 DV36 [115] | 9 | 1.02 | 27 February 2017 |
1998 SL36 [116] | 313 | 8.34 | 16 March 2017 |
2017 FT102 [117] | 4 | 1.05 1.04 moon | 3 April 2017 |
2014 JO25 [118] | 823 | 4.57 | 19 April 2017 |
(418094) 2007 WV4 [119] | 890 | 7.96 | 1 June 2017 |
2017 KQ27 [120] | 30 | 1.02 1.34 moon | 6 June 2017 |
2017 MF [121] | 20 | 1.21 moon | 19 June 2017 |
2017 NT5 [122] | 110 | 1.11 1.27 moon | 14 July 2017 |
2006 SR131 [123] | 8 | 0.32 and 11 [ clarification needed ] | 17–28 September 2017 |
(496817) 1989 VB [124] | 394 | 7.88 | 29 September 2017 |
YT83F29 [ citation needed ] | 4 | 2.6 0.73 moon | 14 October 2017 |
(171576) 1999 VP11 [125] | 685 | 5.77 | 22 October 2017 |
(444584) 2006 UK [126] | 313 | 8.66 | 17 November 2017 |
month | <1 LD | <5 LD |
---|---|---|
January | 3 | 17 |
February | 3 | 27 |
March | 9 | 34 |
April | 5 | 28 |
May | 3 | 14 |
June | 0 | 10 |
July | 1 | 11 |
August | 2 | 17 |
September | 5 | 32 |
October | 14 | 52 |
November | 8 | 29 |
December | 2 | 28 |
Abs. mag | <1 LD | <5 LD |
---|---|---|
H <20 | 0 | 1 |
<21 | 0 | 0 |
<22 | 0 | 1 |
<23 | 0 | 3 |
<24 | 0 | 7 |
<25 | 3 | 19 |
<26 | 2 | 40 |
<27 | 4 | 74 |
<28 | 11 | 72 |
<29 | 18 | 57 |
<30 | 13 | 19 |
<31 | 4 | 5 |
<32 | 1 | 1 |
<33 | 1 | 1 |
Survey | <1 LD | <5 LD |
---|---|---|
408 – Mount Nyukasa Station | 0 | 1 |
703 – Catalina Sky Survey | 12 | 52 |
704 – Lincoln Laboratory ETS | 0 | 1 |
C51 – WISE | 0 | 1 |
F51 – Pan-STARRS 1 | 10 | 56 |
G45 – Space Surveillance Telescope | 0 | 3 |
G96 – Mt. Lemmon Survey | 28 | 157 |
I52 – Steward Observatory, Mount Lemmon | 0 | 1 |
J04 – ESA OGS | 0 | 1 |
K88 – GINOP-KHK | 0 | 1 |
T05 – ATLAS – Haleakala | 2 | 11 |
T08 – ATLAS – Mauna Loa | 5 | 15 |
Y00 – SONEAR | 0 | 2 |
List of asteroids with a Palermo Technical Impact Hazard Scale greater than −6 that are listed on the Sentry Risk Table because they have short observation arcs with poorly constrained orbits and have a chance of impacting Earth in 2017. Given a short observation arc, many different orbits fit the observed data. 2010 XB73 could have approached Earth around May 2017 or could have been 9 AU [127] from Earth on the way to a close approach with Saturn in 2018. A Palermo rating of −4 indicates an event that is 10,000 times less likely than the background hazard level of Earth impacts, which is defined as the average risk posed by objects of the same size or larger over the years until the date of the potential impact.
