Where is it now
- Distance from Sun
- 0.92 AU
- True anomaly
- 251.44°
- Distance from Earth
- 1.468 AU
- As of
- 20 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
- 11h 16m 54s
- Declination
- -00° 41′ 01″
- Constellation
- Leo
- Distance from Earth
- 1.47 AU
- Elongation from the Sun
- 38° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
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
- 0.898 AU
- Eccentricity
- 0.2139
- Inclination
- 8.92°
- Orbital period
- 310.8 days
- Perihelion
- 0.706 AU
- Aphelion
- 1.09 AU
- Longitude of ascending node
- 189.6°
- Argument of periapsis
- 46.1°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.2 LD
- 0.003 AU
- Tisserand (Jupiter)
- 6.596
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 6
- Data arc
- 2 days
- First observed
- 3 October 2018
- Last observed
- 5 October 2018
- Residual RMS
- 0.38 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 28.18
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 31 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-10-11 14:34 UTC close approach of 2018 TS6. Catalogue miss distance 158.5 LD · 6.09 × 10⁷ km. The curve is the geocentric path from 2029-10-08 to 2029-10-14, 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. 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 |
|---|---|---|---|---|
| 2029-10-11 14:34:00 | Earth | 0.4073 AU | 158.5 LD | 19.2 km/s |
| 2031-01-15 12:08:00 | Earth | 0.182 AU | 70.8 LD | 9.9 km/s |
| 2035-10-03 12:38:00 | Earth | 0.1521 AU | 59.2 LD | 11.6 km/s |
| 2036-04-22 03:52:00 | Venus | 0.1481 AU | 57.6 LD | 13.5 km/s |
| 2037-01-02 10:22:00 | Earth | 0.397 AU | 154.5 LD | 17.9 km/s |
| 2048-01-26 14:52:00 | Earth | 0.1473 AU | 57.3 LD | 6.3 km/s |
| 2052-10-06 13:15:00 | Earth | 0.2734 AU | 106.4 LD | 15.2 km/s |
| 2053-05-22 01:46:00 | Earth | 0.3231 AU | 125.7 LD | 10.2 km/s |
| 2054-01-08 08:49:00 | Earth | 0.2876 AU | 111.9 LD | 14.1 km/s |
| 2054-03-17 12:24:00 | Venus | 0.0678 AU | 26.4 LD | 7.7 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