| Designat. | NEAT name & Image | Disc. with NEAT/ | Date | Vel. (deg/day) | Mag. | Size in km (miles) | Orbit Visual. | Comment* |
| 1999 JE1 | RBURI4A | Palomar | 5 May | 1.3 | 19 | - | - | Apollo, not discovered with NEAT |
| 2002 JA9 | RBVMXJB | Palomar | 5 May | 0.4 | 20 | 0.7 (0.4) | orbit | Amor |
| 2002 GY9 | RC8J4TB | Palomar | 6 May | 0.8 | 19 | - | - | Not NEA |
| 2002 JQ97 | RDAC5UB | Palomar | 9 May | 0.3 | 20 | 0.1 (0.06) | orbit | Amor |
| C/2002 J4 (NEAT) | RESEKDB | Palomar | 13 May | 0.1 | 18 | - | orbit | Comet NEAT-IAUC 7899-has a parabolic orbit with perihelion between Mars and Jupiter. |
| 2002 JR100 | RF4VNRC | Palomar | 14 May | 1.6 | 20 | 0.09 (0.05) | orbit | Aten |
| 2002 KR | RFRGBVC | Palomar | 16 May | 0.4 | 20 | Not NEA | ||
| C/2002 K1 (NEAT) | RFWI14 | MSSS | 16 May | 0.3 | 20 | - | orbit | Comet-IAUC 7902--has a parabolic orbit with perihelion between Mars and Jupiter. The orbit is nearly perpendicular to the ecliptic. |
| - | RFWPDB | MSSS | 16 May | 0.1 | 20 | - | - | Not real or lost |
| 2002 KJ9 | RFWPMA | MSSS | 16 May | 0.7 | 21 | - | - | Not NEA |
| 2002 KJ3 | RGI8YUC | Palomar | 18 May | 0.4 | 20 | 0.7 (0.4) | orbit | Amor |
| 2002 KJ8 | RGICO0C | Palomar | 18 May | 0.2 | 21 | 0.4 (0.2) | orbit | Not NEA-high eccentricity, Mars crossing asteroid |
| 2002 KD4 | RGL8LIC | Palomar | 18 May | 0.1 | 20 | - | - | Not NEA |
| - | RGLBTBC | Palomar | 18 May | 0.3 | 21 | - | - | Lost or not real |
| 2002 KL6 | RJTH11 | MSSS | 27 May | 1.4 | 17 | 1.5 (0.9) | orbit | Amor-large |
| C/2002 K4 (NEAT) | RJUK0O | MSSS | 27 May | 0.4 | 18 | - | orbit | Comet-IAUC 7909--has a parabolic orbit with perihelion between Mars and Jupiter. The orbit is nearly perpendicular to the ecliptic. |
| - | RK3KETA | Palomar | 28 May | 0.5 | 18 | - | - | Not real or lost |
| - | RK80Q5 | MSSS | 28 May | 0.1 | 20 | - | - | Not real or lost |
| - | RKTYI6B | Palomar | 30 May | 2.8 | 19 | - | - | Lost or not real |
*Amors, Apollos, and Atens are the three categories of Near-Earth asteroids (NEAs). Amor asteroids approach the Earth's orbit from the outside, Apollo asteroids cross the Earth's orbit, and Aten asteroids approach the Earth's orbit from the inside. Potentially Hazardous asteroids (PHAs) are larger than ~200 m (0.1 mile) and approach close enough to present a potential hazard but not a current hazard.