Date | Object | Estimated diameter (meters) | Obs arc (days) | Impact probability (1 in) | Palermo scale | JPL Horizons nominal geocentric distance (AU) | NEODyS nominal geocentric distance (AU) |
---|---|---|---|---|---|---|---|
2017-05-22 [128] | 2010 GZ60 | 2,000 [lower-alpha 1] | 1.3 | 830,000,000 | -1.83 | 0.4 AU (60,000,000 km; 37,000,000 mi) | Not listed |
2017-05-25 [129] | 2010 XB73 | 110 | 1.1 | 120,000,000 | -4.47 | 1.6 AU (240,000,000 km; 150,000,000 mi) | 9.0 AU (1.35×109 km; 840,000,000 mi) [127] |
2017-08-19 [130] | 2015 ME131 | 500 | 1.8 | 420,000,000 | -3.41 | 0.4 AU (60,000,000 km; 37,000,000 mi) | 0.4 AU (60,000,000 km; 37,000,000 mi) |
2017-09-18 [131] | 2015 HV182 | 157 | 0.9 | 7,700,000,000 | -5.78 | 2.3 AU (340,000,000 km; 210,000,000 mi) | 2.3 AU (340,000,000 km; 210,000,000 mi) |
2017-11-18 [132] | 2008 VS4 | 45 | 0.083 | 100,000,000 | -5.50 | 4.6 AU (690,000,000 km; 430,000,000 mi) | 3.9 AU (580,000,000 km; 360,000,000 mi) |
2017-11-29 [133] | 2007 YM | 20 | 0.13 | 2,000,000 | -5.21 | 5.1 AU (760,000,000 km; 470,000,000 mi) | 5.1 AU (760,000,000 km; 470,000,000 mi) |
2017-12-01 [128] | 2010 GZ60 | 2,000 [lower-alpha 1] | 1.3 | 10,000,000,000 | -3.62 | 1.0 AU (150,000,000 km; 93,000,000 mi) | Not listed |
2017-12-13 [134] | 2005 TM173 | 53 | 1.9 | 230,000,000 | -5.98 | 5.7 AU (850,000,000 km; 530,000,000 mi) | 5.7 AU (850,000,000 km; 530,000,000 mi) |
2017-12-20 [128] | 2010 GZ60 | 2,000 [lower-alpha 1] | 1.3 | 83,000,000 | -1.97 | 1.2 AU (180,000,000 km; 110,000,000 mi) | Not listed |
1994 WR12 is an asteroid and near-Earth object approximately 130 meters (430 feet) in diameter. As a member of the Aten group almost all of its orbit is closer to the Sun than Earth is. On 24 November 1994 it passed about 374100 km from the Moon. First imaged at Kitami Observatory on 26 November 1994, it was discovered two nights later by American astronomer Carolyn S. Shoemaker at Palomar Observatory on 28 November 1994. The asteroid then went unobserved from 1994 until it was recovered by Mauna Kea in March 2016. It was removed from the Sentry Risk Table on 2 April 2016.
(454101) 2013 BP73, provisional designation 2013 BP73, is a sub-kilometer asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 310 meters (1,020 ft) in diameter.
(523662) 2012 MU2, provisional designation 2012 MU2, is a sub-kilometer asteroid on an eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group. It was discovered on 18 June 2012 by astronomers of the Catalina Sky Survey at an apparent magnitude of 19.9 using a 0.68-meter (27 in) Schmidt–Cassegrain telescope. It has an estimated diameter of 240 meters (790 ft). The asteroid was listed on Sentry Risk Table with a Torino Scale rating of 1 on 23 June 2012.
(163132) 2002 CU11, provisional designation 2002 CU11, is a bright, sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group. Based on absolute magnitude, it is the second largest asteroid known to have passed closer than the Moon.
2014 OO6 (also written 2014 OO6) is an Apollo near-Earth asteroid discovered in 2014 and was the most dangerous one discovered in 2014 that remained on the Sentry Risk Table as of early December 2014. The asteroid is estimated to be roughly 75 meters (246 ft) in diameter and had a 1 in 83,000 chance of impacting Earth on 11 January 2051. However, the nominal best-fit orbit shows that 2014 OO6 will be 1.5 AU (220,000,000 km; 140,000,000 mi) from Earth on 11 January 2051.
2014 XL7 is a near-Earth object and Apollo asteroid, approximately 230 meters (750 feet) in diameter. It was the most dangerous potentially hazardous asteroid on Sentry Risk Table upon its discovery by the Mount Lemmon Survey in December 2014. At the time, the asteroid had a cumulative 1 in 83000 chance of impacting Earth on 4–5 June between the years 2048 and 2084. After the object's observation arc had been extended to 35 days, it was removed from the Sentry Risk Table on 15 January 2015. Since then the asteroid's orbit has been secured. Although it has an Earth minimum orbit intersection distance of less than one lunar distance, there are no projected close encounters with Earth in the foreseeable future, with its closest passage to occur in May 2046, still millions of kilometers away.
2012 TV is a near-Earth Apollo asteroid with an estimated diameter of 30 metres (98 ft). Its closest approach to the Earth was on October 7, 2012 with a distance of 0.0017 astronomical units. It also approached the Moon an hour earlier with a distance of 0.0028 astronomical units. With a short observation arc of 1.8 days, the asteroid is listed on the Sentry Risk Table and has a 1:500,000 chance of impacting Earth on April 2, 2081.
2013 TX68 is an Apollo asteroid and near-Earth object discovered on 6 October 2013 by the Catalina Sky Survey, during which it was near a close approach of 5.4 Lunar distances (LD) from the Earth. The asteroid only has a 10-day observation arc which makes long-term predictions of its position less certain. It was observed for three days as it approached Earth in the night sky starting with the sixth of October, 2013. Then it became unobservable by being between the Earth and the Sun, then not recovered due to its small size and dimness. Precovery images by Pan-STARRS from 29 September 2013 were announced on 11 February 2016 that extended the observation arc to 10 days. It was removed from the Sentry Risk Table on 11 February 2016, so there is no risk of impact from this object for the next hundred years or more. The asteroid was last observed on 9 October 2013.
2017 OO1 is a small asteroid, classified as near-Earth object of the Aten group, approximately 35–76 meters (115–249 feet) in diameter. It was first observed on 23 July 2017, by the robotic ATLAS survey at Mauna Loa Observatory, Hawaii, two days after the object had approached Earth at 0.33 lunar distances on 21 July 2017.
