Where is it now
- Distance from Sun
- 0.938 AU
- True anomaly
- 265.55°
- Distance from Earth
- 1.043 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
- 10h 18m 22s
- Declination
- +01° 25′ 36″
- Constellation
- Sextans
- Distance from Earth
- 1.04 AU
- Elongation from the Sun
- 54.61° — 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.
Your location stays in your browser and is sent only for this calculation. Using a what3words address is optional; if you do, the three words go to what3words to be converted and we don't record them. Set a location first, then you can save an email alert for this object. See our privacy policy.
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
- 0.959 AU
- Eccentricity
- 0.1906
- Inclination
- 11.26°
- Orbital period
- 343.1 days
- Perihelion
- 0.776 AU
- Aphelion
- 1.142 AU
- Longitude of ascending node
- 218.04°
- Argument of periapsis
- 331.11°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 37.4 LD
- 0.0961 AU
- Tisserand (Jupiter)
- 6.252
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 48
- Data arc
- 413 days
- First observed
- 2 October 2022
- Last observed
- 19 November 2023
- Residual RMS
- 0.49 ″
- Solution · Otto Matic
- 19 November 2023
Visual & observation
- Absolute magnitude (H)
- 23.71
Discovery & classification
Close approaches 136 on record
Top-down view of the ecliptic, Earth at the centre, for the 2036-08-11 05:58 UTC close approach of 2022 TU. Catalogue miss distance 167.1 LD · 6.42 × 10⁷ km. The curve is the geocentric path from 2036-08-08 to 2036-08-14, 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. At closest approach the object is north 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 |
|---|---|---|---|---|
| 2030-10-31 15:28:00 | Venus | 0.1484 AU | 57.8 LD | 8.8 km/s |
| 2032-09-01 12:23:00 | Venus | 0.1307 AU | 50.9 LD | 11.2 km/s |
| 2036-08-11 05:58:00 | Earth | 0.4293 AU | 167.1 LD | 17 km/s |
| 2037-07-11 13:22:00 | Earth | 0.1949 AU | 75.8 LD | 7.1 km/s |
| 2038-04-26 16:24:00 | Earth | 0.2168 AU | 84.4 LD | 9.3 km/s |
| 2038-10-29 23:56:00 | Earth | 0.1316 AU | 51.2 LD | 7 km/s |
| 2039-02-13 20:58:00 | Earth | 0.2429 AU | 94.5 LD | 6.2 km/s |
| 2039-11-28 14:35:00 | Earth | 0.2229 AU | 86.7 LD | 12 km/s |
| 2048-08-31 22:15:00 | Venus | 0.1058 AU | 41.2 LD | 8.7 km/s |
| 2052-08-01 17:10:00 | Earth | 0.28 AU | 109.0 LD | 11.6 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