Where is it now
- Distance from Sun
- 1.188 AU
- True anomaly
- 192.33°
- Distance from Earth
- 1.117 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
- 09h 36m 17s
- Declination
- +15° 21′ 32″
- Constellation
- Leo
- Distance from Earth
- 1.12 AU
- Elongation from the Sun
- 68.24° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.943 AU
- Eccentricity
- 0.2701
- Inclination
- 1.04°
- Orbital period
- 334.7 days
- Perihelion
- 0.689 AU
- Aphelion
- 1.198 AU
- Longitude of ascending node
- 21.48°
- Argument of periapsis
- 236.3°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.7 LD
- 0.0019 AU
- Tisserand (Jupiter)
- 6.335
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 22
- Data arc
- 2 days
- First observed
- 10 October 2023
- Last observed
- 12 October 2023
- Residual RMS
- 0.39 ″
- Solution · Otto Matic
- 13 October 2023
Visual & observation
- Absolute magnitude (H)
- 29.16
Discovery & classification
Close approaches 172 on record
Top-down view of the ecliptic, Earth at the centre, for the 2034-10-09 14:31 UTC close approach of 2023 TX6. Catalogue miss distance 18.9 LD · 7.25 × 10⁶ km. The curve is the geocentric path from 2034-10-06 to 2034-10-12, 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 |
|---|---|---|---|---|
| 2027-04-11 16:01:00 | Venus | 0.025 AU | 9.7 LD | 7.7 km/s |
| 2029-01-30 15:04:00 | Venus | 0.0292 AU | 11.4 LD | 5.9 km/s |
| 2030-11-11 05:19:00 | Venus | 0.0361 AU | 14.1 LD | 5.9 km/s |
| 2032-08-29 13:19:00 | Venus | 0.0377 AU | 14.7 LD | 7.8 km/s |
| 2034-06-26 22:10:00 | Venus | 0.1132 AU | 44.1 LD | 12 km/s |
| 2034-10-09 14:31:00 | Earth | 0.0485 AU | 18.9 LD | 9.8 km/s |
| 2035-07-10 17:58:00 | Earth | 0.3082 AU | 119.9 LD | 10 km/s |
| 2035-12-19 00:15:00 | Earth | 0.2124 AU | 82.7 LD | 7 km/s |
| 2036-04-26 20:33:00 | Earth | 0.2831 AU | 110.2 LD | 8.9 km/s |
| 2037-02-07 21:49:00 | Earth | 0.1521 AU | 59.2 LD | 13 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