2017 XO2, also written 2017 XO2, is a sub-kilometer asteroid and near-Earth object of the Apollo group approximately 110 meters (360 feet) in diameter. The asteroid was discovered by Pan-STARRS in December 2017, after it already had approached Earth at 0.051 AU (7,600,000 km) or 20 lunar distances (LD) on 6 November 2017. On 26 April 2057, it will pass Earth at a similar distance of 21 LD again.
2010 WC9, unofficially designated ZJ99C60, is a sub-kilometer near-Earth asteroid of the Apollo group, approximately 100 meters (330 feet) in diameter. First observed for eleven days by the Catalina Sky Survey in 2010, the asteroid was recovered in May 2018 during its sub-lunar close encounter with Earth.
2018 XB4 (also written 2018 XB4) is an Apollo near-Earth asteroid roughly 53 meters (170 feet) in diameter. It was discovered on 13 December 2018 when the asteroid was about 0.125 AU (18,700,000 km; 11,600,000 mi) from Earth and had a solar elongation of 146°. It passed closest approach to Earth on 1 January 2019. Of the asteroids discovered in 2018, it had the highest Palermo scale rating at –3.6. In mid-2019 it was recovered which extended the observation arc to 177 days and was removed from the Sentry Risk Table on 12 June 2019. It is now known that on 22 June 2092 the asteroid will pass about 0.033±0.015 AU from Earth.
2020 LD is an Apollo near-Earth asteroid roughly 140 meters in diameter. It was discovered on 7 June 2020 when the asteroid was about 0.03 AU from Earth and had a solar elongation of 154 degrees. The glare of the Sun had masked the approach of the asteroid since November 2019. The asteroid passed closest approach to Earth on 5 June 2020 at a distance of 0.002 AU. The close approach distance is now known with an accuracy of roughly ± 1000 km. This is the largest asteroid to pass closer than the Moon this year and possibly the largest since (308635) 2005 YU55 in November 2011. The asteroid makes close approaches to Mercury, Venus, Earth, and Mars. It will be brighter than apparent magnitude 24 until 18 July 2020.
(458732) 2011 MD5 is an Apollo near-Earth asteroid around 1.2 kilometers (0.75 miles) in diameter. It is the largest asteroid known to have passed closer than the Moon. On 17 September 1918 the asteroid passed 0.00234 AU (350 thousand km; 0.91 LD) from Earth with a peak apparent magnitude of around 8.4. The 1918 close approach distance is known with an accuracy of roughly ±120 km. The asteroid had come to opposition (opposite the Sun in the sky) on 9 August 1918 at magnitude 16.
2016 NL56 (also written 2016 NL56) is a near-Earth object (NEO) and a potentially hazardous object (PHA), meaning that it has an orbit that can make close approaches to the Earth and large enough to cause significant regional damage in the event of impact. It is an Apollo asteroid, meaning that it is an Earth-crossing asteroid that has an orbit larger than the orbit of the Earth. It was first observed on 12 July 2016, when the asteroid was more than 1 AU from Earth and had a solar elongation of 163 degrees.
2020 XR is an Apollo near-Earth object and potentially hazardous asteroid roughly 390 meters in diameter. With a 5-day observation arc it was briefly listed as having a 1 in 11,000 chance of impacting Earth on 1 December 2028 placing it at the top of the Sentry Risk Table with a Palermo scale rating of -0.70.
2020 AP1 is an Apollo near-Earth object roughly 5 meters (20 feet) in diameter. On 2 January 2020 it passed 0.00218 AU (326 thousand km; 0.85 LD) from Earth. With a short 1-day observation arc it was roughly expected to pass about 0.01 AU (1.5 million km; 3.9 LD) from Earth on 7 January 2022, but with an uncertainty of ±8 days for the close approach date it could have passed significantly closer or further.
2021 UA1 is a small (~2 meter) near-Earth object that passed about 3047 km from the surface of Earth while passing over Antarctica on 25 October 2021 around 03:07 UT. Given the small size of the asteroid it only reached the brightness of Pluto at around apparent magnitude 14. Since it approached from the direction of the Sun, it was not discovered until 4 hours after closest approach.
2022 QX4 is a Tunguska event-sized asteroid, classified as a near-Earth object of the Aten group, approximately 40 meters (130 feet) in diameter. It was discovered by ATLAS on 24 August 2022, when it was 0.03 AU (4.5 million km) from Earth. On 4 September 2022 with an observation arc of 8 days, it was listed with a 1-in-109 chance of impacting Earth with a Torino scale of 1 for a virtual impactor on 4 September 2068 00:52 UTC. Five precovery images from August 2013 were published on 11 September 2022 extending the observation arc to 9 years and 2022 QX4 was removed from the Sentry Risk Table. The nominal approach is expected to occur 26 August 2068.