Where is it now
- Distance from Sun
- 1.227 AU
- True anomaly
- 155.99°
- Distance from Earth
- 1.481 AU
- As of
- 22 October 2026
Two-body Kepler propagation — accurate to ~0.1% for major planets over decades, less so for highly-perturbed bodies. Use JPL Horizons for high precision.
In the sky
- Right ascension
- 17h 35m 07s
- Declination
- -31° 01′ 36″
- Constellation
- Scorpius
- Distance from Earth
- 1.48 AU
- Elongation from the Sun
- 55.19° — near the Sun — look low at dusk or dawn
Favours the southern hemisphere; low or below the horizon from far north.
From your location
See how high it is right now, whether it is up after civil twilight, and when it rises and sets where you are.
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Two-body approximation, good to about a degree for the planets — enough to find the constellation and know whether it is up.
Orbital elements
- Semi-major axis
- 0.952 AU
- Eccentricity
- 0.3488
- Inclination
- 10.28°
- Orbital period
- 339.1 days
- Perihelion
- 0.62 AU
- Aphelion
- 1.284 AU
- Longitude of ascending node
- 11.68°
- Argument of periapsis
- 138.48°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 22.9 LD
- 0.0588 AU
- Tisserand (Jupiter)
- 6.257
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 27
- Data arc
- 12 days
- First observed
- 6 October 2018
- Last observed
- 18 October 2018
- Residual RMS
- 0.3 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.8
Discovery & classification
Close approaches 89 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-07-01 08:10 UTC close approach of 2018 TJ3. Catalogue miss distance 138.6 LD · 5.33 × 10⁷ km. The curve is the geocentric path from 2028-06-28 to 2028-07-04, with a mark at UTC midnights and an arrow for the direction of motion. The circle is the Moon’s mean orbit; the Moon is plotted at closest approach. A ray shows the Sun’s direction. The labelled distance is the full separation. The drawn radius is the part that lies in the ecliptic plane. At closest approach the object is south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2028-07-01 08:10:00 | Earth | 0.3562 AU | 138.6 LD | 19.6 km/s |
| 2029-06-01 03:54:00 | Earth | 0.2097 AU | 81.6 LD | 7.8 km/s |
| 2030-03-19 05:02:00 | Earth | 0.3573 AU | 139.0 LD | 14.1 km/s |
| 2030-09-02 01:18:00 | Earth | 0.2966 AU | 115.4 LD | 9 km/s |
| 2031-01-23 20:34:00 | Earth | 0.3709 AU | 144.3 LD | 12.9 km/s |
| 2031-10-21 17:39:00 | Earth | 0.08 AU | 31.1 LD | 9.6 km/s |
| 2032-10-11 01:12:00 | Earth | 0.3769 AU | 146.7 LD | 21.8 km/s |
| 2041-07-02 01:50:00 | Earth | 0.3655 AU | 142.3 LD | 19.9 km/s |
| 2043-03-21 10:38:00 | Earth | 0.3544 AU | 137.9 LD | 14 km/s |
| 2043-08-31 10:10:00 | Earth | 0.2994 AU | 116.5 LD | 9 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB