Where is it now
- Distance from Sun
- 1.087 AU
- True anomaly
- 189.89°
- Distance from Earth
- 0.736 AU
- As of
- 19 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
- 18h 53m 07s
- Declination
- -16° 56′ 37″
- Constellation
- Sagittarius
- Distance from Earth
- 0.74 AU
- Elongation from the Sun
- 75.99° — well clear of the Sun
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
- 0.849 AU
- Eccentricity
- 0.2871
- Inclination
- 7.64°
- Orbital period
- 285.9 days
- Perihelion
- 0.605 AU
- Aphelion
- 1.093 AU
- Longitude of ascending node
- 197.29°
- Argument of periapsis
- 318.03°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.7 LD
- 0.0043 AU
- Tisserand (Jupiter)
- 6.894
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 34
- Data arc
- 5 days
- First observed
- 4 October 2023
- Last observed
- 9 October 2023
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 11 October 2023
Visual & observation
- Absolute magnitude (H)
- 27.28
Discovery & classification
Close approaches 26 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-02-26 12:26 UTC close approach of 2023 TW. Catalogue miss distance 151.8 LD · 5.84 × 10⁷ km. The curve is the geocentric path from 2027-02-23 to 2027-03-01, 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 |
|---|---|---|---|---|
| 2027-02-26 12:26:00 | Earth | 0.3901 AU | 151.8 LD | 13.8 km/s |
| 2029-07-27 10:11:00 | Venus | 0.0842 AU | 32.8 LD | 8.8 km/s |
| 2030-08-09 22:28:00 | Earth | 0.1335 AU | 52.0 LD | 6.1 km/s |
| 2030-12-12 08:18:00 | Earth | 0.293 AU | 114.0 LD | 6.2 km/s |
| 2034-03-30 07:12:00 | Earth | 0.3686 AU | 143.4 LD | 12.8 km/s |
| 2034-10-06 05:40:00 | Earth | 0.2436 AU | 94.8 LD | 14.9 km/s |
| 2034-11-15 02:58:00 | Venus | 0.1309 AU | 50.9 LD | 15 km/s |
| 2037-07-22 17:15:00 | Earth | 0.2288 AU | 89.0 LD | 12.6 km/s |
| 2038-01-24 05:45:00 | Earth | 0.3722 AU | 144.8 LD | 11.9 km/s |
| 2038-02-28 08:42:00 | Venus | 0.1095 AU | 42.6 LD | 8.8 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